This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_UMi-02-Q1b1x1_231918_TTUQ1b1x1_1257846_KU7UCfPg
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.47 13:21:36.40 +71:58:07.4
119.63998 44.96620 galactic UMi Second-epoch detections are separated by 1.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:36.40 +71:58:07.4 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:36.40 +71:58:07.4: 13.64 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:36.40 +71:58:07.4: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.48 13:32:08.94 +71:25:13.3
118.33742 45.34296 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687093051137050496 | 13:32:08.86 +71:25:13.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.634+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:08.94 +71:25:13.3: 10.53 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:08.94 +71:25:13.3: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.54 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687093051137050496,2461335.6793,9.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687093051137050496 20261022.1793 9.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.52 13:14:17.41 +72:12:56.4
120.47590 44.80345 galactic UMi Second-epoch detections are separated by 1.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:14:17.41 +72:12:56.4 (user input) | T | P | (position from user input) J-Ks=0.629+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:17.41 +72:12:56.4: 13.66 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:17.41 +72:12:56.4: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.46 13:19:33.78 +71:55:20.3
119.85057 45.03730 galactic UMi Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687839207215466240 | 13:19:33.87 +71:55:20.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.207+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:33.78 +71:55:20.3: 10.67 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:33.78 +71:55:20.3: 10.66 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.67 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687839207215466240,2461335.6793,9.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687839207215466240 20261022.1793 9.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.65 13:20:10.61 +71:38:59.2
119.72299 45.29899 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687782028315359872 | 13:20:10.60 +71:38:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.160+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:20:10.61 +71:38:59.2: 10.79 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:20:10.61 +71:38:59.2: 10.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.78 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687782028315359872,2461335.6793,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687782028315359872 20261022.1793 9.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.74 13:32:39.82 +72:03:58.1
118.48639 44.70455 galactic UMi Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687140879892893568 | 13:32:39.77 +72:03:58.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956PMcCO..13a....B AG+72 358 J-Ks=0.335+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:39.82 +72:03:58.1: 10.81 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:39.82 +72:03:58.1: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.81 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687140879892893568,2461335.6793,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687140879892893568 20261022.1793 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.67 13:13:30.12 +72:30:27.1
120.60945 44.52109 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688150609524344192 | 13:13:30.19 +72:30:26.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.268+/-0.036 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:13:30.12 +72:30:27.1: 10.86 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:13:30.12 +72:30:27.1: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688150609524344192,2461335.6793,9.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688150609524344192 20261022.1793 9.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.84 13:35:06.68 +71:37:16.2
118.07914 45.09332 galactic UMi Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687078035931363072 | 13:35:06.83 +71:37:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.410+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:35:06.68 +71:37:16.2: 10.93 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:35:06.68 +71:37:16.2: 10.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687078035931363072,2461335.6793,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687078035931363072 20261022.1793 9.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.95 13:28:50.89 +72:13:38.2
118.93641 44.60961 galactic UMi Second-epoch detections are separated by 0.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687908751325829376 | 13:28:50.85 +72:13:38.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.275+/-0.032 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:50.89 +72:13:38.2: 11.16 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:50.89 +72:13:38.2: 11.15 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687908751325829376,2461335.6793,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687908751325829376 20261022.1793 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.81 15:37:01.65 +65:32:17.8
100.65621 43.74928 galactic Dra Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1641418479126045440 | 15:37:01.70 +65:32:17.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.612+/-0.025 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:37:01.65 +65:32:17.8: 11.27 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:37:01.65 +65:32:17.8: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.28 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1641418479126045440,2461335.6793,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1641418479126045440 20261022.1793 9.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.12 13:40:12.72 +71:01:57.3
117.30511 45.55906 galactic UMi Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686836624409544960 | 13:40:12.84 +71:01:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.641+/-0.025 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:40:12.72 +71:01:57.3: 11.30 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:40:12.72 +71:01:57.3: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686836624409544960,2461335.6793,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686836624409544960 20261022.1793 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.98 13:16:09.04 +71:42:06.3
120.17882 45.29417 galactic UMi Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687809589120291968 | 13:16:09.10 +71:42:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.185+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:16:09.04 +71:42:06.3: 11.30 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:16:09.04 +71:42:06.3: 11.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687809589120291968,2461335.6793,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687809589120291968 20261022.1793 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.24 13:39:59.05 +71:25:10.6
117.47735 45.19098 galactic UMi Second-epoch detections are separated by 0.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686870606190812288 | 13:39:59.10 +71:25:10.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.286+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:39:59.05 +71:25:10.6: 11.39 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:39:59.05 +71:25:10.6: 11.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.39 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686870606190812288,2461335.6793,10.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686870606190812288 20261022.1793 10.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.21 13:39:22.44 +71:07:42.1
117.43493 45.48481 galactic UMi Second-epoch detections are separated by 0.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686842259406642816 | 13:39:22.59 +71:07:42.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.310+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:39:22.44 +71:07:42.1: 11.43 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:39:22.44 +71:07:42.1: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686842259406642816,2461335.6793,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686842259406642816 20261022.1793 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.29 13:32:34.71 +72:01:22.6
118.48178 44.74812 galactic UMi Second-epoch detections are separated by 1.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687140295777337856 | 13:32:34.66 +72:01:23.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.644+/-0.034 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:34.71 +72:01:22.6: 11.52 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:34.71 +72:01:22.6: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687140295777337856,2461335.6793,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687140295777337856 20261022.1793 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.21 13:19:56.41 +71:30:15.9
119.71662 45.44548 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687757053081005952 | 13:19:56.45 +71:30:15.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.624+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:56.41 +71:30:15.9: 11.54 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:56.41 +71:30:15.9: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687757053081005952,2461335.6793,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687757053081005952 20261022.1793 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.67 13:35:24.95 +72:17:30.1
118.27189 44.43648 galactic UMi Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687523028902909440 | 13:35:24.85 +72:17:29.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.660+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:35:24.95 +72:17:30.1: 11.57 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:35:24.95 +72:17:30.1: 11.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687523028902909440,2461335.6793,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687523028902909440 20261022.1793 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.39 13:35:29.66 +71:23:40.1
117.96001 45.30607 galactic UMi Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687048933232956160 | 13:35:29.65 +71:23:40.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.696+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:35:29.66 +71:23:40.1: 11.71 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:35:29.66 +71:23:40.1: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687048933232956160,2461335.6793,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687048933232956160 20261022.1793 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.41 13:28:43.51 +71:22:13.7
118.70200 45.45030 galactic UMi Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687001929110837760 | 13:28:43.41 +71:22:13.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.270+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:43.51 +71:22:13.7: 11.71 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:43.51 +71:22:13.7: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687001929110837760,2461335.6793,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687001929110837760 20261022.1793 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.91 13:34:39.39 +70:31:39.6
117.75532 46.16375 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686891187673980544 | 13:34:39.49 +70:31:39.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:34:39.39 +70:31:39.6: 11.78 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:34:39.39 +70:31:39.6: 11.77 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686891187673980544,2461335.6793,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686891187673980544 20261022.1793 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.57 13:36:35.78 +71:56:58.8
118.03243 44.74650 galactic UMi Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687464544332900864 | 13:36:35.86 +71:56:59.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.380+/-0.025 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:36:35.78 +71:56:58.8: 11.79 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:36:35.78 +71:56:58.8: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687464544332900864,2461335.6793,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687464544332900864 20261022.1793 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.71 13:25:33.26 +70:55:51.6
118.93706 45.93171 galactic UMi Second-epoch detections are separated by 1.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686971447727647232 | 13:25:33.26 +70:55:51.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.336+/-0.027 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:33.26 +70:55:51.6: 11.97 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:33.26 +70:55:51.6: 11.99 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686971447727647232,2461335.6793,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686971447727647232 20261022.1793 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.62 13:34:40.95 +71:34:31.7
118.11033 45.14575 galactic UMi Second-epoch detections are separated by 0.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1687077520535284992 | 13:34:40.92 +71:34:31.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.356+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:34:40.95 +71:34:31.7: 12.04 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:34:40.95 +71:34:31.7: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1687077520535284992,2461335.6793,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1687077520535284992 20261022.1793 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.44 15:34:06.07 +65:42:32.3
101.09333 43.89365 galactic UMi Second-epoch detections are separated by 0.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644436187571600256 | 15:34:06.07 +65:42:32.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.593+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:34:06.07 +65:42:32.3: 12.08 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:34:06.07 +65:42:32.3: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644436187571600256,2461335.6793,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644436187571600256 20261022.1793 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.89 13:32:41.35 +70:58:12.1
118.13145 45.77180 galactic UMi Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686942207589980672 | 13:32:41.38 +70:58:12.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.398+/-0.027 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:41.35 +70:58:12.1: 12.18 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:41.35 +70:58:12.1: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686942207589980672,2461335.6793,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686942207589980672 20261022.1793 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.64 13:27:33.94 +71:46:45.9
118.94664 45.06823 galactic UMi Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687116686341184768 | 13:27:37.76 +71:47:19.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:33.94 +71:46:45.9: 12.24 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:33.94 +71:46:45.9: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687116686341184768,2461335.6793,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687116686341184768 20261022.1793 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.21 13:25:31.63 +70:40:09.0
118.86847 46.18919 galactic UMi Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1685453984242018944 | 13:25:31.70 +70:40:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.333+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:31.63 +70:40:09.0: 12.32 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:31.63 +70:40:09.0: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1685453984242018944,2461335.6793,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1685453984242018944 20261022.1793 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.21 13:39:16.57 +70:16:48.5
117.12283 46.30479 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686705159754752896 | 13:39:16.58 +70:16:48.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.586+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:39:16.57 +70:16:48.5: 12.34 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:39:16.57 +70:16:48.5: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686705159754752896,2461335.6793,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686705159754752896 20261022.1793 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.02 13:23:20.53 +72:39:07.6
119.61947 44.27037 galactic UMi Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687979699889782016 | 13:23:20.50 +72:39:08.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.313+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:20.53 +72:39:07.6: 12.39 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:20.53 +72:39:07.6: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687979699889782016,2461335.6793,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687979699889782016 20261022.1793 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.70 15:36:58.16 +65:28:47.1
100.59501 43.78812 galactic Dra Second-epoch detections are separated by 2.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1641417306599228928 | 15:36:58.16 +65:28:47.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.535+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:36:58.16 +65:28:47.1: 12.49 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:36:58.16 +65:28:47.1: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1641417306599228928,2461335.6793,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1641417306599228928 20261022.1793 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.10 13:38:08.95 +71:03:09.2
117.54352 45.58385 galactic UMi Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686835211364474624 | 13:38:09.06 +71:03:09.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.483+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:38:08.95 +71:03:09.2: 12.59 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:38:08.95 +71:03:09.2: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686835211364474624,2461335.6793,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686835211364474624 20261022.1793 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.22 13:38:35.67 +71:01:20.0
117.48236 45.60379 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:38:35.67 +71:01:20.0 (user input) | T | P | (position from user input) J-Ks=0.215+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:38:35.67 +71:01:20.0: 12.61 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:38:35.67 +71:01:20.0: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.03 13:28:02.22 +71:33:15.8
118.83145 45.28134 galactic UMi Second-epoch detections are separated by 1.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687109642594825600 | 13:28:02.24 +71:33:16.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.682+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:02.22 +71:33:15.8: 12.73 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:02.22 +71:33:15.8: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687109642594825600,2461335.6793,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687109642594825600 20261022.1793 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.49 13:28:23.57 +70:39:09.1
118.52791 46.15843 galactic UMi Second-epoch detections are separated by 2.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:28:23.57 +70:39:09.1 (user input) | T | P | (position from user input) J-Ks=0.297+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:23.57 +70:39:09.1: 12.78 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:23.57 +70:39:09.1: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.20 13:22:58.81 +71:33:49.3
119.39251 45.34717 galactic UMi Second-epoch detections are separated by 1.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:22:58.81 +71:33:49.3 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:22:58.81 +71:33:49.3: 13.08 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:22:58.81 +71:33:49.3: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.55 13:29:09.79 +72:14:06.7
118.90563 44.59695 galactic UMi Second-epoch detections are separated by 3.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:29:09.79 +72:14:06.7 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:29:09.79 +72:14:06.7: 13.24 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:29:09.79 +72:14:06.7: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.63 13:37:40.30 +71:23:59.4
117.72278 45.25789 galactic UMi Second-epoch detections are separated by 2.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:37:40.30 +71:23:59.4 (user input) | T | P | (position from user input) J-Ks=0.275+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:37:40.30 +71:23:59.4: 13.40 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:37:40.30 +71:23:59.4: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.56 13:36:41.40 +71:23:59.0
117.83042 45.27763 galactic UMi Second-epoch detections are separated by 2.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:36:41.40 +71:23:59.0 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:36:41.40 +71:23:59.0: 13.44 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:36:41.40 +71:23:59.0: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.61 13:35:24.47 +71:05:40.9
117.86614 45.59861 galactic UMi Second-epoch detections are separated by 1.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:35:24.47 +71:05:40.9 (user input) | T | P | (position from user input) J-Ks=0.597+/-0.034 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:35:24.47 +71:05:40.9: 13.50 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:35:24.47 +71:05:40.9: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.53 12:51:17.47 +73:31:33.0
122.94629 43.60241 galactic Dra Second-epoch detections are separated by 1.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:51:17.47 +73:31:33.0 (user input) | T | P | (position from user input) J-Ks=0.785+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:51:17.47 +73:31:33.0: 13.51 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:51:17.47 +73:31:33.0: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.46 13:15:56.81 +72:02:25.8
120.26600 44.96067 galactic UMi Second-epoch detections are separated by 2.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:56.81 +72:02:25.8 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:56.81 +72:02:25.8: 13.51 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:56.81 +72:02:25.8: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.62 13:41:41.88 +71:05:34.0
117.16294 45.46832 galactic UMi Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:41:41.88 +71:05:34.0 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:41:41.88 +71:05:34.0: 13.50 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:41:41.88 +71:05:34.0: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.49 12:47:50.85 +72:59:34.6
123.29770 44.13276 galactic Dra Second-epoch detections are separated by 1.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:47:50.85 +72:59:34.6 (user input) | T | P | (position from user input) J-Ks=0.354+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:47:50.85 +72:59:34.6: 13.50 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:47:50.85 +72:59:34.6: 13.54 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.40 13:16:27.07 +71:56:08.2
120.19123 45.05930 galactic UMi Second-epoch detections are separated by 1.7" and 7.4 pix
The object was found in VSX 1" Gaia DR3 1687847900229274240
Type: ROT
# Max. Min./Amp. JD0 Period
13.190 G 13.230 G G
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:16:27.07 +71:56:08.2: 13.50 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:16:27.07 +71:56:08.2: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687847900229274240,2461335.6793,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687847900229274240 20261022.1793 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.53 12:50:18.37 +72:36:12.5
123.05057 44.52452 galactic Dra Second-epoch detections are separated by 1.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:50:18.37 +72:36:12.5 (user input) | T | P | (position from user input) J-Ks=0.621+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:50:18.37 +72:36:12.5: 13.48 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:50:18.37 +72:36:12.5: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.70 13:21:30.41 +71:27:07.9
119.52953 45.47689 galactic UMi Second-epoch detections are separated by 2.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:30.41 +71:27:07.9 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:30.41 +71:27:07.9: 13.47 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:30.41 +71:27:07.9: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.76 13:13:50.51 +71:48:33.2
120.45315 45.21105 galactic UMi Second-epoch detections are separated by 1.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:13:50.51 +71:48:33.2 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:13:50.51 +71:48:33.2: 13.51 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:13:50.51 +71:48:33.2: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.53 12:58:42.59 +72:58:36.9
122.19038 44.14086 galactic Dra Second-epoch detections are separated by 0.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:58:42.59 +72:58:36.9 (user input) | T | P | (position from user input) J-Ks=0.461+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:42.59 +72:58:36.9: 13.49 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:42.59 +72:58:36.9: 13.49 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.45 13:00:01.80 +72:50:19.0
122.04689 44.27487 galactic Dra Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:00:01.80 +72:50:19.0 (user input) | T | P | (position from user input) J-Ks=0.382+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:01.80 +72:50:19.0: 13.47 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:01.80 +72:50:19.0: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.41 12:51:25.91 +72:45:38.4
122.93255 44.36758 galactic Dra Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:51:25.91 +72:45:38.4 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:51:25.91 +72:45:38.4: 13.50 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:51:25.91 +72:45:38.4: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.46 13:03:40.05 +72:56:33.0
121.68238 44.15607 galactic Dra Second-epoch detections are separated by 0.3" and 7.4 pix
The object was found in VSX 1" Gaia DR3 1688142500626030080
Type: ROT
# Max. Min./Amp. JD0 Period
13.020 G 13.080 G K
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:03:40.05 +72:56:33.0: 13.46 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:03:40.05 +72:56:33.0: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688142500626030080,2461335.6793,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688142500626030080 20261022.1793 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.63 13:01:23.83 +73:19:03.4
121.94205 43.79149 galactic Dra Second-epoch detections are separated by 1.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:01:23.83 +73:19:03.4 (user input) | T | P | (position from user input) J-Ks=0.781+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:23.83 +73:19:03.4: 13.47 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:23.83 +73:19:03.4: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.47 13:13:32.47 +72:42:16.1
120.63844 44.32522 galactic UMi Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:13:32.47 +72:42:16.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:13:32.47 +72:42:16.1: 13.47 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:13:32.47 +72:42:16.1: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.47 13:05:33.68 +72:16:21.0
121.41717 44.81419 galactic UMi Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:05:33.68 +72:16:21.0 (user input) | T | P | (position from user input) J-Ks=0.564+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:05:33.68 +72:16:21.0: 13.45 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:05:33.68 +72:16:21.0: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.59 13:07:25.77 +72:39:06.8
121.26386 44.42453 galactic UMi Second-epoch detections are separated by 1.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:07:25.77 +72:39:06.8 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:25.77 +72:39:06.8: 13.46 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:25.77 +72:39:06.8: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.69 13:04:26.17 +73:14:02.6
121.63243 43.86138 galactic UMi Second-epoch detections are separated by 2.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:04:26.17 +73:14:02.6 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:04:26.17 +73:14:02.6: 13.46 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:04:26.17 +73:14:02.6: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.38 12:48:47.38 +72:59:37.4
123.20171 44.13314 galactic Dra Second-epoch detections are separated by 2.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:48:47.38 +72:59:37.4 (user input) | T | P | (position from user input) J-Ks=0.582+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:48:47.38 +72:59:37.4: 13.45 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:48:47.38 +72:59:37.4: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.42 12:56:27.99 +72:42:58.8
122.40913 44.40681 galactic Dra Second-epoch detections are separated by 2.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:56:27.99 +72:42:58.8 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.032 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:27.99 +72:42:58.8: 13.45 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:27.99 +72:42:58.8: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.55 13:07:20.98 +72:44:49.8
121.28368 44.33013 galactic UMi Second-epoch detections are separated by 1.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:07:20.98 +72:44:49.8 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:20.98 +72:44:49.8: 13.47 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:20.98 +72:44:49.8: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.56 13:21:59.20 +71:34:54.7
119.50699 45.34269 galactic UMi Second-epoch detections are separated by 2.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:59.20 +71:34:54.7 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:59.20 +71:34:54.7: 13.43 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:59.20 +71:34:54.7: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.60 13:24:16.16 +71:30:22.0
119.23499 45.38574 galactic UMi Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:24:16.16 +71:30:22.0 (user input) | T | P | (position from user input) J-Ks=0.522+/-0.032 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:24:16.16 +71:30:22.0: 13.43 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:24:16.16 +71:30:22.0: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.57 13:10:44.22 +71:45:25.8
120.78705 45.29063 galactic UMi Second-epoch detections are separated by 1.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:10:44.22 +71:45:25.8 (user input) | T | P | (position from user input) J-Ks=0.192+/-0.035 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:10:44.22 +71:45:25.8: 13.43 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:10:44.22 +71:45:25.8: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.64 12:57:25.78 +73:24:36.7
122.34029 43.71117 galactic Dra Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:57:25.78 +73:24:36.7 (user input) | T | P | (position from user input) J-Ks=0.334+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:57:25.78 +73:24:36.7: 13.42 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:57:25.78 +73:24:36.7: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.46 13:08:33.28 +72:39:18.9
121.14734 44.41364 galactic UMi Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:08:33.28 +72:39:18.9 (user input) | T | P | (position from user input) J-Ks=0.343+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:08:33.28 +72:39:18.9: 13.41 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:08:33.28 +72:39:18.9: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.39 13:07:33.55 +72:54:30.0
121.28169 44.16823 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:07:33.55 +72:54:30.0 (user input) | T | P | (position from user input) J-Ks=0.344+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:33.55 +72:54:30.0: 13.40 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:33.55 +72:54:30.0: 13.43 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.77 13:14:10.93 +71:30:50.6
120.36303 45.50058 galactic UMi Second-epoch detections are separated by 5.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:14:10.93 +71:30:50.6 (user input) | T | P | (position from user input) J-Ks=0.554+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:10.93 +71:30:50.6: 13.40 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:10.93 +71:30:50.6: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.57 13:24:01.15 +71:55:46.8
119.37027 44.97259 galactic UMi Second-epoch detections are separated by 1.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:24:01.15 +71:55:46.8 (user input) | T | P | (position from user input) J-Ks=0.597+/-0.036 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:24:01.15 +71:55:46.8: 13.40 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:24:01.15 +71:55:46.8: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.28 12:55:04.45 +72:47:32.2
122.55595 44.33332 galactic Dra Second-epoch detections are separated by 1.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:55:04.45 +72:47:32.2 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:55:04.45 +72:47:32.2: 13.39 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:55:04.45 +72:47:32.2: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.46 13:00:49.89 +72:58:31.6
121.97412 44.13533 galactic Dra Second-epoch detections are separated by 1.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:00:49.89 +72:58:31.6 (user input) | T | P | (position from user input) J-Ks=0.840+/-0.027 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:49.89 +72:58:31.6: 13.39 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:49.89 +72:58:31.6: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.65 13:26:30.90 +72:01:59.4
119.12948 44.83521 galactic UMi Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:26:30.90 +72:01:59.4 (user input) | T | P | (position from user input) J-Ks=0.559+/-0.035 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:26:30.90 +72:01:59.4: 13.38 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:26:30.90 +72:01:59.4: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.34 13:06:08.59 +72:20:50.3
121.36340 44.73613 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1688086494251713920 | 13:06:08.59 +72:20:50.3 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.823+/-0.029 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:08.59 +72:20:50.3: 13.35 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:08.59 +72:20:50.3: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1688086494251713920,2461335.6793,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1688086494251713920 20261022.1793 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.59 13:18:15.77 +72:31:25.4
120.11565 44.45755 galactic UMi Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:18:15.77 +72:31:25.4 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:15.77 +72:31:25.4: 13.36 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:15.77 +72:31:25.4: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.46 13:06:42.04 +72:40:56.5
121.34320 44.39878 galactic UMi Second-epoch detections are separated by 1.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:06:42.04 +72:40:56.5 (user input) | T | P | (position from user input) J-Ks=0.289+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:42.04 +72:40:56.5: 13.36 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:42.04 +72:40:56.5: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.69 13:23:54.43 +71:33:11.7
119.28722 45.34453 galactic UMi Second-epoch detections are separated by 2.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:23:54.43 +71:33:11.7 (user input) | T | P | (position from user input) J-Ks=0.311+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:54.43 +71:33:11.7: 13.38 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:54.43 +71:33:11.7: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.34 13:15:46.85 +72:10:09.7
120.30816 44.83467 galactic UMi Second-epoch detections are separated by 2.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:46.85 +72:10:09.7 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.058 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:46.85 +72:10:09.7: 13.36 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:46.85 +72:10:09.7: 13.38 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.54 12:57:44.81 +73:14:08.2
122.30078 43.88491 galactic Dra Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:57:44.81 +73:14:08.2 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:57:44.81 +73:14:08.2: 13.33 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:57:44.81 +73:14:08.2: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.33 12:44:20.10 +73:18:22.2
123.63870 43.81234 galactic Dra Second-epoch detections are separated by 1.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:44:20.10 +73:18:22.2 (user input) | T | P | (position from user input) J-Ks=0.802+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:44:20.10 +73:18:22.2: 13.36 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:44:20.10 +73:18:22.2: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.54 13:08:31.68 +72:09:36.8
121.08524 44.90670 galactic UMi Second-epoch detections are separated by 1.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:08:31.68 +72:09:36.8 (user input) | T | P | (position from user input) J-Ks=0.588+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:08:31.68 +72:09:36.8: 13.38 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:08:31.68 +72:09:36.8: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.63 13:32:42.39 +71:06:13.9
118.17322 45.64117 galactic UMi Second-epoch detections are separated by 2.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:32:42.39 +71:06:13.9 (user input) | T | P | (position from user input) J-Ks=0.750+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:42.39 +71:06:13.9: 13.37 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:42.39 +71:06:13.9: 13.39 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.43 13:32:16.86 +71:26:19.0
118.32866 45.32282 galactic UMi Second-epoch detections are separated by 2.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:32:16.86 +71:26:19.0 (user input) | T | P | (position from user input) J-Ks=0.794+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:16.86 +71:26:19.0: 13.33 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:16.86 +71:26:19.0: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.96 12:48:18.74 +73:10:12.2
123.24619 43.95629 galactic Dra Second-epoch detections are separated by 0.9" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691196497251416832 | 12:48:19.01 +73:10:12.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.533+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:48:18.74 +73:10:12.2: 12.81 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:48:18.74 +73:10:12.2: 12.87 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691196497251416832,2461335.6793,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691196497251416832 20261022.1793 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.54 13:34:15.26 +71:33:17.2
118.15007 45.17383 galactic UMi Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:34:15.26 +71:33:17.2 (user input) | T | P | (position from user input) J-Ks=0.243+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:34:15.26 +71:33:17.2: 13.30 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:34:15.26 +71:33:17.2: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.52 13:24:02.37 +72:15:55.0
119.45221 44.64205 galactic UMi Second-epoch detections are separated by 2.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:24:02.37 +72:15:55.0 (user input) | T | P | (position from user input) J-Ks=0.319+/-0.034 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:24:02.37 +72:15:55.0: 13.32 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:24:02.37 +72:15:55.0: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.32 13:05:42.21 +72:16:06.7
121.40153 44.81731 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:05:42.21 +72:16:06.7 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:05:42.21 +72:16:06.7: 13.31 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:05:42.21 +72:16:06.7: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.57 13:36:16.68 +71:41:24.7
117.97669 45.00415 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:36:16.68 +71:41:24.7 (user input) | T | P | (position from user input) J-Ks=0.604+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:36:16.68 +71:41:24.7: 13.33 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:36:16.68 +71:41:24.7: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.79 13:20:55.33 +71:03:56.8
119.50456 45.86576 galactic UMi Second-epoch detections are separated by 2.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:20:55.33 +71:03:56.8 (user input) | T | P | (position from user input) J-Ks=0.289+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:20:55.33 +71:03:56.8: 13.32 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:20:55.33 +71:03:56.8: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.36 13:29:32.39 +71:37:49.6
118.68870 45.18258 galactic UMi Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:29:32.39 +71:37:49.6 (user input) | T | P | (position from user input) J-Ks=0.655+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:29:32.39 +71:37:49.6: 13.32 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:29:32.39 +71:37:49.6: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.65 13:37:44.01 +71:56:18.1
117.90831 44.73557 galactic UMi Second-epoch detections are separated by 1.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:37:44.01 +71:56:18.1 (user input) | T | P | (position from user input) J-Ks=0.342+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:37:44.01 +71:56:18.1: 13.29 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:37:44.01 +71:56:18.1: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.35 12:54:20.09 +72:46:51.1
122.63213 44.34570 galactic Dra Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:54:20.09 +72:46:51.1 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:54:20.09 +72:46:51.1: 13.29 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:54:20.09 +72:46:51.1: 13.25 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.26 13:13:17.73 +72:11:14.5
120.57739 44.84083 galactic UMi Second-epoch detections are separated by 1.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:13:17.73 +72:11:14.5 (user input) | T | P | (position from user input) J-Ks=0.495+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:13:17.73 +72:11:14.5: 13.29 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:13:17.73 +72:11:14.5: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.33 12:50:31.15 +73:11:01.3
123.02421 43.94439 galactic Dra Second-epoch detections are separated by 2.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1691198833712957312 | 12:50:31.15 +73:11:01.3 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.387+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:50:31.15 +73:11:01.3: 13.31 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:50:31.15 +73:11:01.3: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1691198833712957312,2461335.6793,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1691198833712957312 20261022.1793 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.38 13:15:47.45 +72:07:13.3
120.29788 44.88313 galactic UMi Second-epoch detections are separated by 1.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:47.45 +72:07:13.3 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:47.45 +72:07:13.3: 13.29 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:47.45 +72:07:13.3: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.21 12:40:05.33 +73:13:28.7
124.06760 43.87858 galactic Dra Second-epoch detections are separated by 1.9" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:40:05.33 +73:13:28.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:40:05.33 +73:13:28.7: 13.31 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:40:05.33 +73:13:28.7: 13.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.52 13:20:46.11 +71:47:47.1
119.69121 45.14682 galactic UMi Second-epoch detections are separated by 0.9" and 7.4 pix
The object was found in VSX 1" Gaia DR3 1687790278947988864
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.130 G 13.160 G F
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:20:46.11 +71:47:47.1: 13.29 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:20:46.11 +71:47:47.1: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687790278947988864,2461335.6793,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687790278947988864 20261022.1793 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.53 13:09:22.55 +71:38:50.5
120.92221 45.41083 galactic UMi Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:09:22.55 +71:38:50.5 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:09:22.55 +71:38:50.5: 13.30 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:09:22.55 +71:38:50.5: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.40 13:01:03.11 +72:18:20.9
121.90261 44.80323 galactic Dra Second-epoch detections are separated by 0.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:01:03.11 +72:18:20.9 (user input) | T | P | (position from user input) J-Ks=0.306+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:03.11 +72:18:20.9: 13.27 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:03.11 +72:18:20.9: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.47 13:15:15.15 +71:47:14.5
120.29410 45.21872 galactic UMi Second-epoch detections are separated by 2.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:15.15 +71:47:14.5 (user input) | T | P | (position from user input) J-Ks=0.015+/-0.048 (A)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:15.15 +71:47:14.5: 13.27 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:15.15 +71:47:14.5: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.24 13:11:11.35 +71:58:03.5
120.76950 45.07759 galactic UMi Second-epoch detections are separated by 1.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:11:11.35 +71:58:03.5 (user input) | T | P | (position from user input) J-Ks=0.434+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:11:11.35 +71:58:03.5: 13.27 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:11:11.35 +71:58:03.5: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.51 13:21:19.87 +72:18:09.9
119.74651 44.64015 galactic UMi Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:19.87 +72:18:09.9 (user input) | T | P | (position from user input) J-Ks=0.373+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:19.87 +72:18:09.9: 13.26 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:19.87 +72:18:09.9: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.36 12:55:17.14 +73:24:59.2
122.55212 43.70897 galactic Dra Second-epoch detections are separated by 0.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:55:17.14 +73:24:59.2 (user input) | T | P | (position from user input) J-Ks=0.423+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:55:17.14 +73:24:59.2: 13.25 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:55:17.14 +73:24:59.2: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.54 13:21:16.99 +71:30:26.7
119.56751 45.42537 galactic UMi Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:16.99 +71:30:26.7 (user input) | T | P | (position from user input) J-Ks=0.310+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:16.99 +71:30:26.7: 13.25 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:16.99 +71:30:26.7: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.55 13:10:52.40 +71:46:07.1
120.77372 45.27808 galactic UMi Second-epoch detections are separated by 1.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:10:52.40 +71:46:07.1 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:10:52.40 +71:46:07.1: 13.26 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:10:52.40 +71:46:07.1: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.37 13:07:29.03 +73:10:26.5
121.32139 43.90401 galactic UMi Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:07:29.03 +73:10:26.5 (user input) | T | P | (position from user input) J-Ks=0.342+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:29.03 +73:10:26.5: 13.25 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:29.03 +73:10:26.5: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.54 13:17:40.41 +72:20:00.1
120.13888 44.65234 galactic UMi Second-epoch detections are separated by 2.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:17:40.41 +72:20:00.1 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:17:40.41 +72:20:00.1: 13.26 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:17:40.41 +72:20:00.1: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.39 13:16:59.46 +72:03:29.2
120.15682 44.93220 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:16:59.46 +72:03:29.2 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.035 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:16:59.46 +72:03:29.2: 13.25 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:16:59.46 +72:03:29.2: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.29 12:58:30.58 +72:46:28.4
122.19995 44.34364 galactic Dra Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:58:30.58 +72:46:28.4 (user input) | T | P | (position from user input) J-Ks=0.363+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:30.58 +72:46:28.4: 13.24 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:30.58 +72:46:28.4: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.51 13:36:15.70 +71:16:33.1
117.83409 45.40611 galactic UMi Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:36:15.70 +71:16:33.1 (user input) | T | P | (position from user input) J-Ks=11.827+/- (unrealisitic color!)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:36:15.70 +71:16:33.1: 13.26 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:36:15.70 +71:16:33.1: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.47 13:16:11.35 +72:52:41.5
120.39805 44.12808 galactic UMi Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:16:11.35 +72:52:41.5 (user input) | T | P | (position from user input) J-Ks=0.396+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:16:11.35 +72:52:41.5: 13.23 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:16:11.35 +72:52:41.5: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.43 13:24:46.70 +71:35:06.3
119.19911 45.30075 galactic UMi Second-epoch detections are separated by 1.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:24:46.70 +71:35:06.3 (user input) | T | P | (position from user input) J-Ks=0.342+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:24:46.70 +71:35:06.3: 13.24 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:24:46.70 +71:35:06.3: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.36 13:21:23.84 +72:06:14.9
119.69388 44.83528 galactic UMi Second-epoch detections are separated by 1.6" and 7.6 pix
The object was found in VSX 2" Gaia DR3 1687890334506098176
Type: ROT
# Max. Min./Amp. JD0 Period
12.850 G 12.880 G K
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:23.84 +72:06:14.9: 13.22 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:23.84 +72:06:14.9: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687890334506098176,2461335.6793,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687890334506098176 20261022.1793 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.53 13:22:55.68 +72:32:11.9
119.63444 44.38944 galactic UMi Second-epoch detections are separated by 1.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:22:55.68 +72:32:11.9 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:22:55.68 +72:32:11.9: 13.24 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:22:55.68 +72:32:11.9: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.30 12:59:27.31 +72:44:42.9
122.10037 44.37005 galactic Dra Second-epoch detections are separated by 1.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:59:27.31 +72:44:42.9 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:27.31 +72:44:42.9: 13.21 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:27.31 +72:44:42.9: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.66 12:57:30.88 +73:39:04.8
122.34275 43.46997 galactic Dra Second-epoch detections are separated by 0.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:57:30.88 +73:39:04.8 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:57:30.88 +73:39:04.8: 13.22 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:57:30.88 +73:39:04.8: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.62 13:04:18.31 +71:56:04.9
121.51788 45.15821 galactic UMi Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:04:18.31 +71:56:04.9 (user input) | T | P | (position from user input) J-Ks=0.560+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:04:18.31 +71:56:04.9: 13.22 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:04:18.31 +71:56:04.9: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.29 12:41:38.63 +72:44:23.5
123.94796 44.36906 galactic Dra Second-epoch detections are separated by 1.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:41:38.63 +72:44:23.5 (user input) | T | P | (position from user input) J-Ks=0.351+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:41:38.63 +72:44:23.5: 13.14 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:41:38.63 +72:44:23.5: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.58 13:28:20.72 +71:55:35.1
118.90403 44.91207 galactic UMi Second-epoch detections are separated by 1.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:28:20.72 +71:55:35.1 (user input) | T | P | (position from user input) J-Ks=0.480+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:20.72 +71:55:35.1: 13.24 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:20.72 +71:55:35.1: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.24 13:07:18.75 +72:22:07.7
121.24168 44.70731 galactic UMi Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:07:18.75 +72:22:07.7 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:18.75 +72:22:07.7: 13.21 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:18.75 +72:22:07.7: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.34 13:14:20.50 +72:35:29.9
120.53629 44.42992 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:14:20.50 +72:35:29.9 (user input) | T | P | (position from user input) J-Ks=0.553+/-0.034 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:20.50 +72:35:29.9: 13.20 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:20.50 +72:35:29.9: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.31 13:21:39.25 +71:43:36.0
119.57805 45.20430 galactic UMi Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:39.25 +71:43:36.0 (user input) | T | P | (position from user input) J-Ks=0.328+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:39.25 +71:43:36.0: 13.22 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:39.25 +71:43:36.0: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.70 13:04:26.86 +72:50:34.0
121.59303 44.25164 galactic UMi Second-epoch detections are separated by 2.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:04:26.86 +72:50:34.0 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.036 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:04:26.86 +72:50:34.0: 13.72 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:04:26.86 +72:50:34.0: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.18 12:47:02.63 +73:12:57.3
123.37220 43.90858 galactic Dra Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:47:02.63 +73:12:57.3 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.027 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:47:02.63 +73:12:57.3: 13.21 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:47:02.63 +73:12:57.3: 13.16 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.46 13:27:41.73 +72:08:56.9
119.03582 44.70381 galactic UMi Second-epoch detections are separated by 1.5" and 7.3 pix
The object was found in VSX 1" Gaia DR3 1687901673219720448
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.970 G 13.000 G F
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:41.73 +72:08:56.9: 13.20 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:41.73 +72:08:56.9: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687901673219720448,2461335.6793,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687901673219720448 20261022.1793 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.19 12:43:48.66 +73:22:47.2
123.68663 43.73730 galactic Dra Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:43:48.66 +73:22:47.2 (user input) | T | P | (position from user input) J-Ks=0.479+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:43:48.66 +73:22:47.2: 13.10 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:43:48.66 +73:22:47.2: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.36 12:50:10.58 +73:36:21.6
123.05468 43.52195 galactic Dra Second-epoch detections are separated by 1.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:50:10.58 +73:36:21.6 (user input) | T | P | (position from user input) J-Ks=0.305+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:50:10.58 +73:36:21.6: 13.22 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:50:10.58 +73:36:21.6: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.23 13:21:14.53 +71:48:45.1
119.64319 45.12492 galactic UMi Second-epoch detections are separated by 1.1" and 7.4 pix
The object was found in VSX 1" Gaia DR3 1687790759984326656
Type: ROT
# Max. Min./Amp. JD0 Period
12.820 G 12.850 G K
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:14.53 +71:48:45.1: 13.19 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:14.53 +71:48:45.1: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687790759984326656,2461335.6793,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687790759984326656 20261022.1793 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.30 13:12:39.08 +72:25:47.2
120.68589 44.60585 galactic UMi Second-epoch detections are separated by 1.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:12:39.08 +72:25:47.2 (user input) | T | P | (position from user input) J-Ks=0.728+/-0.034 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:12:39.08 +72:25:47.2: 13.19 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:12:39.08 +72:25:47.2: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.31 13:12:16.25 +72:21:42.9
120.71513 44.67656 galactic UMi Second-epoch detections are separated by 2.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:12:16.25 +72:21:42.9 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:12:16.25 +72:21:42.9: 13.18 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:12:16.25 +72:21:42.9: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.34 12:54:54.68 +73:09:36.4
122.58242 43.96578 galactic Dra Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:54:54.68 +73:09:36.4 (user input) | T | P | (position from user input) J-Ks=0.419+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:54:54.68 +73:09:36.4: 13.18 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:54:54.68 +73:09:36.4: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.44 13:12:34.95 +72:59:46.7
120.78390 44.04365 galactic UMi Second-epoch detections are separated by 2.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:12:34.95 +72:59:46.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:12:34.95 +72:59:46.7: 13.19 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:12:34.95 +72:59:46.7: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.17 12:52:55.29 +72:50:35.1
122.77909 44.28473 galactic Dra Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:52:55.29 +72:50:35.1 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:52:55.29 +72:50:35.1: 13.17 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:52:55.29 +72:50:35.1: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.28 13:26:50.22 +71:29:45.5
118.94752 45.35743 galactic UMi Second-epoch detections are separated by 2.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:26:50.22 +71:29:45.5 (user input) | T | P | (position from user input) J-Ks=0.475+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:26:50.22 +71:29:45.5: 13.19 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:26:50.22 +71:29:45.5: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.31 13:06:03.28 +72:30:52.9
121.39158 44.56982 galactic UMi Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:06:03.28 +72:30:52.9 (user input) | T | P | (position from user input) J-Ks=0.697+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:03.28 +72:30:52.9: 13.19 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:03.28 +72:30:52.9: 13.19 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.37 13:34:11.36 +71:38:15.8
118.18467 45.09440 galactic UMi Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:34:11.36 +71:38:15.8 (user input) | T | P | (position from user input) J-Ks=0.456+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:34:11.36 +71:38:15.8: 13.17 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:34:11.36 +71:38:15.8: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.33 13:21:39.33 +71:41:36.8
119.57009 45.23693 galactic UMi Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:39.33 +71:41:36.8 (user input) | T | P | (position from user input) J-Ks=0.345+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:39.33 +71:41:36.8: 13.17 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:39.33 +71:41:36.8: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.32 13:23:26.11 +71:20:57.7
119.28819 45.55184 galactic UMi Second-epoch detections are separated by 1.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:23:26.11 +71:20:57.7 (user input) | T | P | (position from user input) J-Ks=0.569+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:26.11 +71:20:57.7: 13.14 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:26.11 +71:20:57.7: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.19 13:00:41.05 +72:40:50.2
121.96848 44.43034 galactic Dra Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:00:41.05 +72:40:50.2 (user input) | T | P | (position from user input) J-Ks=0.340+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:41.05 +72:40:50.2: 13.12 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:41.05 +72:40:50.2: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.40 13:28:32.68 +71:45:48.2
118.83589 45.06859 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:28:32.68 +71:45:48.2 (user input) | T | P | (position from user input) J-Ks=0.561+/-0.034 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:32.68 +71:45:48.2: 13.14 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:32.68 +71:45:48.2: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.21 13:16:26.32 +71:58:12.7
120.19930 45.02517 galactic UMi Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:16:26.32 +71:58:12.7 (user input) | T | P | (position from user input) J-Ks=0.301+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:16:26.32 +71:58:12.7: 13.14 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:16:26.32 +71:58:12.7: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.19 12:41:39.35 +72:54:10.6
123.93463 44.20626 galactic Dra Second-epoch detections are separated by 1.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:41:39.35 +72:54:10.6 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:41:39.35 +72:54:10.6: 13.18 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:41:39.35 +72:54:10.6: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.31 13:06:30.73 +72:08:40.3
121.30057 44.93594 galactic UMi Second-epoch detections are separated by 1.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:06:30.73 +72:08:40.3 (user input) | T | P | (position from user input) J-Ks=0.539+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:30.73 +72:08:40.3: 13.11 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:30.73 +72:08:40.3: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.12 13:08:06.85 +72:26:10.3
121.16523 44.63481 galactic UMi Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:08:06.85 +72:26:10.3 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.032 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:08:06.85 +72:26:10.3: 13.11 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:08:06.85 +72:26:10.3: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.46 13:13:03.94 +72:55:30.5
120.72353 44.11026 galactic UMi Second-epoch detections are separated by 2.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:13:03.94 +72:55:30.5 (user input) | T | P | (position from user input) J-Ks=0.399+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:13:03.94 +72:55:30.5: 13.12 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:13:03.94 +72:55:30.5: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.21 12:58:03.43 +72:40:46.8
122.24199 44.43972 galactic Dra Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:58:03.43 +72:40:46.8 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:03.43 +72:40:46.8: 13.10 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:03.43 +72:40:46.8: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.15 13:15:16.78 +72:31:47.3
120.42763 44.48233 galactic UMi Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:16.78 +72:31:47.3 (user input) | T | P | (position from user input) J-Ks=0.614+/-0.034 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:16.78 +72:31:47.3: 13.09 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:16.78 +72:31:47.3: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.19 13:01:49.98 +73:05:38.2
121.88140 44.01310 galactic Dra Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:01:49.98 +73:05:38.2 (user input) | T | P | (position from user input) J-Ks=0.455+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:49.98 +73:05:38.2: 13.11 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:49.98 +73:05:38.2: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.29 13:18:02.85 +71:49:01.7
119.99332 45.15898 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:18:02.85 +71:49:01.7 (user input) | T | P | (position from user input) J-Ks=0.556+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:02.85 +71:49:01.7: 13.10 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:02.85 +71:49:01.7: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.48 13:32:15.12 +72:06:01.5
118.54055 44.67819 galactic UMi Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:32:15.12 +72:06:01.5 (user input) | T | P | (position from user input) J-Ks=0.358+/-0.035 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:15.12 +72:06:01.5: 13.10 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:15.12 +72:06:01.5: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.43 13:04:41.75 +73:27:59.1
121.62943 43.62829 galactic UMi Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:04:41.75 +73:27:59.1 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:04:41.75 +73:27:59.1: 13.08 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:04:41.75 +73:27:59.1: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.11 13:01:01.23 +72:35:09.9
121.92657 44.52346 galactic Dra Second-epoch detections are separated by 0.3" and 7.4 pix
The object was found in VSX 6" Gaia DR3 1688108106527911680
Type: ROT
# Max. Min./Amp. JD0 Period
12.320 G 12.350 G M
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:01.23 +72:35:09.9: 13.07 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:01.23 +72:35:09.9: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688108106527911680,2461335.6793,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688108106527911680 20261022.1793 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.30 15:36:12.29 +65:44:49.7
100.95947 43.69652 galactic UMi Second-epoch detections are separated by 3.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:36:12.29 +65:44:49.7 (user input) | T | P | (position from user input) J-Ks=0.563+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:36:12.29 +65:44:49.7: 13.08 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:36:12.29 +65:44:49.7: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.26 13:15:22.65 +72:12:29.8
120.35849 44.80016 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:15:22.65 +72:12:29.8 (user input) | T | P | (position from user input) J-Ks=0.495+/-0.035 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:22.65 +72:12:29.8: 13.05 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:22.65 +72:12:29.8: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.50 13:25:41.60 +70:54:24.1
118.91437 45.95341 galactic UMi Second-epoch detections are separated by 1.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:25:41.60 +70:54:24.1 (user input) | T | P | (position from user input) J-Ks=0.594+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:41.60 +70:54:24.1: 13.09 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:41.60 +70:54:24.1: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.15 12:55:10.52 +72:36:54.7
122.54045 44.51022 galactic Dra Second-epoch detections are separated by 1.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:55:10.52 +72:36:54.7 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:55:10.52 +72:36:54.7: 13.05 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:55:10.52 +72:36:54.7: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.30 12:58:33.33 +73:28:20.1
122.23247 43.64633 galactic Dra Second-epoch detections are separated by 1.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:58:33.33 +73:28:20.1 (user input) | T | P | (position from user input) J-Ks=0.269+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:33.33 +73:28:20.1: 13.05 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:33.33 +73:28:20.1: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.27 13:20:38.91 +72:39:08.2
119.89615 44.30339 galactic UMi Second-epoch detections are separated by 2.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:20:38.91 +72:39:08.2 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:20:38.91 +72:39:08.2: 13.06 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:20:38.91 +72:39:08.2: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.28 13:19:51.40 +71:37:45.7
119.75382 45.32312 galactic UMi Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:19:51.40 +71:37:45.7 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:51.40 +71:37:45.7: 13.04 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:51.40 +71:37:45.7: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.21 13:20:15.71 +72:34:31.1
119.91912 44.38394 galactic UMi Second-epoch detections are separated by 1.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:20:15.71 +72:34:31.1 (user input) | T | P | (position from user input) J-Ks=0.583+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:20:15.71 +72:34:31.1: 13.05 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:20:15.71 +72:34:31.1: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.49 13:20:46.24 +72:50:03.0
119.92380 44.12235 galactic UMi Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:20:46.24 +72:50:03.0 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:20:46.24 +72:50:03.0: 13.03 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:20:46.24 +72:50:03.0: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.44 13:23:33.99 +71:14:51.7
119.24761 45.65003 galactic UMi Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:23:33.99 +71:14:51.7 (user input) | T | P | (position from user input) J-Ks=0.695+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:33.99 +71:14:51.7: 13.03 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:33.99 +71:14:51.7: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.19 13:02:01.31 +73:04:44.8
121.86116 44.02713 galactic Dra Second-epoch detections are separated by 1.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:02:01.31 +73:04:44.8 (user input) | T | P | (position from user input) J-Ks=0.555+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:02:01.31 +73:04:44.8: 13.02 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:02:01.31 +73:04:44.8: 12.91 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.11 12:57:13.79 +72:39:06.6
122.32695 44.46961 galactic Dra Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:57:13.79 +72:39:06.6 (user input) | T | P | (position from user input) J-Ks=0.349+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:57:13.79 +72:39:06.6: 13.03 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:57:13.79 +72:39:06.6: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.22 12:58:19.98 +72:16:20.8
122.19172 44.84590 galactic Dra Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:58:19.98 +72:16:20.8 (user input) | T | P | (position from user input) J-Ks=0.642+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:19.98 +72:16:20.8: 13.01 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:19.98 +72:16:20.8: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.22 13:14:32.87 +72:41:53.3
120.53354 44.32233 galactic UMi Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:14:32.87 +72:41:53.3 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.038 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:32.87 +72:41:53.3: 13.02 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:32.87 +72:41:53.3: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.20 13:21:29.70 +72:15:42.4
119.71983 44.67854 galactic UMi Second-epoch detections are separated by 2.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:29.70 +72:15:42.4 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:29.70 +72:15:42.4: 13.02 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:29.70 +72:15:42.4: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.26 13:23:03.77 +72:21:31.9
119.57775 44.56285 galactic UMi Second-epoch detections are separated by 1.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:23:03.77 +72:21:31.9 (user input) | T | P | (position from user input) J-Ks=0.712+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:03.77 +72:21:31.9: 13.02 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:03.77 +72:21:31.9: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.32 13:16:37.10 +72:17:29.9
120.24226 44.70488 galactic UMi Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1687954101885273856 | 13:16:37.10 +72:17:29.9 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.493+/-0.036 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:16:37.10 +72:17:29.9: 12.99 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:16:37.10 +72:17:29.9: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1687954101885273856,2461335.6793,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1687954101885273856 20261022.1793 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.15 12:58:02.55 +72:22:52.0
122.22842 44.73812 galactic Dra Second-epoch detections are separated by 0.9" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:58:02.55 +72:22:52.0 (user input) | T | P | (position from user input) J-Ks=0.505+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:02.55 +72:22:52.0: 13.01 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:02.55 +72:22:52.0: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.66 13:35:04.47 +70:56:11.1
117.84897 45.75875 galactic UMi Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:35:04.47 +70:56:11.1 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:35:04.47 +70:56:11.1: 13.03 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:35:04.47 +70:56:11.1: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.10 13:00:16.10 +72:41:56.2
122.01300 44.41355 galactic Dra Second-epoch detections are separated by 1.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:00:16.10 +72:41:56.2 (user input) | T | P | (position from user input) J-Ks=0.604+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:16.10 +72:41:56.2: 12.98 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:16.10 +72:41:56.2: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.52 13:04:04.51 +73:30:49.2
121.69471 43.58421 galactic UMi Second-epoch detections are separated by 1.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:04:04.51 +73:30:49.2 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:04:04.51 +73:30:49.2: 12.99 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:04:04.51 +73:30:49.2: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.06 13:08:37.09 +72:31:21.5
121.12338 44.54523 galactic UMi Second-epoch detections are separated by 0.3" and 7.4 pix
The object was found in VSX 0" Gaia DR3 1688066668683393536
Type: ROT
# Max. Min./Amp. JD0 Period
12.590 G 12.620 G G
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:08:37.09 +72:31:21.5: 12.98 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:08:37.09 +72:31:21.5: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688066668683393536,2461335.6793,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688066668683393536 20261022.1793 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.21 13:22:50.13 +72:28:43.5
119.63022 44.44767 galactic UMi Second-epoch detections are separated by 1.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:22:50.13 +72:28:43.5 (user input) | T | P | (position from user input) J-Ks=0.658+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:22:50.13 +72:28:43.5: 12.99 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:22:50.13 +72:28:43.5: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.36 13:23:26.14 +71:25:54.5
119.30893 45.47069 galactic UMi Second-epoch detections are separated by 1.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:23:26.14 +71:25:54.5 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:26.14 +71:25:54.5: 12.99 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:26.14 +71:25:54.5: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.33 13:28:54.98 +72:25:59.5
118.98792 44.40693 galactic UMi Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:28:54.98 +72:25:59.5 (user input) | T | P | (position from user input) J-Ks=0.455+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:54.98 +72:25:59.5: 12.99 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:54.98 +72:25:59.5: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.43 13:22:57.92 +71:04:38.9
119.27299 45.82614 galactic UMi Second-epoch detections are separated by 1.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:22:57.92 +71:04:38.9 (user input) | T | P | (position from user input) J-Ks=0.560+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:22:57.92 +71:04:38.9: 12.98 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:22:57.92 +71:04:38.9: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.51 13:24:12.23 +70:57:15.2
119.09900 45.92940 galactic UMi Second-epoch detections are separated by 2.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:24:12.23 +70:57:15.2 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:24:12.23 +70:57:15.2: 12.93 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:24:12.23 +70:57:15.2: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.51 13:00:06.20 +73:36:25.2
122.08912 43.50707 galactic Dra Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:00:06.20 +73:36:25.2 (user input) | T | P | (position from user input) J-Ks=0.594+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:06.20 +73:36:25.2: 12.97 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:06.20 +73:36:25.2: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.10 12:49:44.61 +73:08:59.7
123.10255 43.97777 galactic Dra Second-epoch detections are separated by 1.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:49:44.61 +73:08:59.7 (user input) | T | P | (position from user input) J-Ks=0.413+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:49:44.61 +73:08:59.7: 12.98 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:49:44.61 +73:08:59.7: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.19 13:16:54.28 +72:37:21.5
120.27622 44.37406 galactic UMi Second-epoch detections are separated by 1.8" and 7.1 pix
The object was found in VSX 1" NSVS 897646
Type: EB
# Max. Min./Amp. JD0 Period
12.914 g Y 0.357 g 2458282.77980 0.721203400000
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:16:54.28 +72:37:21.5: 12.94 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:16:54.28 +72:37:21.5: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 897646,2461335.6793,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 897646 20261022.1793 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.31 13:25:00.45 +71:26:31.6
119.13619 45.43792 galactic UMi Second-epoch detections are separated by 1.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:25:00.45 +71:26:31.6 (user input) | T | P | (position from user input) J-Ks=0.550+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:00.45 +71:26:31.6: 12.97 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:00.45 +71:26:31.6: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.48 13:26:39.43 +71:55:52.2
119.08662 44.93320 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:26:39.43 +71:55:52.2 (user input) | T | P | (position from user input) J-Ks=0.879+/-0.026 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:26:39.43 +71:55:52.2: 12.95 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:26:39.43 +71:55:52.2: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.07 13:05:55.27 +72:05:29.6
121.35841 44.99242 galactic UMi Second-epoch detections are separated by 1.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:05:55.27 +72:05:29.6 (user input) | T | P | (position from user input) J-Ks=0.341+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:05:55.27 +72:05:29.6: 12.94 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:05:55.27 +72:05:29.6: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.22 13:17:31.63 +72:07:02.2
120.11100 44.86780 galactic UMi Second-epoch detections are separated by 1.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:17:31.63 +72:07:02.2 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:17:31.63 +72:07:02.2: 12.93 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:17:31.63 +72:07:02.2: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.04 13:06:34.93 +72:25:03.3
121.32488 44.66338 galactic UMi Second-epoch detections are separated by 0.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:06:34.93 +72:25:03.3 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.032 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:34.93 +72:25:03.3: 12.91 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:34.93 +72:25:03.3: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.39 13:29:23.30 +71:07:50.6
118.55641 45.67375 galactic UMi Second-epoch detections are separated by 0.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:29:23.30 +71:07:50.6 (user input) | T | P | (position from user input) J-Ks=0.306+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:29:23.30 +71:07:50.6: 12.92 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:29:23.30 +71:07:50.6: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.14 12:49:19.10 +73:14:08.8
123.14400 43.89160 galactic Dra Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:49:19.10 +73:14:08.8 (user input) | T | P | (position from user input) J-Ks=0.332+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:49:19.10 +73:14:08.8: 12.96 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:49:19.10 +73:14:08.8: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.32 13:29:10.08 +72:02:46.5
118.85060 44.78180 galactic UMi Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:29:10.08 +72:02:46.5 (user input) | T | P | (position from user input) J-Ks=0.267+/-0.035 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:29:10.08 +72:02:46.5: 12.92 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:29:10.08 +72:02:46.5: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.10 13:28:38.58 +71:33:53.7
118.76780 45.26132 galactic UMi Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:28:38.58 +71:33:53.7 (user input) | T | P | (position from user input) J-Ks=0.422+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:38.58 +71:33:53.7: 12.91 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:38.58 +71:33:53.7: 12.97 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.14 13:00:02.15 +73:26:50.1
122.08551 43.66687 galactic Dra Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691250991796390144 | 13:00:02.15 +73:26:50.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.623+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:02.15 +73:26:50.1: 12.91 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:02.15 +73:26:50.1: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691250991796390144,2461335.6793,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691250991796390144 20261022.1793 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.12 15:34:52.40 +65:39:51.3
100.97807 43.85604 galactic UMi Second-epoch detections are separated by 1.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:34:52.40 +65:39:51.3 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:34:52.40 +65:39:51.3: 12.92 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:34:52.40 +65:39:51.3: 12.92 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.05 12:51:40.12 +73:07:19.8
122.90863 44.00607 galactic Dra Second-epoch detections are separated by 0.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691186464207806080 | 12:51:40.19 +73:07:19.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.295+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:51:40.12 +73:07:19.8: 12.91 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:51:40.12 +73:07:19.8: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691186464207806080,2461335.6793,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691186464207806080 20261022.1793 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.21 13:24:51.51 +72:16:27.4
119.36828 44.62200 galactic UMi Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:24:51.51 +72:16:27.4 (user input) | T | P | (position from user input) J-Ks=0.717+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:24:51.51 +72:16:27.4: 12.93 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:24:51.51 +72:16:27.4: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.50 13:39:02.21 +71:46:34.8
117.71179 44.86634 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:39:02.21 +71:46:34.8 (user input) | T | P | (position from user input) J-Ks=0.459+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:39:02.21 +71:46:34.8: 12.94 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:39:02.21 +71:46:34.8: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.23 12:49:02.47 +72:33:11.0
123.18411 44.57402 galactic Dra Second-epoch detections are separated by 0.9" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689653092163944832 | 12:49:02.49 +72:33:11.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.585+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:49:02.47 +72:33:11.0: 12.90 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:49:02.47 +72:33:11.0: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689653092163944832,2461335.6793,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689653092163944832 20261022.1793 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.29 13:09:59.18 +73:16:31.0
121.08517 43.78640 galactic UMi Second-epoch detections are separated by 1.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:09:59.18 +73:16:31.0 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:09:59.18 +73:16:31.0: 12.89 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:09:59.18 +73:16:31.0: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.26 13:29:14.34 +72:06:34.7
118.86142 44.71865 galactic UMi Second-epoch detections are separated by 1.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:29:14.34 +72:06:34.7 (user input) | T | P | (position from user input) J-Ks=0.347+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:29:14.34 +72:06:34.7: 12.90 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:29:14.34 +72:06:34.7: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.08 12:56:55.90 +72:43:26.2
122.36110 44.39822 galactic Dra Second-epoch detections are separated by 1.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:56:55.90 +72:43:26.2 (user input) | T | P | (position from user input) J-Ks=0.319+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:55.90 +72:43:26.2: 12.90 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:55.90 +72:43:26.2: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.28 13:30:18.59 +72:11:50.2
118.77426 44.61584 galactic UMi Second-epoch detections are separated by 1.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:30:18.59 +72:11:50.2 (user input) | T | P | (position from user input) J-Ks=0.336+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:30:18.59 +72:11:50.2: 12.90 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:30:18.59 +72:11:50.2: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.29 13:27:04.28 +72:07:49.8
119.09674 44.73145 galactic UMi Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:27:04.28 +72:07:49.8 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.034 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:04.28 +72:07:49.8: 12.89 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:04.28 +72:07:49.8: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.38 13:44:18.84 +70:54:55.5
116.79981 45.57807 galactic UMi Second-epoch detections are separated by 0.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:44:18.84 +70:54:55.5 (user input) | T | P | (position from user input) J-Ks=0.302+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:44:18.84 +70:54:55.5: 12.90 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:44:18.84 +70:54:55.5: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.01 12:53:47.77 +73:06:29.5
122.69370 44.01897 galactic Dra Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691183504974427392 | 12:53:47.82 +73:06:29.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.350+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:53:47.77 +73:06:29.5: 12.87 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:53:47.77 +73:06:29.5: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691183504974427392,2461335.6793,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691183504974427392 20261022.1793 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.18 13:18:32.27 +71:51:10.9
119.94724 45.11784 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:18:32.27 +71:51:10.9 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:32.27 +71:51:10.9: 12.89 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:32.27 +71:51:10.9: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.30 13:25:07.60 +71:30:29.7
119.14040 45.37118 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:25:07.60 +71:30:29.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:07.60 +71:30:29.7: 12.88 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:07.60 +71:30:29.7: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.09 12:53:37.32 +73:38:13.3
122.71989 43.49032 galactic Dra Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:53:37.32 +73:38:13.3 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:53:37.32 +73:38:13.3: 12.89 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:53:37.32 +73:38:13.3: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.01 12:46:02.58 +73:26:50.2
123.46315 43.67541 galactic Dra Second-epoch detections are separated by 0.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691393928307979136 | 12:46:02.52 +73:26:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.295+/-0.025 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:46:02.58 +73:26:50.2: 12.91 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:46:02.58 +73:26:50.2: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691393928307979136,2461335.6793,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691393928307979136 20261022.1793 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.12 12:45:47.38 +72:40:57.0
123.52056 44.43930 galactic Dra Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689658379267985920 | 12:45:47.46 +72:40:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.375+/-0.026 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:45:47.38 +72:40:57.0: 12.91 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:45:47.38 +72:40:57.0: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689658379267985920,2461335.6793,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689658379267985920 20261022.1793 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.02 13:00:03.31 +72:38:31.1
122.03142 44.47121 galactic Dra Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:00:03.31 +72:38:31.1 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:03.31 +72:38:31.1: 12.85 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:03.31 +72:38:31.1: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.68 12:51:43.56 +73:19:25.6
122.90328 43.80446 galactic Dra Second-epoch detections are separated by 1.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:51:43.56 +73:19:25.6 (user input) | T | P | (position from user input) J-Ks=0.616+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:51:43.56 +73:19:25.6: 13.92 +/- 0.07 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:51:43.56 +73:19:25.6: 14.03 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.97 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.05 13:21:11.75 +72:24:54.3
119.78630 44.53097 galactic UMi Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:11.75 +72:24:54.3 (user input) | T | P | (position from user input) J-Ks=0.307+/-0.035 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:11.75 +72:24:54.3: 12.85 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:11.75 +72:24:54.3: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.18 13:32:54.13 +72:02:59.2
118.45603 44.71637 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:32:54.13 +72:02:59.2 (user input) | T | P | (position from user input) J-Ks=0.549+/-0.034 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:54.13 +72:02:59.2: 12.86 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:54.13 +72:02:59.2: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.18 13:33:55.24 +71:21:23.3
118.12079 45.37284 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:33:55.24 +71:21:23.3 (user input) | T | P | (position from user input) J-Ks=0.312+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:33:55.24 +71:21:23.3: 12.85 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:33:55.24 +71:21:23.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.07 13:02:11.40 +72:52:54.1
121.82818 44.22351 galactic Dra Second-epoch detections are separated by 0.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:02:11.40 +72:52:54.1 (user input) | T | P | (position from user input) J-Ks=0.448+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:02:11.40 +72:52:54.1: 12.82 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:02:11.40 +72:52:54.1: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.11 13:26:11.69 +71:43:24.4
119.08039 45.14398 galactic UMi Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:26:11.69 +71:43:24.4 (user input) | T | P | (position from user input) J-Ks=0.425+/-0.027 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:26:11.69 +71:43:24.4: 12.85 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:26:11.69 +71:43:24.4: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.16 13:25:51.17 +72:01:49.7
119.19947 44.84753 galactic UMi Second-epoch detections are separated by 2.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:25:51.17 +72:01:49.7 (user input) | T | P | (position from user input) J-Ks=0.513+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:51.17 +72:01:49.7: 12.83 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:51.17 +72:01:49.7: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.06 13:10:56.33 +72:05:25.6
120.81536 44.95758 galactic UMi Second-epoch detections are separated by 0.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1688022069742926720 | 13:10:56.33 +72:05:25.6 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.316+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:10:56.33 +72:05:25.6: 12.84 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:10:56.33 +72:05:25.6: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1688022069742926720,2461335.6793,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1688022069742926720 20261022.1793 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.78 12:44:07.35 +73:18:47.2
123.65946 43.80480 galactic Dra Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691388843066695936 | 12:44:07.31 +73:18:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.583+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:44:07.35 +73:18:47.2: 12.62 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:44:07.35 +73:18:47.2: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691388843066695936,2461335.6793,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691388843066695936 20261022.1793 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.97 13:05:21.53 +72:25:45.3
121.45562 44.65908 galactic UMi Second-epoch detections are separated by 0.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:05:21.53 +72:25:45.3 (user input) | T | P | (position from user input) J-Ks=0.255+/-0.037 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:05:21.53 +72:25:45.3: 12.82 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:05:21.53 +72:25:45.3: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.02 12:42:32.14 +73:16:03.8
123.82015 43.84517 galactic Dra Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689899142250379392 | 12:42:32.12 +73:16:04.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.571+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:42:32.14 +73:16:03.8: 12.83 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:42:32.14 +73:16:03.8: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689899142250379392,2461335.6793,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689899142250379392 20261022.1793 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.64 13:36:46.97 +70:23:25.7
117.45739 46.25279 galactic UMi Second-epoch detections are separated by 2.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:36:46.97 +70:23:25.7 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:36:46.97 +70:23:25.7: 12.84 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:36:46.97 +70:23:25.7: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.03 12:38:00.58 +73:14:46.5
124.27308 43.84702 galactic Dra Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689942293785698048 | 12:38:00.78 +73:14:46.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.307+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:38:00.58 +73:14:46.5: 12.87 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:38:00.58 +73:14:46.5: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689942293785698048,2461335.6793,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689942293785698048 20261022.1793 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.25 13:34:29.57 +71:15:58.4
118.02709 45.44978 galactic UMi Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:34:29.57 +71:15:58.4 (user input) | T | P | (position from user input) J-Ks=0.371+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:34:29.57 +71:15:58.4: 12.83 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:34:29.57 +71:15:58.4: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.95 13:07:43.13 +72:45:32.8
121.24704 44.31584 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688123259172497280 | 13:07:52.41 +72:45:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.633+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:43.13 +72:45:32.8: 12.82 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:43.13 +72:45:32.8: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688123259172497280,2461335.6793,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688123259172497280 20261022.1793 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.16 15:28:43.89 +66:32:41.9
102.47170 43.81575 galactic UMi Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:28:43.89 +66:32:41.9 (user input) | T | P | (position from user input) J-Ks=0.379+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:28:43.89 +66:32:41.9: 12.80 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:28:43.89 +66:32:41.9: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.03 12:56:54.39 +73:23:00.8
122.39085 43.73895 galactic Dra Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691170280771009536 | 12:56:54.48 +73:23:00.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.367+/-0.025 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:54.39 +73:23:00.8: 12.80 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:54.39 +73:23:00.8: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691170280771009536,2461335.6793,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691170280771009536 20261022.1793 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.10 12:59:27.94 +72:23:49.7
122.07793 44.71780 galactic Dra Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689600693563322880 | 12:59:27.78 +72:23:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.393+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:27.94 +72:23:49.7: 12.80 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:27.94 +72:23:49.7: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689600693563322880,2461335.6793,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689600693563322880 20261022.1793 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.13 13:26:01.91 +71:22:30.4
119.00390 45.48838 galactic UMi Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687010927066530560 | 13:26:01.83 +71:22:30.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.603+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:26:01.91 +71:22:30.4: 12.80 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:26:01.91 +71:22:30.4: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687010927066530560,2461335.6793,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687010927066530560 20261022.1793 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.49 13:32:45.22 +72:24:54.7
118.58651 44.36280 galactic UMi Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:32:45.22 +72:24:54.7 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:45.22 +72:24:54.7: 12.80 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:45.22 +72:24:54.7: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.09 13:30:35.62 +72:05:15.3
118.71167 44.71842 galactic UMi Second-epoch detections are separated by 0.5" and 7.3 pix
The object was found in VSX 0" Gaia DR3 1687147717480830208
Type: VAR
# Max. Min./Amp. JD0 Period
12.450 G 12.670 G 0.067411200000 K
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:30:35.62 +72:05:15.3: 12.78 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:30:35.62 +72:05:15.3: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687147717480830208,2461335.6793,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687147717480830208 20261022.1793 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.30 12:57:46.68 +73:39:23.0
122.31747 43.46430 galactic Dra Second-epoch detections are separated by 2.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691273669223730432 | 12:57:46.50 +73:39:22.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.459+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:57:46.68 +73:39:23.0: 12.78 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:57:46.68 +73:39:23.0: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691273669223730432,2461335.6793,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691273669223730432 20261022.1793 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.88 13:11:07.42 +72:13:00.7
120.81463 44.83037 galactic UMi Second-epoch detections are separated by 0.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688046357782371712 | 13:11:07.23 +72:13:01.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.804+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:11:07.42 +72:13:00.7: 12.77 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:11:07.42 +72:13:00.7: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688046357782371712,2461335.6793,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688046357782371712 20261022.1793 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.02 13:15:02.19 +72:13:36.0
120.39824 44.78531 galactic UMi Second-epoch detections are separated by 0.4" and 7.4 pix
The object was found in VSX 0" Gaia DR3 1687861987722042368
Type: ROT
# Max. Min./Amp. JD0 Period
12.500 G 12.540 G G
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:02.19 +72:13:36.0: 12.77 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:02.19 +72:13:36.0: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687861987722042368,2461335.6793,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687861987722042368 20261022.1793 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.10 13:13:55.31 +72:54:06.9
120.63270 44.12582 galactic UMi Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688163421410823552 | 13:13:55.54 +72:54:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.276+/-0.032 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:13:55.31 +72:54:06.9: 12.78 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:13:55.31 +72:54:06.9: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688163421410823552,2461335.6793,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688163421410823552 20261022.1793 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.29 13:01:07.46 +72:00:39.1
121.87271 45.09746 galactic Dra Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686583874174903424 | 13:01:07.57 +72:00:38.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.510+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:07.46 +72:00:39.1: 12.77 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:07.46 +72:00:39.1: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686583874174903424,2461335.6793,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686583874174903424 20261022.1793 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.96 13:01:27.38 +72:29:55.0
121.87419 44.60906 galactic Dra Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688101028422377472 | 13:01:27.54 +72:29:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.447+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:27.38 +72:29:55.0: 12.77 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:27.38 +72:29:55.0: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688101028422377472,2461335.6793,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688101028422377472 20261022.1793 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.36 13:25:38.02 +70:53:08.5
118.91551 45.97496 galactic UMi Second-epoch detections are separated by 1.0" and 7.5 pix
The object was found in VSX 2" Gaia DR3 1686970180712560128
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.540 G 12.570 G G
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:38.02 +70:53:08.5: 12.77 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:38.02 +70:53:08.5: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686970180712560128,2461335.6793,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686970180712560128 20261022.1793 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.07 13:03:23.25 +73:20:26.6
121.74659 43.76002 galactic Dra Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691251331098044160 | 13:03:23.15 +73:20:26.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.340+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:03:23.25 +73:20:26.6: 12.75 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:03:23.25 +73:20:26.6: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691251331098044160,2461335.6793,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691251331098044160 20261022.1793 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.27 13:26:52.74 +72:29:14.7
119.21349 44.38406 galactic UMi Second-epoch detections are separated by 1.3" and 7.1 pix
The object was found in VSX 3" Gaia DR3 1687916757144883328
Type: ROT
# Max. Min./Amp. JD0 Period
13.030 G 13.060 G G
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:26:52.74 +72:29:14.7: 12.76 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:26:52.74 +72:29:14.7: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687916757144883328,2461335.6793,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687916757144883328 20261022.1793 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.05 13:19:07.73 +71:38:23.1
119.83666 45.32171 galactic UMi Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1687806050067924992 | 13:19:07.73 +71:38:23.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.349+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:07.73 +71:38:23.1: 12.75 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:07.73 +71:38:23.1: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1687806050067924992,2461335.6793,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1687806050067924992 20261022.1793 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.93 13:08:39.58 +72:36:27.7
121.13020 44.46026 galactic UMi Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688073334472641536 | 13:08:39.46 +72:36:27.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.427+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:08:39.58 +72:36:27.7: 12.75 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:08:39.58 +72:36:27.7: 12.76 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688073334472641536,2461335.6793,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688073334472641536 20261022.1793 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.13 13:01:54.63 +73:25:18.7
121.89921 43.68538 galactic Dra Second-epoch detections are separated by 1.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:01:54.63 +73:25:18.7 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:54.63 +73:25:18.7: 12.75 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:54.63 +73:25:18.7: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.04 13:21:38.43 +72:25:09.0
119.74076 44.52147 galactic UMi Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:38.43 +72:25:09.0 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:38.43 +72:25:09.0: 12.75 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:38.43 +72:25:09.0: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.09 13:28:19.69 +71:29:48.9
118.78282 45.33297 galactic UMi Second-epoch detections are separated by 2.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:28:19.69 +71:29:48.9 (user input) | T | P | (position from user input) J-Ks=0.517+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:19.69 +71:29:48.9: 12.75 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:19.69 +71:29:48.9: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.00 13:18:41.07 +72:34:08.8
120.08117 44.40802 galactic UMi Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687964547245157504 | 13:18:41.09 +72:34:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.429+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:41.07 +72:34:08.8: 12.73 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:41.07 +72:34:08.8: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687964547245157504,2461335.6793,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687964547245157504 20261022.1793 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.46 13:33:08.25 +70:43:28.4
117.99888 46.00222 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1686920427811592832 | 13:33:08.25 +70:43:28.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.385+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:33:08.25 +70:43:28.4: 12.74 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:33:08.25 +70:43:28.4: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1686920427811592832,2461335.6793,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1686920427811592832 20261022.1793 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.23 13:44:18.13 +71:01:29.2
116.84647 45.47370 galactic UMi Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:44:18.13 +71:01:29.2 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:44:18.13 +71:01:29.2: 12.72 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:44:18.13 +71:01:29.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.08 13:22:51.32 +72:33:44.9
119.64811 44.36491 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687973107115857536 | 13:22:51.34 +72:33:45.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.467+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:22:51.32 +72:33:44.9: 12.72 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:22:51.32 +72:33:44.9: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687973107115857536,2461335.6793,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687973107115857536 20261022.1793 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.28 13:40:17.14 +71:20:14.4
117.41328 45.26387 galactic UMi Second-epoch detections are separated by 1.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:40:17.14 +71:20:14.4 (user input) | T | P | (position from user input) J-Ks=0.356+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:40:17.14 +71:20:14.4: 12.72 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:40:17.14 +71:20:14.4: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.16 12:59:18.43 +72:06:04.4
122.07678 45.01396 galactic Dra Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686588444019659136 | 12:59:18.65 +72:06:05.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.404+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:18.43 +72:06:04.4: 12.71 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:18.43 +72:06:04.4: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686588444019659136,2461335.6793,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686588444019659136 20261022.1793 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.10 13:34:59.54 +71:46:21.3
118.14300 44.94848 galactic UMi Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687081433249619840 | 13:34:59.59 +71:46:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.545+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:34:59.54 +71:46:21.3: 12.73 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:34:59.54 +71:46:21.3: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687081433249619840,2461335.6793,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687081433249619840 20261022.1793 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.88 13:01:13.53 +72:36:59.1
121.90735 44.49236 galactic Dra Second-epoch detections are separated by 1.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688108553204511744 | 13:01:13.44 +72:36:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.395+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:13.53 +72:36:59.1: 12.71 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:13.53 +72:36:59.1: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688108553204511744,2461335.6793,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688108553204511744 20261022.1793 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.93 12:59:48.61 +72:54:01.2
122.07342 44.21396 galactic Dra Second-epoch detections are separated by 1.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691141792252451712 | 12:59:48.57 +72:54:00.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.671+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:48.61 +72:54:01.2: 12.70 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:48.61 +72:54:01.2: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691141792252451712,2461335.6793,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691141792252451712 20261022.1793 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.18 13:29:26.24 +71:09:19.0
118.55825 45.64891 galactic UMi Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:29:26.24 +71:09:19.0 (user input) | T | P | (position from user input) J-Ks=0.297+/-0.027 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:29:26.24 +71:09:19.0: 12.71 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:29:26.24 +71:09:19.0: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.94 13:16:44.77 +71:50:45.0
120.14149 45.14505 galactic UMi Second-epoch detections are separated by 1.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687835423348774784 | 13:16:44.77 +71:50:45.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.674+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:16:44.77 +71:50:45.0: 12.69 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:16:44.77 +71:50:45.0: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687835423348774784,2461335.6793,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687835423348774784 20261022.1793 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.25 13:31:41.30 +70:58:43.2
118.24818 45.78179 galactic UMi Second-epoch detections are separated by 1.0" and 7.4 pix
The object was found in VSX 1" Gaia DR3 1686939531825907584
Type: ROT
# Max. Min./Amp. JD0 Period
12.460 G 12.490 G G
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:31:41.30 +70:58:43.2: 12.70 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:31:41.30 +70:58:43.2: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686939531825907584,2461335.6793,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686939531825907584 20261022.1793 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.94 13:04:27.57 +72:47:52.2
121.58738 44.29641 galactic UMi Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688137720327215488 | 13:04:27.53 +72:47:52.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.327+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:04:27.57 +72:47:52.2: 12.68 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:04:27.57 +72:47:52.2: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688137720327215488,2461335.6793,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688137720327215488 20261022.1793 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.20 13:00:22.15 +73:31:39.7
122.05805 43.58540 galactic Dra Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691257142189563904 | 13:00:22.18 +73:31:38.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.333+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:22.15 +73:31:39.7: 12.69 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:22.15 +73:31:39.7: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691257142189563904,2461335.6793,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691257142189563904 20261022.1793 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.09 13:22:19.72 +71:26:12.9
119.43394 45.48095 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:22:19.72 +71:26:12.9 (user input) | T | P | (position from user input) J-Ks=0.278+/-0.052 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:22:19.72 +71:26:12.9: 12.70 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:22:19.72 +71:26:12.9: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.95 13:08:16.60 +72:54:34.7
121.20866 44.16223 galactic UMi Second-epoch detections are separated by 0.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688218431352322048 | 13:08:16.53 +72:54:34.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.662+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:08:16.60 +72:54:34.7: 12.68 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:08:16.60 +72:54:34.7: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688218431352322048,2461335.6793,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688218431352322048 20261022.1793 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.84 12:58:14.71 +72:56:30.5
122.23593 44.17725 galactic Dra Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691142689901080064 | 12:58:14.77 +72:56:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.386+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:14.71 +72:56:30.5: 12.68 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:14.71 +72:56:30.5: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691142689901080064,2461335.6793,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691142689901080064 20261022.1793 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.38 12:59:55.35 +73:40:22.7
122.11082 43.44175 galactic Dra Second-epoch detections are separated by 1.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691271809502191360 | 12:59:55.25 +73:40:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.308+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:55.35 +73:40:22.7: 12.69 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:55.35 +73:40:22.7: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691271809502191360,2461335.6793,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691271809502191360 20261022.1793 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.98 13:20:06.04 +71:40:53.7
119.73854 45.26853 galactic UMi Second-epoch detections are separated by 0.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687782921668557312 | 13:20:06.14 +71:40:53.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.386+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:20:06.04 +71:40:53.7: 12.68 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:20:06.04 +71:40:53.7: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687782921668557312,2461335.6793,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687782921668557312 20261022.1793 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.10 13:31:48.45 +71:15:56.7
118.32620 45.49977 galactic UMi Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686949869811401344 | 13:31:48.46 +71:15:56.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.653+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:31:48.45 +71:15:56.7: 12.69 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:31:48.45 +71:15:56.7: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686949869811401344,2461335.6793,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686949869811401344 20261022.1793 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.02 13:32:13.19 +71:33:08.7
118.37161 45.21300 galactic UMi Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:32:13.19 +71:33:08.7 (user input) | T | P | (position from user input) J-Ks=0.517+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:13.19 +71:33:08.7: 12.68 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:13.19 +71:33:08.7: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.18 12:58:42.80 +72:05:27.3
122.14068 45.02616 galactic Dra Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689589389208891008 | 12:58:42.68 +72:05:26.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.258+/-0.032 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:42.80 +72:05:27.3: 12.69 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:42.80 +72:05:27.3: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689589389208891008,2461335.6793,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689589389208891008 20261022.1793 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.14 13:19:37.39 +71:23:41.3
119.72765 45.55768 galactic UMi Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687754815402570112 | 13:19:37.42 +71:23:41.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.354+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:37.39 +71:23:41.3: 12.68 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:37.39 +71:23:41.3: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687754815402570112,2461335.6793,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687754815402570112 20261022.1793 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.46 13:33:04.68 +72:21:22.5
118.53455 44.41475 galactic UMi Second-epoch detections are separated by 1.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687533096306295168 | 13:33:04.80 +72:21:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.461+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:33:04.68 +72:21:22.5: 12.68 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:33:04.68 +72:21:22.5: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687533096306295168,2461335.6793,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687533096306295168 20261022.1793 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.93 12:43:15.10 +73:28:01.8
123.73662 43.64829 galactic Dra Second-epoch detections are separated by 0.3" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691403342876295552 | 12:43:15.16 +73:28:02.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.436+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:43:15.10 +73:28:01.8: 12.70 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:43:15.10 +73:28:01.8: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691403342876295552,2461335.6793,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691403342876295552 20261022.1793 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.89 12:51:36.05 +72:53:33.5
122.91520 44.23561 galactic Dra Second-epoch detections are separated by 0.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691176736105974144 | 12:51:36.10 +72:53:33.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.399+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:51:36.05 +72:53:33.5: 12.66 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:51:36.05 +72:53:33.5: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691176736105974144,2461335.6793,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691176736105974144 20261022.1793 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.09 13:03:17.60 +73:14:32.6
121.74722 43.85858 galactic Dra Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688242281306398848 | 13:03:17.47 +73:14:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.306+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:03:17.60 +73:14:32.6: 12.65 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:03:17.60 +73:14:32.6: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688242281306398848,2461335.6793,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688242281306398848 20261022.1793 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.97 12:49:19.04 +73:42:45.5
123.13660 43.41477 galactic Dra Second-epoch detections are separated by 0.5" and 7.6 pix
The object was found in VSX 1" Gaia DR3 1691239756162049152
Type: E
# Max. Min./Amp. JD0 Period
12.920 G 13.160 G 0.200076000000
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:49:19.04 +73:42:45.5: 12.68 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:49:19.04 +73:42:45.5: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691239756162049152,2461335.6793,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691239756162049152 20261022.1793 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.92 13:19:54.76 +72:02:26.1
119.83871 44.91626 galactic UMi Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687842196512709760 | 13:19:54.64 +72:02:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.456+/-0.035 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:54.76 +72:02:26.1: 12.66 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:54.76 +72:02:26.1: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687842196512709760,2461335.6793,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687842196512709760 20261022.1793 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.90 13:01:39.47 +72:18:56.2
121.83858 44.79094 galactic Dra Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688094878028622464 | 13:01:39.49 +72:18:56.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.380+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:39.47 +72:18:56.2: 12.66 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:39.47 +72:18:56.2: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688094878028622464,2461335.6793,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688094878028622464 20261022.1793 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.84 13:17:03.17 +71:48:26.8
120.10030 45.17971 galactic UMi Second-epoch detections are separated by 0.4" and 7.4 pix
The object was found in VSX 1" Gaia DR3 1687835049687117952
Type: ROT
# Max. Min./Amp. JD0 Period
12.410 G 12.440 G G
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:17:03.17 +71:48:26.8: 12.65 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:17:03.17 +71:48:26.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687835049687117952,2461335.6793,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687835049687117952 20261022.1793 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.63 12:42:13.46 +73:02:14.2
123.86709 44.07424 galactic Dra Second-epoch detections are separated by 1.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:42:13.46 +73:02:14.2 (user input) | T | P | (position from user input) J-Ks=0.427+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:42:13.46 +73:02:14.2: 13.92 +/- 0.07 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:42:13.46 +73:02:14.2: 13.98 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.86 12:39:30.60 +72:52:10.6
124.15725 44.23025 galactic Dra Second-epoch detections are separated by 0.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689860899861550336 | 12:39:30.39 +72:52:11.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.915+/-0.026 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:39:30.60 +72:52:10.6: 12.65 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:39:30.60 +72:52:10.6: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689860899861550336,2461335.6793,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689860899861550336 20261022.1793 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.07 13:25:23.90 +72:27:25.4
119.35878 44.43483 galactic UMi Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687927443023514624 | 13:25:23.93 +72:27:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.468+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:23.90 +72:27:25.4: 12.65 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:23.90 +72:27:25.4: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687927443023514624,2461335.6793,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687927443023514624 20261022.1793 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.53 13:36:53.39 +72:04:01.7
118.04215 44.62706 galactic UMi Second-epoch detections are separated by 1.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:36:53.39 +72:04:01.7 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:36:53.39 +72:04:01.7: 12.66 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:36:53.39 +72:04:01.7: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.24 15:27:01.80 +66:33:21.5
102.63087 43.94069 galactic UMi Second-epoch detections are separated by 2.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:27:01.80 +66:33:21.5 (user input) | T | P | (position from user input) J-Ks=0.300+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:27:01.80 +66:33:21.5: 12.64 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:27:01.80 +66:33:21.5: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.48 13:01:11.16 +73:48:31.4
121.99839 43.30186 galactic Dra Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691285798211382016 | 13:01:11.15 +73:48:31.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.359+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:11.16 +73:48:31.4: 12.63 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:11.16 +73:48:31.4: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691285798211382016,2461335.6793,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691285798211382016 20261022.1793 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.16 15:28:57.10 +66:27:31.1
102.35912 43.85236 galactic UMi Second-epoch detections are separated by 2.5" and 6.2 pix
The object was found in VSX 0" ZKRA-V1
Type: DSCT
# Max. Min./Amp. JD0 Period
12.410 V 12.500 V 2460204.45500 0.065939500000
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:28:57.10 +66:27:31.1: 12.64 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:28:57.10 +66:27:31.1: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZKRA-V1,2461335.6793,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZKRA-V1 20261022.1793 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.92 13:27:37.84 +71:47:18.5
118.94213 45.05835 galactic UMi Second-epoch detections are separated by 0.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687116686341184768 | 13:27:37.76 +71:47:19.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.663+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:37.84 +71:47:18.5: 12.62 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:37.84 +71:47:18.5: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687116686341184768,2461335.6793,10.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687116686341184768 20261022.1793 10.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.12 13:00:10.37 +72:03:17.6
121.97964 45.05721 galactic Dra Second-epoch detections are separated by 1.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686587340211883776 | 13:00:10.20 +72:03:17.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.523+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:10.37 +72:03:17.6: 12.63 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:10.37 +72:03:17.6: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686587340211883776,2461335.6793,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686587340211883776 20261022.1793 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.29 12:49:00.94 +72:24:24.9
123.18951 44.72012 galactic Dra Second-epoch detections are separated by 0.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689638691137490560 | 12:49:00.93 +72:24:24.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.388+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:49:00.94 +72:24:24.9: 12.63 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:49:00.94 +72:24:24.9: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689638691137490560,2461335.6793,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689638691137490560 20261022.1793 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.96 13:20:36.16 +72:00:44.9
119.75821 44.93563 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687841200080255232 | 13:20:36.14 +72:00:45.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.276+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:20:36.16 +72:00:44.9: 12.63 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:20:36.16 +72:00:44.9: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687841200080255232,2461335.6793,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687841200080255232 20261022.1793 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.09 13:31:41.01 +72:09:42.0
118.61930 44.62805 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687154761227199488 | 13:31:41.11 +72:09:41.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.356+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:31:41.01 +72:09:42.0: 12.63 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:31:41.01 +72:09:42.0: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687154761227199488,2461335.6793,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687154761227199488 20261022.1793 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.04 13:27:08.57 +72:23:21.6
119.15968 44.47647 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687914347667397632 | 13:27:08.62 +72:23:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.335+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:08.57 +72:23:21.6: 12.62 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:08.57 +72:23:21.6: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687914347667397632,2461335.6793,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687914347667397632 20261022.1793 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.80 12:37:56.18 +73:19:38.4
124.27224 43.76576 galactic Dra Second-epoch detections are separated by 0.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689944290946604800 | 12:37:56.05 +73:19:38.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.387+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:37:56.18 +73:19:38.4: 12.74 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:37:56.18 +73:19:38.4: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689944290946604800,2461335.6793,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689944290946604800 20261022.1793 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.15 13:06:53.34 +71:45:28.9
121.21336 45.31863 galactic UMi Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686523332315362560 | 13:06:53.28 +71:45:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.663+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:53.34 +71:45:28.9: 12.61 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:53.34 +71:45:28.9: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686523332315362560,2461335.6793,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686523332315362560 20261022.1793 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.82 13:00:19.85 +73:03:09.9
122.03030 44.05993 galactic Dra Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691150077245421440 | 13:00:20.01 +73:03:10.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.484+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:19.85 +73:03:09.9: 12.60 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:19.85 +73:03:09.9: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691150077245421440,2461335.6793,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691150077245421440 20261022.1793 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.89 13:05:50.96 +73:04:52.6
121.47501 44.00618 galactic UMi Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688236749388492416 | 13:05:51.02 +73:04:52.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.092+/-0.033 (A)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:05:50.96 +73:04:52.6: 12.60 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:05:50.96 +73:04:52.6: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688236749388492416,2461335.6793,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688236749388492416 20261022.1793 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.94 13:22:48.03 +72:00:00.3
119.51889 44.91975 galactic UMi Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687884458990829056 | 13:22:48.03 +72:00:00.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.317+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:22:48.03 +72:00:00.3: 12.60 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:22:48.03 +72:00:00.3: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687884458990829056,2461335.6793,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687884458990829056 20261022.1793 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.15 12:58:30.90 +73:39:51.8
122.24650 43.45444 galactic Dra Second-epoch detections are separated by 1.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691273875382160128 | 12:58:31.11 +73:39:51.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.426+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:30.90 +73:39:51.8: 12.59 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:30.90 +73:39:51.8: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691273875382160128,2461335.6793,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691273875382160128 20261022.1793 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.88 12:44:20.69 +73:04:03.1
123.65040 44.05083 galactic Dra Second-epoch detections are separated by 1.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689883680368049792 | 12:44:20.87 +73:04:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.282+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:44:20.69 +73:04:03.1: 12.62 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:44:20.69 +73:04:03.1: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689883680368049792,2461335.6793,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689883680368049792 20261022.1793 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.91 15:28:35.36 +66:28:09.1
102.40182 43.87409 galactic UMi Second-epoch detections are separated by 0.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644717014009054592 | 15:28:35.47 +66:28:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.681+/-0.032 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:28:35.36 +66:28:09.1: 12.61 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:28:35.36 +66:28:09.1: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644717014009054592,2461335.6793,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644717014009054592 20261022.1793 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.01 13:32:26.42 +71:26:46.4
118.31353 45.31256 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687093429094173568 | 13:32:26.45 +71:26:46.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.354+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:26.42 +71:26:46.4: 12.60 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:26.42 +71:26:46.4: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687093429094173568,2461335.6793,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687093429094173568 20261022.1793 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.88 13:00:17.61 +73:18:02.6
122.05052 43.81237 galactic Dra Second-epoch detections are separated by 1.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691247315304834432 | 13:00:17.62 +73:18:02.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.345+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:17.61 +73:18:02.6: 12.58 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:17.61 +73:18:02.6: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691247315304834432,2461335.6793,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691247315304834432 20261022.1793 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.89 12:59:09.66 +72:19:15.5
122.10578 44.79489 galactic Dra Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689598524603237120 | 12:59:09.79 +72:19:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.331+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:09.66 +72:19:15.5: 12.58 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:09.66 +72:19:15.5: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689598524603237120,2461335.6793,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689598524603237120 20261022.1793 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.94 13:15:10.93 +71:40:05.6
120.27968 45.33755 galactic UMi Second-epoch detections are separated by 0.5" and 7.4 pix
The object was found in VSX 2" Gaia DR3 1687815116743402368
Type: ROT
# Max. Min./Amp. JD0 Period
12.310 G 12.340 G K
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:10.93 +71:40:05.6: 12.58 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:10.93 +71:40:05.6: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687815116743402368,2461335.6793,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687815116743402368 20261022.1793 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.06 13:33:40.87 +71:40:50.5
118.25388 45.06189 galactic UMi Second-epoch detections are separated by 0.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687125963470547072 | 13:33:41.03 +71:40:50.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.406+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:33:40.87 +71:40:50.5: 12.60 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:33:40.87 +71:40:50.5: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687125963470547072,2461335.6793,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687125963470547072 20261022.1793 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.26 13:11:40.69 +73:16:13.9
120.91679 43.77844 galactic UMi Second-epoch detections are separated by 0.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J197.9023+73.2647 | 13:11:40.86 +73:16:14.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.282+/-0.036 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:11:40.69 +73:16:13.9: 12.56 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:11:40.69 +73:16:13.9: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J197.9023+73.2647,2461335.6793,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J197.9023+73.2647 20261022.1793 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.21 13:37:38.92 +71:42:32.2
117.83592 44.95927 galactic UMi Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687070682947356160 | 13:37:38.81 +71:42:32.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.592+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:37:38.92 +71:42:32.2: 12.58 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:37:38.92 +71:42:32.2: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687070682947356160,2461335.6793,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687070682947356160 20261022.1793 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.88 13:14:57.57 +72:44:33.8
120.49904 44.27425 galactic UMi Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688158542327979008 | 13:14:57.57 +72:44:34.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.779+/-0.037 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:57.57 +72:44:33.8: 12.56 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:57.57 +72:44:33.8: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688158542327979008,2461335.6793,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688158542327979008 20261022.1793 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.75 12:53:05.28 +73:01:37.1
122.76423 44.10074 galactic Dra Second-epoch detections are separated by 1.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691182031801549824 | 12:53:05.24 +73:01:36.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.690+/-0.032 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:53:05.28 +73:01:37.1: 12.56 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:53:05.28 +73:01:37.1: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691182031801549824,2461335.6793,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691182031801549824 20261022.1793 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.89 13:10:07.76 +72:55:54.2
121.02293 44.12718 galactic UMi Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688178161738954112 | 13:10:07.80 +72:55:53.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.305+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:10:07.76 +72:55:54.2: 12.56 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:10:07.76 +72:55:54.2: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688178161738954112,2461335.6793,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688178161738954112 20261022.1793 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.79 13:01:32.18 +72:37:38.2
121.87569 44.48026 galactic Dra Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688108415766128128 | 13:01:32.34 +72:37:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:32.18 +72:37:38.2: 12.55 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:32.18 +72:37:38.2: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688108415766128128,2461335.6793,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688108415766128128 20261022.1793 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.09 13:31:33.28 +72:04:33.9
118.60661 44.71372 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687152630923416320 | 13:31:33.24 +72:04:33.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.294+/-0.035 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:31:33.28 +72:04:33.9: 12.57 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:31:33.28 +72:04:33.9: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687152630923416320,2461335.6793,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687152630923416320 20261022.1793 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.16 13:35:27.28 +70:59:16.7
117.82378 45.70122 galactic UMi Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686930800156842240 | 13:35:27.46 +70:59:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.579+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:35:27.28 +70:59:16.7: 12.56 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:35:27.28 +70:59:16.7: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686930800156842240,2461335.6793,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686930800156842240 20261022.1793 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.78 12:56:30.64 +72:54:58.5
122.41223 44.20688 galactic Dra Second-epoch detections are separated by 1.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691130144300746752 | 12:56:30.62 +72:54:59.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.579+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:30.64 +72:54:58.5: 12.54 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:30.64 +72:54:58.5: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691130144300746752,2461335.6793,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691130144300746752 20261022.1793 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.81 12:50:07.55 +72:52:27.4
123.06677 44.25363 galactic Dra Second-epoch detections are separated by 2.1" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1689687829858473088 | 12:50:07.55 +72:52:27.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.559+/-0.076 (Very red! L if it's a dwarf)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:50:07.55 +72:52:27.4: 12.54 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:50:07.55 +72:52:27.4: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1689687829858473088,2461335.6793,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1689687829858473088 20261022.1793 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.17 13:18:38.01 +72:55:44.6
120.16033 44.05255 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688001866216917888 | 13:18:38.10 +72:55:44.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.361+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:38.01 +72:55:44.6: 12.55 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:38.01 +72:55:44.6: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688001866216917888,2461335.6793,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688001866216917888 20261022.1793 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.93 13:12:41.18 +72:27:00.4
120.68551 44.58534 galactic UMi Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688056425185702656 | 13:12:40.95 +72:27:00.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.397+/-0.035 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:12:41.18 +72:27:00.4: 12.55 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:12:41.18 +72:27:00.4: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688056425185702656,2461335.6793,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688056425185702656 20261022.1793 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.79 12:49:08.21 +73:19:04.7
123.16075 43.80926 galactic Dra Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691203609717268864 | 12:49:08.33 +73:19:04.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.365+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:49:08.21 +73:19:04.7: 12.58 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:49:08.21 +73:19:04.7: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691203609717268864,2461335.6793,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691203609717268864 20261022.1793 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.02 13:22:57.38 +71:26:45.7
119.36603 45.46337 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687764058172196992 | 13:22:57.45 +71:26:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:22:57.38 +71:26:45.7: 12.55 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:22:57.38 +71:26:45.7: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687764058172196992,2461335.6793,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687764058172196992 20261022.1793 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.13 13:14:05.92 +73:07:24.7
120.65237 43.90429 galactic UMi Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688201835598684416 | 13:14:05.95 +73:07:24.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.302+/-0.034 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:05.92 +73:07:24.7: 12.53 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:05.92 +73:07:24.7: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688201835598684416,2461335.6793,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688201835598684416 20261022.1793 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.76 12:52:18.39 +73:31:17.5
122.84685 43.60658 galactic Dra Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691222026537040384 | 12:52:18.41 +73:31:17.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:52:18.39 +73:31:17.5: 12.54 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:52:18.39 +73:31:17.5: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691222026537040384,2461335.6793,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691222026537040384 20261022.1793 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.01 13:12:34.00 +71:40:43.6
120.57182 45.35253 galactic UMi Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687818243479312256 | 13:12:33.98 +71:40:43.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.625+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:12:34.00 +71:40:43.6: 12.53 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:12:34.00 +71:40:43.6: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687818243479312256,2461335.6793,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687818243479312256 20261022.1793 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.88 13:19:40.86 +72:10:33.9
119.89312 44.78515 galactic UMi Second-epoch detections are separated by 1.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687937098110505216 | 13:19:40.84 +72:10:33.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.486+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:40.86 +72:10:33.9: 12.52 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:40.86 +72:10:33.9: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687937098110505216,2461335.6793,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687937098110505216 20261022.1793 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.04 13:35:54.74 +71:15:19.2
117.86565 45.43290 galactic UMi Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687034605222050560 | 13:35:54.83 +71:15:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.400+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:35:54.74 +71:15:19.2: 12.54 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:35:54.74 +71:15:19.2: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687034605222050560,2461335.6793,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687034605222050560 20261022.1793 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.68 13:06:48.64 +72:26:55.8
121.30439 44.63081 galactic UMi Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:06:48.64 +72:26:55.8 (user input) | T | P | (position from user input) J-Ks=0.509+/-0.035 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:48.64 +72:26:55.8: 12.51 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:48.64 +72:26:55.8: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.77 13:18:21.95 +72:06:23.4
120.01889 44.86913 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687846182242365056 | 13:18:21.78 +72:06:23.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.475+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:21.95 +72:06:23.4: 12.51 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:21.95 +72:06:23.4: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687846182242365056,2461335.6793,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687846182242365056 20261022.1793 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.35 13:30:10.78 +70:33:21.9
118.28901 46.22134 galactic UMi Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686900911479962240 | 13:30:10.80 +70:33:22.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.539+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:30:10.78 +70:33:21.9: 12.52 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:30:10.78 +70:33:21.9: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686900911479962240,2461335.6793,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686900911479962240 20261022.1793 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.81 12:45:53.95 +72:47:08.0
123.50482 44.33653 galactic Dra Second-epoch detections are separated by 0.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689870241414760576 | 12:45:53.98 +72:47:07.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.187+/-0.025 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:45:53.95 +72:47:08.0: 12.53 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:45:53.95 +72:47:08.0: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689870241414760576,2461335.6793,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689870241414760576 20261022.1793 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.46 12:50:00.76 +72:46:21.6
123.07950 44.35518 galactic Dra Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689673875509993344 | 12:50:00.78 +72:46:20.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.556+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:50:00.76 +72:46:21.6: 12.17 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:50:00.76 +72:46:21.6: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689673875509993344,2461335.6793,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689673875509993344 20261022.1793 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.43 12:44:45.40 +73:28:34.8
123.58831 43.64340 galactic Dra Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691397467361082624 | 12:44:45.43 +73:28:35.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.687+/-0.023 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:44:45.40 +73:28:34.8: 12.17 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:44:45.40 +73:28:34.8: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691397467361082624,2461335.6793,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691397467361082624 20261022.1793 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.90 13:00:11.37 +72:16:50.2
121.99314 44.83168 galactic Dra Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686597064017838464 | 13:00:11.46 +72:16:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.517+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:11.37 +72:16:50.2: 12.48 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:11.37 +72:16:50.2: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686597064017838464,2461335.6793,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686597064017838464 20261022.1793 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.72 13:05:36.91 +72:15:20.6
121.40958 44.83060 galactic UMi Second-epoch detections are separated by 1.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688079858527279744 | 13:05:36.87 +72:15:20.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.468+/-0.050 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:05:36.91 +72:15:20.6: 12.49 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:05:36.91 +72:15:20.6: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688079858527279744,2461335.6793,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688079858527279744 20261022.1793 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.22 13:01:36.16 +73:35:42.3
121.94256 43.51364 galactic Dra Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691258718441712640 | 13:01:36.25 +73:35:42.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.583+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:36.16 +73:35:42.3: 12.49 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:36.16 +73:35:42.3: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691258718441712640,2461335.6793,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691258718441712640 20261022.1793 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.03 13:35:52.59 +71:40:36.9
118.01539 45.02471 galactic UMi Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687076794685703680 | 13:35:52.33 +71:40:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.634+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:35:52.59 +71:40:36.9: 12.47 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:35:52.59 +71:40:36.9: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687076794685703680,2461335.6793,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687076794685703680 20261022.1793 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.84 13:19:53.73 +71:41:05.4
119.76188 45.26785 galactic UMi Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687782887308812544 | 13:19:53.73 +71:41:05.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.573+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:53.73 +71:41:05.4: 12.47 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:53.73 +71:41:05.4: 12.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687782887308812544,2461335.6793,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687782887308812544 20261022.1793 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.04 13:26:06.62 +70:54:58.2
118.86887 45.93758 galactic UMi Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686970661748899456 | 13:26:06.70 +70:54:58.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.705+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:26:06.62 +70:54:58.2: 12.49 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:26:06.62 +70:54:58.2: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686970661748899456,2461335.6793,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686970661748899456 20261022.1793 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.31 13:36:03.99 +70:46:41.7
117.68033 45.89224 galactic UMi Second-epoch detections are separated by 1.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686923691986480128 | 13:36:04.11 +70:46:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.314+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:36:03.99 +70:46:41.7: 12.49 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:36:03.99 +70:46:41.7: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686923691986480128,2461335.6793,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686923691986480128 20261022.1793 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.40 13:36:22.02 +70:31:25.0
117.55440 46.13268 galactic UMi Second-epoch detections are separated by 1.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686726260929970816 | 13:36:21.94 +70:31:24.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.317+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:36:22.02 +70:31:25.0: 12.47 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:36:22.02 +70:31:25.0: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686726260929970816,2461335.6793,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686726260929970816 20261022.1793 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.85 15:34:39.02 +65:26:07.3
100.74013 44.00953 galactic Dra Second-epoch detections are separated by 5.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644413578864257280 | 15:34:38.94 +65:26:07.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.628+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:34:39.02 +65:26:07.3: 12.46 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:34:39.02 +65:26:07.3: 12.45 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644413578864257280,2461335.6793,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644413578864257280 20261022.1793 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.82 13:15:22.53 +72:25:33.6
120.39868 44.58432 galactic UMi Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687959053982894464 | 13:15:22.56 +72:25:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.389+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:22.53 +72:25:33.6: 12.45 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:22.53 +72:25:33.6: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687959053982894464,2461335.6793,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687959053982894464 20261022.1793 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.79 12:56:33.26 +73:10:21.6
122.41763 43.95048 galactic Dra Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691161244159810304 | 12:56:33.25 +73:10:20.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.274+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:33.26 +73:10:21.6: 12.47 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:33.26 +73:10:21.6: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691161244159810304,2461335.6793,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691161244159810304 20261022.1793 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.88 13:28:28.14 +71:51:10.9
118.86979 44.98201 galactic UMi Second-epoch detections are separated by 1.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687122463073152640 | 13:28:28.25 +71:51:10.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.435+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:28.14 +71:51:10.9: 12.45 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:28.14 +71:51:10.9: 12.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687122463073152640,2461335.6793,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687122463073152640 20261022.1793 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.75 13:17:18.56 +71:47:13.1
120.06805 45.19714 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1687834220757933056 | 13:17:18.56 +71:47:13.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.340+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:17:18.56 +71:47:13.1: 12.44 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:17:18.56 +71:47:13.1: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1687834220757933056,2461335.6793,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1687834220757933056 20261022.1793 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.73 12:52:58.53 +72:33:10.8
122.77013 44.57477 galactic Dra Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689661991336131456 | 12:52:58.58 +72:33:10.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.344+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:52:58.53 +72:33:10.8: 12.43 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:52:58.53 +72:33:10.8: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689661991336131456,2461335.6793,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689661991336131456 20261022.1793 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.60 12:56:38.70 +72:33:07.3
122.38405 44.57068 galactic Dra Second-epoch detections are separated by 0.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689617903496195584 | 12:56:38.64 +72:33:07.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.635+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:38.70 +72:33:07.3: 12.42 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:38.70 +72:33:07.3: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689617903496195584,2461335.6793,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689617903496195584 20261022.1793 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.16 13:17:43.98 +71:18:39.2
119.92307 45.66343 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687794470836081792 | 13:17:43.95 +71:18:40.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.603+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:17:43.98 +71:18:39.2: 12.43 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:17:43.98 +71:18:39.2: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687794470836081792,2461335.6793,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687794470836081792 20261022.1793 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.05 13:24:28.41 +72:43:10.4
119.52033 44.18920 galactic UMi Second-epoch detections are separated by 1.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687934933446538752 | 13:24:28.34 +72:43:10.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:24:28.41 +72:43:10.4: 12.43 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:24:28.41 +72:43:10.4: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687934933446538752,2461335.6793,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687934933446538752 20261022.1793 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.97 13:41:40.94 +71:00:43.9
117.13293 45.54612 galactic UMi Second-epoch detections are separated by 1.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686826213408817920 | 13:41:41.07 +71:00:43.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.330+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:41:40.94 +71:00:43.9: 12.42 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:41:40.94 +71:00:43.9: 12.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686826213408817920,2461335.6793,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686826213408817920 20261022.1793 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.11 13:31:53.93 +72:18:53.8
118.64387 44.47489 galactic UMi Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687531996794666240 | 13:31:54.05 +72:18:54.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.351+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:31:53.93 +72:18:53.8: 12.43 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:31:53.93 +72:18:53.8: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687531996794666240,2461335.6793,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687531996794666240 20261022.1793 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 12.05 12:59:18.60 +72:30:03.5
122.10075 44.61457 galactic Dra Second-epoch detections are separated by 2.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:59:18.60 +72:30:03.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:18.60 +72:30:03.5: 14.12 +/- 0.08 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:18.60 +72:30:03.5: 14.12 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.90 13:26:16.50 +71:23:52.9
118.98300 45.46217 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687010347246739840 | 13:26:16.65 +71:23:52.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.027 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:26:16.50 +71:23:52.9: 12.42 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:26:16.50 +71:23:52.9: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687010347246739840,2461335.6793,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687010347246739840 20261022.1793 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.74 13:19:01.41 +72:26:20.4
120.01873 44.53288 galactic UMi Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:19:01.41 +72:26:20.4 (user input) | T | P | (position from user input) J-Ks=0.291+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:01.41 +72:26:20.4: 12.39 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:01.41 +72:26:20.4: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.01 13:36:55.68 +71:52:42.9
117.97261 44.80905 galactic UMi Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687086003095584896 | 13:36:55.69 +71:52:42.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.303+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:36:55.68 +71:52:42.9: 12.39 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:36:55.68 +71:52:42.9: 12.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687086003095584896,2461335.6793,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687086003095584896 20261022.1793 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.80 13:02:01.61 +73:01:21.9
121.85617 44.08338 galactic Dra Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691146327737915520 | 13:02:01.59 +73:01:22.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.395+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:02:01.61 +73:01:21.9: 12.38 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:02:01.61 +73:01:21.9: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691146327737915520,2461335.6793,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691146327737915520 20261022.1793 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.82 13:02:29.57 +73:12:00.8
121.82361 43.90423 galactic Dra Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691243020337074048 | 13:02:29.69 +73:12:01.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.522+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:02:29.57 +73:12:00.8: 12.38 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:02:29.57 +73:12:00.8: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691243020337074048,2461335.6793,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691243020337074048 20261022.1793 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.88 13:29:17.60 +71:21:49.5
118.63673 45.44748 galactic UMi Second-epoch detections are separated by 0.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687001787376075264 | 13:29:17.60 +71:21:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.431+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:29:17.60 +71:21:49.5: 12.39 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:29:17.60 +71:21:49.5: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687001787376075264,2461335.6793,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687001787376075264 20261022.1793 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.80 13:23:07.70 +71:31:41.0
119.36724 45.38022 galactic UMi Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687766875670740992 | 13:23:07.75 +71:31:40.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.291+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:07.70 +71:31:41.0: 12.39 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:07.70 +71:31:41.0: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687766875670740992,2461335.6793,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687766875670740992 20261022.1793 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.06 13:34:09.85 +70:52:16.0
117.93027 45.83996 galactic UMi Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686928261831717760 | 13:34:09.68 +70:52:15.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.551+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:34:09.85 +70:52:16.0: 12.38 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:34:09.85 +70:52:16.0: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686928261831717760,2461335.6793,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686928261831717760 20261022.1793 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.90 13:05:00.73 +72:02:27.4
121.45159 45.04827 galactic UMi Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686575589181362176 | 13:05:00.84 +72:02:27.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.440+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:05:00.73 +72:02:27.4: 12.37 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:05:00.73 +72:02:27.4: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686575589181362176,2461335.6793,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686575589181362176 20261022.1793 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.61 13:03:11.12 +72:22:32.4
121.68085 44.72404 galactic Dra Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688096424216852608 | 13:03:11.01 +72:22:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.417+/-0.026 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:03:11.12 +72:22:32.4: 12.37 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:03:11.12 +72:22:32.4: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688096424216852608,2461335.6793,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688096424216852608 20261022.1793 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.79 13:31:21.37 +71:29:17.8
118.44623 45.29070 galactic UMi Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687094386870991104 | 13:31:21.50 +71:29:17.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.312+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:31:21.37 +71:29:17.8: 12.40 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:31:21.37 +71:29:17.8: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687094386870991104,2461335.6793,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687094386870991104 20261022.1793 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.20 13:27:38.60 +72:38:45.3
119.17788 44.21747 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was found in VSX 0" Gaia DR3 1688293438660815744
Type: ROT
# Max. Min./Amp. JD0 Period
12.090 G 12.130 G G
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:38.60 +72:38:45.3: 12.37 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:38.60 +72:38:45.3: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688293438660815744,2461335.6793,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688293438660815744 20261022.1793 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.95 13:04:13.52 +73:26:41.2
121.67351 43.65222 galactic UMi Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688251485420613760 | 13:04:13.78 +73:26:40.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.473+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:04:13.52 +73:26:41.2: 12.34 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:04:13.52 +73:26:41.2: 12.38 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688251485420613760,2461335.6793,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688251485420613760 20261022.1793 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.65 12:45:58.85 +73:10:10.9
123.48056 43.95274 galactic Dra Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689883027533023232 | 12:45:58.86 +73:10:11.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.352+/-0.025 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:45:58.85 +73:10:10.9: 12.36 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:45:58.85 +73:10:10.9: 12.37 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689883027533023232,2461335.6793,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689883027533023232 20261022.1793 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.65 13:18:09.50 +71:49:40.9
119.98345 45.14694 galactic UMi Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687834637370293888 | 13:18:09.46 +71:49:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.315+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:09.50 +71:49:40.9: 12.35 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:09.50 +71:49:40.9: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687834637370293888,2461335.6793,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687834637370293888 20261022.1793 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.76 13:03:45.65 +73:15:30.2
121.70206 43.84042 galactic Dra Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688242586248383488 | 13:03:45.52 +73:15:30.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.613+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:03:45.65 +73:15:30.2: 12.33 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:03:45.65 +73:15:30.2: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688242586248383488,2461335.6793,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688242586248383488 20261022.1793 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.04 13:19:41.36 +71:09:37.0
119.66764 45.78849 galactic UMi Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687742690710355840 | 13:19:41.27 +71:09:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.905+/-0.027 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:41.36 +71:09:37.0: 12.34 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:41.36 +71:09:37.0: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687742690710355840,2461335.6793,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687742690710355840 20261022.1793 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.93 13:24:14.75 +72:35:07.8
119.51035 44.32414 galactic UMi Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687932322106416000 | 13:24:14.73 +72:35:07.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.352+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:24:14.75 +72:35:07.8: 12.34 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:24:14.75 +72:35:07.8: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687932322106416000,2461335.6793,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687932322106416000 20261022.1793 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.85 13:18:21.78 +72:43:44.6
120.14712 44.25332 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687992825310417408 | 13:18:21.67 +72:43:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.716+/-0.032 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:21.78 +72:43:44.6: 12.33 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:21.78 +72:43:44.6: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687992825310417408,2461335.6793,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687992825310417408 20261022.1793 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.68 13:07:22.13 +72:19:13.5
121.22977 44.75515 galactic UMi Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688040001230770432 | 13:07:22.14 +72:19:13.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.340+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:22.13 +72:19:13.5: 12.32 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:22.13 +72:19:13.5: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688040001230770432,2461335.6793,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688040001230770432 20261022.1793 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.64 13:05:51.80 +72:56:33.8
121.45857 44.14424 galactic UMi Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688222382722233600 | 13:05:51.81 +72:56:34.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.640+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:05:51.80 +72:56:33.8: 12.31 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:05:51.80 +72:56:33.8: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688222382722233600,2461335.6793,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688222382722233600 20261022.1793 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.69 12:51:30.25 +73:37:03.7
122.92548 43.51056 galactic Dra Second-epoch detections are separated by 1.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691234670920764032 | 12:51:30.06 +73:37:04.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.497+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:51:30.25 +73:37:03.7: 12.34 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:51:30.25 +73:37:03.7: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691234670920764032,2461335.6793,10.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691234670920764032 20261022.1793 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.95 13:13:05.96 +71:33:21.9
120.49176 45.46940 galactic UMi Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686315146660585216 | 13:13:05.90 +71:33:22.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.623+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:13:05.96 +71:33:21.9: 12.31 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:13:05.96 +71:33:21.9: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686315146660585216,2461335.6793,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686315146660585216 20261022.1793 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.74 13:18:46.50 +71:40:22.8
119.88296 45.29307 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was found in VSX 3" NSVS 898869
Type: EB
# Max. Min./Amp. JD0 Period
12.791 r Y 0.326 r 2458645.78070 0.553961600000
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:46.50 +71:40:22.8: 12.30 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:46.50 +71:40:22.8: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 898869,2461335.6793,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 898869 20261022.1793 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.82 13:31:08.93 +71:54:52.0
118.60024 44.87831 galactic UMi Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687144105412400384 | 13:31:08.87 +71:54:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.321+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:31:08.93 +71:54:52.0: 12.30 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:31:08.93 +71:54:52.0: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687144105412400384,2461335.6793,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687144105412400384 20261022.1793 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.63 13:11:44.00 +72:27:30.6
120.78704 44.58513 galactic UMi Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688055948444978176 | 13:11:44.04 +72:27:30.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:11:44.00 +72:27:30.6: 12.30 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:11:44.00 +72:27:30.6: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688055948444978176,2461335.6793,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688055948444978176 20261022.1793 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.13 15:24:45.65 +66:30:17.5
102.77545 44.14771 galactic UMi Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644750549113737472 | 15:24:45.76 +66:30:16.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.789+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:24:45.65 +66:30:17.5: 12.31 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:24:45.65 +66:30:17.5: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644750549113737472,2461335.6793,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644750549113737472 20261022.1793 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.88 13:15:10.86 +72:52:25.2
120.49974 44.14229 galactic UMi Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688185892679716864 | 13:15:10.82 +72:52:25.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.475+/-0.038 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:10.86 +72:52:25.2: 12.29 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:10.86 +72:52:25.2: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688185892679716864,2461335.6793,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688185892679716864 20261022.1793 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.14 13:29:49.76 +70:39:17.3
118.36072 46.13119 galactic UMi Second-epoch detections are separated by 1.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686904759770663040 | 13:29:49.89 +70:39:16.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.288+/-0.027 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:29:49.76 +70:39:17.3: 12.30 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:29:49.76 +70:39:17.3: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686904759770663040,2461335.6793,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686904759770663040 20261022.1793 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.58 12:59:44.93 +72:30:12.4
122.05461 44.61065 galactic Dra Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691102656510453248 | 12:59:44.88 +72:30:12.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.280+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:44.93 +72:30:12.4: 12.28 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:44.93 +72:30:12.4: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691102656510453248,2461335.6793,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691102656510453248 20261022.1793 10.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.56 12:46:58.60 +72:47:21.7
123.39327 44.33489 galactic Dra Second-epoch detections are separated by 0.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689682882057124352 | 12:46:58.60 +72:47:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.343+/-0.025 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:46:58.60 +72:47:21.7: 12.29 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:46:58.60 +72:47:21.7: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689682882057124352,2461335.6793,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689682882057124352 20261022.1793 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.21 12:55:49.65 +73:55:36.1
122.51516 43.19800 galactic Dra Second-epoch detections are separated by 1.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691325823011106688 | 12:55:49.22 +73:55:36.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.498+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:55:49.65 +73:55:36.1: 12.31 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:55:49.65 +73:55:36.1: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691325823011106688,2461335.6793,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691325823011106688 20261022.1793 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.65 13:23:10.50 +72:08:04.6
119.51152 44.78227 galactic UMi Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687895625905808512 | 13:23:10.42 +72:08:04.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.333+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:10.50 +72:08:04.6: 12.26 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:10.50 +72:08:04.6: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687895625905808512,2461335.6793,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687895625905808512 20261022.1793 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.68 13:06:57.13 +73:02:16.2
121.35877 44.04300 galactic UMi Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688224409946794752 | 13:06:57.22 +73:02:16.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.371+/-0.025 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:57.13 +73:02:16.2: 12.25 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:57.13 +73:02:16.2: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688224409946794752,2461335.6793,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688224409946794752 20261022.1793 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.06 13:19:13.86 +71:13:27.3
119.73421 45.73105 galactic UMi Second-epoch detections are separated by 1.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687743167451264896 | 13:19:13.95 +71:13:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.176+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:13.86 +71:13:27.3: 12.25 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:13.86 +71:13:27.3: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687743167451264896,2461335.6793,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687743167451264896 20261022.1793 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.61 13:07:52.38 +72:45:41.7
121.23144 44.31236 galactic UMi Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688123259172497280 | 13:07:52.41 +72:45:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.346+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:52.38 +72:45:41.7: 12.25 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:52.38 +72:45:41.7: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688123259172497280,2461335.6793,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688123259172497280 20261022.1793 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.57 12:57:19.87 +72:31:46.3
122.31087 44.59162 galactic Dra Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689605984963034496 | 12:57:20.01 +72:31:46.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.320+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:57:19.87 +72:31:46.3: 12.24 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:57:19.87 +72:31:46.3: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689605984963034496,2461335.6793,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689605984963034496 20261022.1793 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.59 13:06:36.56 +72:49:26.6
121.36899 44.25813 galactic UMi Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688126798225551232 | 13:06:36.50 +72:49:26.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.936+/-0.029 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:36.56 +72:49:26.6: 12.24 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:36.56 +72:49:26.6: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688126798225551232,2461335.6793,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688126798225551232 20261022.1793 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.26 13:21:49.45 +70:49:22.6
119.34181 46.09291 galactic UMi Second-epoch detections are separated by 1.1" and 7.2 pix
The object was found in VSX 1" Gaia DR3 1686221477718359168
Type: ROT
# Max. Min./Amp. JD0 Period
12.050 G 12.080 G K
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:49.45 +70:49:22.6: 12.26 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:49.45 +70:49:22.6: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686221477718359168,2461335.6793,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686221477718359168 20261022.1793 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.85 13:38:05.54 +71:09:31.5
117.58883 45.48240 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687029657419753600 | 13:38:05.51 +71:09:31.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.105+/-0.030 (A)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:38:05.54 +71:09:31.5: 12.25 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:38:05.54 +71:09:31.5: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687029657419753600,2461335.6793,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687029657419753600 20261022.1793 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.76 13:24:56.71 +72:31:35.0
119.42341 44.37289 galactic UMi Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687930844637615872 | 13:24:56.71 +72:31:35.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.566+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:24:56.71 +72:31:35.0: 12.24 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:24:56.71 +72:31:35.0: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687930844637615872,2461335.6793,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687930844637615872 20261022.1793 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.04 13:26:41.44 +70:49:07.7
118.77448 46.02382 galactic UMi Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686957811206744960 | 13:26:41.40 +70:49:07.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.843+/-0.027 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:26:41.44 +70:49:07.7: 12.25 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:26:41.44 +70:49:07.7: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686957811206744960,2461335.6793,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686957811206744960 20261022.1793 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.76 13:18:29.52 +72:49:05.2
120.15206 44.16382 galactic UMi Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687995058693410944 | 13:18:29.45 +72:49:04.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.630+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:29.52 +72:49:05.2: 12.23 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:29.52 +72:49:05.2: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687995058693410944,2461335.6793,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687995058693410944 20261022.1793 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.20 13:19:44.63 +70:53:44.4
119.60146 46.04911 galactic UMi Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686219798386548480 | 13:19:44.63 +70:53:44.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.327+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:44.63 +70:53:44.4: 12.23 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:44.63 +70:53:44.4: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686219798386548480,2461335.6793,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686219798386548480 20261022.1793 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.66 13:18:14.35 +72:23:50.7
120.09231 44.58277 galactic UMi Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687955819871601280 | 13:18:14.22 +72:23:50.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.341+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:14.35 +72:23:50.7: 12.22 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:14.35 +72:23:50.7: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687955819871601280,2461335.6793,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687955819871601280 20261022.1793 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.61 13:17:12.36 +71:49:01.2
120.08543 45.16856 galactic UMi Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687835152766333568 | 13:17:12.42 +71:49:02.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.841+/-0.028 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:17:12.36 +71:49:01.2: 12.23 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:17:12.36 +71:49:01.2: 12.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687835152766333568,2461335.6793,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687835152766333568 20261022.1793 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.16 14:39:51.55 +74:45:02.0
113.87600 40.41395 galactic UMi Second-epoch detections are separated by 0.2" and 6.7 pix
The object was found in VSX 0" XZ UMi
Type: RRAB/BL
# Max. Min./Amp. JD0 Period
11.960 R1 12.470 R1 2451612.62000 0.585210000000
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 14:39:51.55 +74:45:02.0: 12.21 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 14:39:51.55 +74:45:02.0: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
XZ UMi,2461335.6793,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
XZ UMi 20261022.1793 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.03 15:34:42.38 +66:40:58.8
102.12105 43.26263 galactic UMi Second-epoch detections are separated by 3.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:34:42.38 +66:40:58.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:34:42.38 +66:40:58.8: 12.20 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:34:42.38 +66:40:58.8: 12.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.60 13:10:18.32 +72:33:22.9
120.95137 44.49926 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688069103929177856 | 13:10:18.39 +72:33:23.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.374+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:10:18.32 +72:33:22.9: 12.19 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:10:18.32 +72:33:22.9: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688069103929177856,2461335.6793,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688069103929177856 20261022.1793 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.60 13:18:04.43 +72:06:32.9
120.05073 44.86981 galactic UMi Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687846216602103680 | 13:18:04.50 +72:06:33.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.335+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:04.43 +72:06:32.9: 12.18 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:04.43 +72:06:32.9: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687846216602103680,2461335.6793,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687846216602103680 20261022.1793 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.60 12:48:33.08 +73:34:19.1
123.21352 43.55470 galactic Dra Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691231303666970624 | 12:48:32.98 +73:34:18.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.374+/-0.027 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:48:33.08 +73:34:19.1: 12.24 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:48:33.08 +73:34:19.1: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691231303666970624,2461335.6793,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691231303666970624 20261022.1793 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.97 13:25:08.75 +70:54:00.5
118.97585 45.96832 galactic UMi Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686971108425532928 | 13:25:08.65 +70:54:00.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.390+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:08.75 +70:54:00.5: 12.19 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:08.75 +70:54:00.5: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686971108425532928,2461335.6793,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686971108425532928 20261022.1793 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.88 15:26:36.25 +66:47:00.3
102.91229 43.82948 galactic UMi Second-epoch detections are separated by 1.0" and 6.5 pix
The object was found in VSX 1" NSVS 2790137
Type: EA
# Max. Min./Amp. JD0 Period
12.110 R1 Y 0.400 R1 2458288.69940 0.828471400000
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:26:36.25 +66:47:00.3: 12.19 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:26:36.25 +66:47:00.3: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2790137,2461335.6793,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 2790137 20261022.1793 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.10 13:27:45.33 +72:42:13.4
119.18223 44.15915 galactic UMi Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688306873318516992 | 13:27:45.27 +72:42:12.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.642+/-0.032 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:45.33 +72:42:13.4: 12.19 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:45.33 +72:42:13.4: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688306873318516992,2461335.6793,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688306873318516992 20261022.1793 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.47 12:41:03.28 +73:03:01.2
123.98465 44.05669 galactic Dra Second-epoch detections are separated by 0.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689889315365189120 | 12:41:12.08 +73:02:35.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.261+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:41:03.28 +73:03:01.2: 12.25 +/- 0.02 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:41:03.28 +73:03:01.2: 12.23 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689889315365189120,2461335.6793,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689889315365189120 20261022.1793 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.68 13:14:10.04 +72:55:43.6
120.61234 44.09696 galactic UMi Second-epoch detections are separated by 1.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688186957831604864 | 13:14:10.17 +72:55:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.433+/-0.035 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:10.04 +72:55:43.6: 12.17 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:10.04 +72:55:43.6: 12.20 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688186957831604864,2461335.6793,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688186957831604864 20261022.1793 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.05 13:41:15.65 +71:45:19.4
117.46732 44.84047 galactic UMi Second-epoch detections are separated by 1.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687444684404126336 | 13:41:15.66 +71:45:19.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.300+/-0.027 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:41:15.65 +71:45:19.4: 12.17 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:41:15.65 +71:45:19.4: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687444684404126336,2461335.6793,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687444684404126336 20261022.1793 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.66 13:00:41.70 +73:25:05.1
122.01868 43.69375 galactic Dra Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691250682558741888 | 13:00:41.78 +73:25:05.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.655+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:00:41.70 +73:25:05.1: 12.16 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:00:41.70 +73:25:05.1: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691250682558741888,2461335.6793,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691250682558741888 20261022.1793 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.81 13:37:37.74 +71:39:49.9
117.82197 45.00329 galactic UMi Second-epoch detections are separated by 0.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687070163256198912 | 13:37:38.16 +71:39:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:37:37.74 +71:39:49.9: 12.16 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:37:37.74 +71:39:49.9: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687070163256198912,2461335.6793,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687070163256198912 20261022.1793 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.46 12:50:06.99 +72:56:48.7
123.06701 44.18104 galactic Dra Second-epoch detections are separated by 1.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689688413974961664 | 12:50:07.14 +72:56:48.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.319+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:50:06.99 +72:56:48.7: 12.13 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:50:06.99 +72:56:48.7: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689688413974961664,2461335.6793,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689688413974961664 20261022.1793 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.54 13:01:30.73 +73:04:14.0
121.91201 44.03774 galactic Dra Second-epoch detections are separated by 0.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691146709990440832 | 13:01:30.71 +73:04:13.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.635+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:30.73 +73:04:14.0: 12.12 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:30.73 +73:04:14.0: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691146709990440832,2461335.6793,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691146709990440832 20261022.1793 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.62 13:29:43.86 +71:43:13.0
118.69453 45.09159 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687117476615169024 | 13:29:43.89 +71:43:13.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.287+/-0.027 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:29:43.86 +71:43:13.0: 12.12 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:29:43.86 +71:43:13.0: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687117476615169024,2461335.6793,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687117476615169024 20261022.1793 10.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.70 13:39:12.41 +71:14:33.8
117.49630 45.37801 galactic UMi Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686844046113044736 | 13:39:12.43 +71:14:34.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.373+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:39:12.41 +71:14:33.8: 12.12 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:39:12.41 +71:14:33.8: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686844046113044736,2461335.6793,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686844046113044736 20261022.1793 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.51 13:10:26.21 +72:53:39.7
120.98631 44.16205 galactic UMi Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688172187440091136 | 13:10:26.22 +72:53:40.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.643+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:10:26.21 +72:53:39.7: 12.08 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:10:26.21 +72:53:39.7: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688172187440091136,2461335.6793,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688172187440091136 20261022.1793 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.56 13:28:10.62 +71:35:05.1
118.82474 45.24938 galactic UMi Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687109784329684736 | 13:28:10.68 +71:35:05.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.344+/-0.027 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:10.62 +71:35:05.1: 12.10 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:10.62 +71:35:05.1: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687109784329684736,2461335.6793,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687109784329684736 20261022.1793 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.84 13:32:57.25 +72:14:56.1
118.51356 44.52145 galactic UMi Second-epoch detections are separated by 1.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1687530622404707968 | 13:32:57.14 +72:14:55.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.175+/-0.034 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:57.25 +72:14:56.1: 12.09 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:57.25 +72:14:56.1: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1687530622404707968,2461335.6793,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1687530622404707968 20261022.1793 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.49 12:57:51.79 +72:37:22.5
122.25942 44.49694 galactic Dra Second-epoch detections are separated by 1.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691107883486101504 | 12:57:51.95 +72:37:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:57:51.79 +72:37:22.5: 12.08 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:57:51.79 +72:37:22.5: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691107883486101504,2461335.6793,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691107883486101504 20261022.1793 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.55 13:02:14.65 +73:06:46.4
121.84144 43.99247 galactic Dra Second-epoch detections are separated by 1.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691148496696838272 | 13:02:14.71 +73:06:46.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.321+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:02:14.65 +73:06:46.4: 12.08 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:02:14.65 +73:06:46.4: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691148496696838272,2461335.6793,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691148496696838272 20261022.1793 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.11 13:33:28.39 +72:24:10.2
118.50853 44.36261 galactic UMi Second-epoch detections are separated by 1.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687533439903681792 | 13:33:28.50 +72:24:10.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=10.774+/- (unrealisitic color!)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:33:28.39 +72:24:10.2: 12.09 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:33:28.39 +72:24:10.2: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687533439903681792,2461335.6793,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687533439903681792 20261022.1793 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.57 13:30:42.83 +71:36:15.4
118.55249 45.18851 galactic UMi Second-epoch detections are separated by 0.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687104183692292480 | 13:30:42.72 +71:36:15.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.708+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:30:42.83 +71:36:15.4: 12.09 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:30:42.83 +71:36:15.4: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687104183692292480,2461335.6793,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687104183692292480 20261022.1793 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.40 12:41:12.12 +73:02:35.7
123.97027 44.06436 galactic Dra Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689889315365189120 | 12:41:12.08 +73:02:35.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.693+/-0.025 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:41:12.12 +73:02:35.7: 12.11 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:41:12.12 +73:02:35.7: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689889315365189120,2461335.6793,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689889315365189120 20261022.1793 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.54 13:01:57.32 +72:14:01.6
121.80015 44.87135 galactic Dra Second-epoch detections are separated by 0.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J195.4973+72.2339 | 13:01:57.20 +72:14:02.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.454+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:57.32 +72:14:01.6: 12.07 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:57.32 +72:14:01.6: 12.03 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J195.4973+72.2339,2461335.6793,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J195.4973+72.2339 20261022.1793 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.50 12:42:14.93 +73:26:26.7
123.83691 43.67135 galactic Dra Second-epoch detections are separated by 0.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691402655681527424 | 12:42:14.92 +73:26:26.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.303+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:42:14.93 +73:26:26.7: 12.13 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:42:14.93 +73:26:26.7: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691402655681527424,2461335.6793,10.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691402655681527424 20261022.1793 10.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.05 12:58:57.08 +73:46:23.7
122.21028 43.34447 galactic Dra Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691276108765160960 | 12:58:56.97 +73:46:24.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.359+/-0.024 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:57.08 +73:46:23.7: 12.06 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:57.08 +73:46:23.7: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691276108765160960,2461335.6793,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691276108765160960 20261022.1793 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.64 13:18:09.40 +72:43:37.2
120.16786 44.25757 galactic UMi Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687992795245983616 | 13:18:09.24 +72:43:37.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.471+/-0.032 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:09.40 +72:43:37.2: 12.05 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:09.40 +72:43:37.2: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687992795245983616,2461335.6793,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687992795245983616 20261022.1793 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.98 13:25:21.16 +72:46:50.2
119.44634 44.11739 galactic UMi Second-epoch detections are separated by 2.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688309935630988032 | 13:25:21.24 +72:46:50.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.549+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:21.16 +72:46:50.2: 12.06 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:21.16 +72:46:50.2: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688309935630988032,2461335.6793,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688309935630988032 20261022.1793 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.94 13:20:48.31 +70:58:12.0
119.49551 45.96180 galactic UMi Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686226807773147008 | 13:20:48.36 +70:58:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.281+/-0.027 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:20:48.31 +70:58:12.0: 12.04 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:20:48.31 +70:58:12.0: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686226807773147008,2461335.6793,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686226807773147008 20261022.1793 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.46 13:19:41.80 +72:00:39.5
119.85548 44.94810 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687841745540401664 | 13:19:41.88 +72:00:39.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.269+/-0.036 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:41.80 +72:00:39.5: 12.05 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:41.80 +72:00:39.5: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687841745540401664,2461335.6793,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687841745540401664 20261022.1793 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.98 15:26:38.72 +66:13:52.6
102.31362 44.17507 galactic UMi Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644684367962375168 | 15:26:38.71 +66:13:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.297+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:26:38.72 +66:13:52.6: 12.04 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:26:38.72 +66:13:52.6: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644684367962375168,2461335.6793,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644684367962375168 20261022.1793 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.40 13:12:08.64 +72:08:20.0
120.69300 44.89924 galactic UMi Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688042204549612160 | 13:12:08.71 +72:08:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.355+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:12:08.64 +72:08:20.0: 12.04 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:12:08.64 +72:08:20.0: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688042204549612160,2461335.6793,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688042204549612160 20261022.1793 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.40 12:53:33.98 +72:58:24.2
122.71476 44.15396 galactic Dra Second-epoch detections are separated by 0.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691175224277483648 | 12:53:33.91 +72:58:24.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.299+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:53:33.98 +72:58:24.2: 12.02 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:53:33.98 +72:58:24.2: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691175224277483648,2461335.6793,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691175224277483648 20261022.1793 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.80 13:32:14.74 +72:16:35.6
118.59597 44.50653 galactic UMi Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687530931642774528 | 13:32:14.73 +72:16:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.749+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:14.74 +72:16:35.6: 12.05 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:14.74 +72:16:35.6: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687530931642774528,2461335.6793,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687530931642774528 20261022.1793 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.39 12:46:55.10 +73:04:47.9
123.38938 44.04426 galactic Dra Second-epoch detections are separated by 1.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689694083330986624 | 12:46:55.17 +73:04:47.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.268+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:46:55.10 +73:04:47.9: 12.05 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:46:55.10 +73:04:47.9: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689694083330986624,2461335.6793,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689694083330986624 20261022.1793 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.80 15:33:52.91 +66:43:08.2
102.22800 43.30596 galactic UMi Second-epoch detections are separated by 1.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644806929148758656 | 15:33:53.06 +66:43:07.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.023 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:33:52.91 +66:43:08.2: 12.02 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:33:52.91 +66:43:08.2: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644806929148758656,2461335.6793,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644806929148758656 20261022.1793 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.90 13:28:32.66 +70:44:48.1
118.53829 46.06371 galactic UMi Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686953138282322432 | 13:28:32.65 +70:44:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.133+/-0.029 (A)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:32.66 +70:44:48.1: 12.03 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:32.66 +70:44:48.1: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686953138282322432,2461335.6793,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686953138282322432 20261022.1793 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.46 12:55:19.61 +73:11:10.9
122.54139 43.93894 galactic Dra Second-epoch detections are separated by 1.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691160896266578560 | 12:55:19.55 +73:11:11.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.346+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:55:19.61 +73:11:10.9: 12.02 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:55:19.61 +73:11:10.9: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691160896266578560,2461335.6793,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691160896266578560 20261022.1793 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.38 12:53:41.96 +72:51:35.4
122.69925 44.26740 galactic Dra Second-epoch detections are separated by 0.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691172750376323840 | 12:53:41.98 +72:51:35.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.252+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:53:41.96 +72:51:35.4: 12.02 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:53:41.96 +72:51:35.4: 12.00 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691172750376323840,2461335.6793,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691172750376323840 20261022.1793 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.52 13:04:49.66 +73:10:44.9
121.58788 43.91415 galactic UMi Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1688238329935677824 | 13:04:49.77 +73:10:45.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.378+/-0.027 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:04:49.66 +73:10:44.9: 11.99 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:04:49.66 +73:10:44.9: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1688238329935677824,2461335.6793,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1688238329935677824 20261022.1793 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.68 13:18:36.11 +72:54:37.6
120.15973 44.07130 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688001449604746368 | 13:18:36.00 +72:54:37.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.292+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:36.11 +72:54:37.6: 11.98 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:36.11 +72:54:37.6: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688001449604746368,2461335.6793,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688001449604746368 20261022.1793 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.84 15:26:54.39 +66:13:17.5
102.27999 44.16071 galactic UMi Second-epoch detections are separated by 0.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644690179053375232 | 15:26:54.42 +66:13:18.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.333+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:26:54.39 +66:13:17.5: 11.99 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:26:54.39 +66:13:17.5: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644690179053375232,2461335.6793,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644690179053375232 20261022.1793 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.60 15:29:40.01 +66:22:09.7
102.20048 43.85160 galactic UMi Second-epoch detections are separated by 1.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644712100566466944 | 15:29:40.18 +66:22:09.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.295+/-0.036 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:29:40.01 +66:22:09.7: 11.96 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:29:40.01 +66:22:09.7: 11.97 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644712100566466944,2461335.6793,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644712100566466944 20261022.1793 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.72 13:21:42.11 +71:49:32.8
119.59617 45.10595 galactic UMi Second-epoch detections are separated by 0.5" and 7.3 pix
The object was found in VSX 1" Gaia DR3 1687790656905111936
Type: ROT
# Max. Min./Amp. JD0 Period
13.560 G 13.590 G K
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:42.11 +71:49:32.8: 13.92 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:42.11 +71:49:32.8: 13.92 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687790656905111936,2461335.6793,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687790656905111936 20261022.1793 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.47 13:19:02.60 +72:12:15.6
119.96707 44.76466 galactic UMi Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687940362285212288 | 13:19:02.44 +72:12:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.326+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:02.60 +72:12:15.6: 11.95 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:02.60 +72:12:15.6: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687940362285212288,2461335.6793,10.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687940362285212288 20261022.1793 10.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.76 12:57:40.47 +73:42:17.3
122.32972 43.41615 galactic Dra Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691274867518904576 | 12:57:40.55 +73:42:17.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.707+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:57:40.47 +73:42:17.3: 11.94 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:57:40.47 +73:42:17.3: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691274867518904576,2461335.6793,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691274867518904576 20261022.1793 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.70 15:32:04.15 +66:44:42.6
102.40657 43.43199 galactic UMi Second-epoch detections are separated by 0.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644821055296868864 | 15:32:04.07 +66:44:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.422+/-0.035 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:32:04.15 +66:44:42.6: 11.94 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:32:04.15 +66:44:42.6: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644821055296868864,2461335.6793,10.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644821055296868864 20261022.1793 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.91 13:12:59.50 +71:49:15.5
120.54863 45.20741 galactic UMi Second-epoch detections are separated by 3.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:12:59.50 +71:49:15.5 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.036 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:12:59.50 +71:49:15.5: 13.93 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:12:59.50 +71:49:15.5: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.97 13:57:59.75 +65:11:33.9
112.04331 50.50507 galactic Dra Second-epoch detections are separated by 2.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1671079248394339840 | 13:57:59.83 +65:11:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.374+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:57:59.75 +65:11:33.9: 11.91 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:57:59.75 +65:11:33.9: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1671079248394339840,2461335.6793,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1671079248394339840 20261022.1793 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.87 15:33:00.32 +66:46:59.1
102.37024 43.33573 galactic UMi Second-epoch detections are separated by 0.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644818512676234752 | 15:33:00.48 +66:46:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.722+/-0.023 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:33:00.32 +66:46:59.1: 11.90 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:33:00.32 +66:46:59.1: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.91 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644818512676234752,2461335.6793,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644818512676234752 20261022.1793 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.45 13:22:13.66 +71:33:59.2
119.47658 45.35467 galactic UMi Second-epoch detections are separated by 1.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687778940234315136 | 13:22:13.79 +71:34:00.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/-0.026 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:22:13.66 +71:33:59.2: 11.89 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:22:13.66 +71:33:59.2: 11.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687778940234315136,2461335.6793,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687778940234315136 20261022.1793 10.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.59 12:47:27.60 +72:58:59.4
123.33746 44.14195 galactic Dra Second-epoch detections are separated by 1.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:47:27.60 +72:58:59.4 (user input) | T | P | (position from user input) J-Ks=0.806+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:47:27.60 +72:58:59.4: 13.90 +/- 0.07 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:47:27.60 +72:58:59.4: 13.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.46 13:28:28.78 +72:14:26.9
118.97892 44.60204 galactic UMi Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687903150688476032 | 13:28:28.85 +72:14:27.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.640+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:28.78 +72:14:26.9: 11.86 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:28.78 +72:14:26.9: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687903150688476032,2461335.6793,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687903150688476032 20261022.1793 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.22 12:42:15.51 +73:10:27.4
123.85419 43.93753 galactic Dra Second-epoch detections are separated by 0.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689896943227115520 | 12:42:15.43 +73:10:27.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.707+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:42:15.51 +73:10:27.4: 11.86 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:42:15.51 +73:10:27.4: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689896943227115520,2461335.6793,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689896943227115520 20261022.1793 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.69 13:16:48.08 +71:47:22.9
120.12436 45.20004 galactic UMi Second-epoch detections are separated by 1.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:16:48.08 +71:47:22.9 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:16:48.08 +71:47:22.9: 13.90 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:16:48.08 +71:47:22.9: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.43 15:38:50.47 +66:21:18.4
101.42425 43.12451 galactic UMi Second-epoch detections are separated by 0.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644551949826360448 | 15:38:50.41 +66:21:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.297+/-0.027 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:38:50.47 +66:21:18.4: 11.85 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:38:50.47 +66:21:18.4: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644551949826360448,2461335.6793,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644551949826360448 20261022.1793 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.80 13:14:51.04 +71:13:37.0
120.23475 45.77850 galactic UMi Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686289067619149440 | 13:14:51.04 +71:13:36.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.335+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:51.04 +71:13:37.0: 11.84 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:51.04 +71:13:37.0: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686289067619149440,2461335.6793,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686289067619149440 20261022.1793 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.25 13:07:36.05 +72:24:14.1
121.21543 44.67043 galactic UMi Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688064091703007360 | 13:07:36.01 +72:24:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.320+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:36.05 +72:24:14.1: 11.83 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:36.05 +72:24:14.1: 11.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688064091703007360,2461335.6793,10.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688064091703007360 20261022.1793 10.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.22 12:42:23.11 +72:56:59.5
123.85674 44.16213 galactic Dra Second-epoch detections are separated by 1.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689864335835388160 | 12:42:23.06 +72:56:59.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.369+/-0.026 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:42:23.11 +72:56:59.5: 11.87 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:42:23.11 +72:56:59.5: 11.84 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689864335835388160,2461335.6793,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689864335835388160 20261022.1793 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.41 13:31:47.08 +71:30:01.6
118.40291 45.27134 galactic UMi Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687094631685019008 | 13:31:47.03 +71:30:01.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.594+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:31:47.08 +71:30:01.6: 11.84 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:31:47.08 +71:30:01.6: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687094631685019008,2461335.6793,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687094631685019008 20261022.1793 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.38 13:16:37.02 +72:38:14.7
120.30880 44.36237 galactic UMi Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687967742701409920 | 13:16:37.12 +72:38:14.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.590+/-0.035 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:16:37.02 +72:38:14.7: 11.83 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:16:37.02 +72:38:14.7: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687967742701409920,2461335.6793,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687967742701409920 20261022.1793 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.27 13:12:11.60 +71:58:43.3
120.66192 45.05796 galactic UMi Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688016056788708224 | 13:12:11.58 +71:58:43.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.431+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:12:11.60 +71:58:43.3: 11.82 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:12:11.60 +71:58:43.3: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688016056788708224,2461335.6793,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688016056788708224 20261022.1793 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.85 13:28:19.91 +71:48:42.0
118.87278 45.02468 galactic UMi Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:28:19.91 +71:48:42.0 (user input) | T | P | (position from user input) J-Ks=0.504+/-0.032 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:19.91 +71:48:42.0: 13.87 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:19.91 +71:48:42.0: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.38 13:19:14.09 +72:21:29.2
119.97946 44.61045 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687949433256146816 | 13:19:13.99 +72:21:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.658+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:14.09 +72:21:29.2: 11.81 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:14.09 +72:21:29.2: 11.83 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687949433256146816,2461335.6793,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687949433256146816 20261022.1793 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.21 12:55:48.29 +72:45:00.8
122.47903 44.37419 galactic Dra Second-epoch detections are separated by 1.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691122825676477568 | 12:55:48.32 +72:45:00.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.251+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:55:48.29 +72:45:00.8: 11.82 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:55:48.29 +72:45:00.8: 11.80 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691122825676477568,2461335.6793,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691122825676477568 20261022.1793 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.27 12:56:35.85 +73:05:53.9
122.41041 44.02472 galactic Dra Second-epoch detections are separated by 0.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691159423093673856 | 12:56:35.95 +73:05:54.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.340+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:35.85 +73:05:53.9: 11.81 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:35.85 +73:05:53.9: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691159423093673856,2461335.6793,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691159423093673856 20261022.1793 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.88 13:59:20.65 +65:04:45.3
111.76716 50.55147 galactic Dra Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1671075434463350400 | 13:59:20.61 +65:04:44.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.406+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:59:20.65 +65:04:45.3: 11.80 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:59:20.65 +65:04:45.3: 11.81 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1671075434463350400,2461335.6793,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1671075434463350400 20261022.1793 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.40 13:23:03.11 +72:12:04.0
119.54077 44.71839 galactic UMi Second-epoch detections are separated by 0.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687896141301890304 | 13:23:03.17 +72:12:03.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.347+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:03.11 +72:12:04.0: 11.81 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:03.11 +72:12:04.0: 11.82 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687896141301890304,2461335.6793,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687896141301890304 20261022.1793 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.53 13:15:58.55 +71:29:31.8
120.15772 45.50368 galactic UMi Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687799792300092800 | 13:15:58.50 +71:29:31.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.255+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:58.55 +71:29:31.8: 11.79 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:58.55 +71:29:31.8: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687799792300092800,2461335.6793,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687799792300092800 20261022.1793 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.31 13:29:41.97 +71:38:00.1
118.67212 45.17709 galactic UMi Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687111089999705728 | 13:29:42.05 +71:38:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.853+/-0.027 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:29:41.97 +71:38:00.1: 11.80 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:29:41.97 +71:38:00.1: 11.78 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.79 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687111089999705728,2461335.6793,10.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687111089999705728 20261022.1793 10.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.77 12:47:59.90 +72:38:01.7
123.29170 44.49204 galactic Dra Second-epoch detections are separated by 0.3" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:47:59.90 +72:38:01.7 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:47:59.90 +72:38:01.7: 13.92 +/- 0.07 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:47:59.90 +72:38:01.7: 13.87 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.13 12:40:39.87 +73:09:49.0
124.01500 43.94198 galactic Dra Second-epoch detections are separated by 0.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689894709844124032 | 12:40:39.80 +73:09:48.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.548+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:40:39.87 +73:09:49.0: 11.79 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:40:39.87 +73:09:49.0: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689894709844124032,2461335.6793,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689894709844124032 20261022.1793 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.82 13:27:49.33 +71:38:22.9
118.87932 45.20117 galactic UMi Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:27:49.33 +71:38:22.9 (user input) | T | P | (position from user input) J-Ks=0.615+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:49.33 +71:38:22.9: 13.88 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:49.33 +71:38:22.9: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.59 13:07:29.14 +72:31:57.2
121.24343 44.54305 galactic UMi Second-epoch detections are separated by 3.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:07:29.14 +72:31:57.2 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:29.14 +72:31:57.2: 13.86 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:29.14 +72:31:57.2: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.74 13:06:14.57 +73:00:50.9
121.42786 44.07085 galactic UMi Second-epoch detections are separated by 1.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:06:14.57 +73:00:50.9 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.046 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:14.57 +73:00:50.9: 13.84 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:14.57 +73:00:50.9: 13.85 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.73 13:18:59.42 +71:06:15.0
119.73526 45.85269 galactic UMi Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686241135784085376 | 13:18:59.42 +71:06:15.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.594+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:59.42 +71:06:15.0: 11.76 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:59.42 +71:06:15.0: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.77 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686241135784085376,2461335.6793,10.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686241135784085376 20261022.1793 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.35 12:53:21.40 +72:25:56.1
122.72824 44.69524 galactic Dra Second-epoch detections are separated by 0.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1689612513312872960 | 12:53:21.48 +72:25:56.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.320+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:53:21.40 +72:25:56.1: 11.74 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:53:21.40 +72:25:56.1: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1689612513312872960,2461335.6793,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1689612513312872960 20261022.1793 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.46 12:59:42.36 +73:31:47.8
122.12302 43.58532 galactic Dra Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691268893220534528 | 12:59:42.35 +73:31:48.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.861+/-0.029 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:42.36 +73:31:47.8: 11.72 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:42.36 +73:31:47.8: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691268893220534528,2461335.6793,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691268893220534528 20261022.1793 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.57 13:04:04.32 +72:11:18.2
121.56836 44.90640 galactic UMi Second-epoch detections are separated by 3.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:04:04.32 +72:11:18.2 (user input) | T | P | (position from user input) J-Ks=0.640+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:04:04.32 +72:11:18.2: 13.85 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:04:04.32 +72:11:18.2: 13.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.32 12:59:58.49 +72:16:01.9
122.01526 44.84586 galactic Dra Second-epoch detections are separated by 0.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686595762643933824 | 12:59:58.47 +72:16:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.641+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:58.49 +72:16:01.9: 11.72 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:58.49 +72:16:01.9: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686595762643933824,2461335.6793,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686595762643933824 20261022.1793 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.56 13:31:30.72 +71:01:18.8
118.28201 45.74284 galactic UMi Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686939944142769920 | 13:31:30.73 +71:01:18.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.277+/-0.025 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:31:30.72 +71:01:18.8: 11.72 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:31:30.72 +71:01:18.8: 11.73 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686939944142769920,2461335.6793,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686939944142769920 20261022.1793 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.22 13:20:15.34 +71:56:49.3
119.78099 45.00450 galactic UMi Second-epoch detections are separated by 0.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687840577309299968 | 13:20:15.36 +71:56:49.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.562+/-0.025 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:20:15.34 +71:56:49.3: 11.72 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:20:15.34 +71:56:49.3: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687840577309299968,2461335.6793,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687840577309299968 20261022.1793 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.61 12:56:04.03 +73:44:00.0
122.48585 43.39091 galactic Dra Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691321871640991232 | 12:56:04.16 +73:43:59.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:04.03 +73:44:00.0: 11.70 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:04.03 +73:44:00.0: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691321871640991232,2461335.6793,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691321871640991232 20261022.1793 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.56 15:30:30.75 +65:56:33.3
101.65983 44.04637 galactic UMi Second-epoch detections are separated by 1.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644480412850700416 | 15:30:30.65 +65:56:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.358+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:30:30.75 +65:56:33.3: 11.73 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:30:30.75 +65:56:33.3: 11.72 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644480412850700416,2461335.6793,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644480412850700416 20261022.1793 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.35 13:28:23.40 +72:16:58.8
119.00021 44.56208 galactic UMi Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687909915261874944 | 13:28:23.40 +72:16:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.377+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:23.40 +72:16:58.8: 11.70 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:23.40 +72:16:58.8: 11.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687909915261874944,2461335.6793,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687909915261874944 20261022.1793 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.12 13:09:35.39 +72:18:19.3
120.99127 44.75443 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688059556217533056 | 13:09:35.34 +72:18:19.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.598+/-0.024 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:09:35.39 +72:18:19.3: 11.68 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:09:35.39 +72:18:19.3: 11.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688059556217533056,2461335.6793,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688059556217533056 20261022.1793 10.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.38 12:46:13.38 +73:23:53.6
123.44733 43.72481 galactic Dra Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:46:13.38 +73:23:53.6 (user input) | T | P | (position from user input) J-Ks=0.592+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:46:13.38 +73:23:53.6: 13.40 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:46:13.38 +73:23:53.6: 13.42 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.36 13:05:01.67 +72:01:12.2
121.44768 45.06901 galactic UMi Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686575142504764416 | 13:05:01.58 +72:01:12.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.717+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:05:01.67 +72:01:12.2: 11.68 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:05:01.67 +72:01:12.2: 11.69 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686575142504764416,2461335.6793,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686575142504764416 20261022.1793 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.43 13:23:48.95 +71:20:01.3
119.24142 45.56184 galactic UMi Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687736849554797312 | 13:23:49.12 +71:20:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.305+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:48.95 +71:20:01.3: 11.68 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:48.95 +71:20:01.3: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687736849554797312,2461335.6793,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687736849554797312 20261022.1793 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.26 13:19:54.31 +72:27:35.2
119.93104 44.50223 galactic UMi Second-epoch detections are separated by 1.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687951597918921600 | 13:19:54.28 +72:27:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.428+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:54.31 +72:27:35.2: 11.67 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:54.31 +72:27:35.2: 11.71 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687951597918921600,2461335.6793,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687951597918921600 20261022.1793 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.15 12:53:30.40 +73:30:54.2
122.72922 43.61238 galactic Dra Second-epoch detections are separated by 1.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691221408061002752 | 12:53:30.49 +73:30:54.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.576+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:53:30.40 +73:30:54.2: 11.65 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:53:30.40 +73:30:54.2: 11.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691221408061002752,2461335.6793,10.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691221408061002752 20261022.1793 10.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.26 13:15:25.65 +72:28:57.1
120.40357 44.52777 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687960703250338048 | 13:15:25.68 +72:28:56.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.383+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:25.65 +72:28:57.1: 11.66 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:25.65 +72:28:57.1: 11.66 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687960703250338048,2461335.6793,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687960703250338048 20261022.1793 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.17 12:57:01.28 +72:31:02.8
122.34299 44.60442 galactic Dra Second-epoch detections are separated by 0.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689606053682018432 | 12:57:01.28 +72:31:02.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.199+/-0.025 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:57:01.28 +72:31:02.8: 11.63 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:57:01.28 +72:31:02.8: 11.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689606053682018432,2461335.6793,10.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689606053682018432 20261022.1793 10.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.64 13:35:11.50 +70:45:22.3
117.77295 45.93128 galactic UMi Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686918709824416128 | 13:35:11.49 +70:45:22.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.263+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:35:11.50 +70:45:22.3: 11.63 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:35:11.50 +70:45:22.3: 11.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.64 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686918709824416128,2461335.6793,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686918709824416128 20261022.1793 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.78 12:42:14.72 +72:54:27.9
123.87394 44.20368 galactic Dra Second-epoch detections are separated by 1.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689863854799048704 | 12:42:14.72 +72:54:28.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.639+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:42:14.72 +72:54:27.9: 11.30 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:42:14.72 +72:54:27.9: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689863854799048704,2461335.6793,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689863854799048704 20261022.1793 9.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.81 12:45:16.50 +72:47:01.5
123.56943 44.33687 galactic Dra Second-epoch detections are separated by 0.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689847087246679936 | 12:45:16.44 +72:47:02.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.606+/-0.024 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:45:16.50 +72:47:01.5: 11.25 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:45:16.50 +72:47:01.5: 11.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689847087246679936,2461335.6793,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689847087246679936 20261022.1793 9.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.54 13:10:21.41 +71:29:45.1
120.79018 45.55363 galactic UMi Second-epoch detections are separated by 0.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686496497359684608 | 13:10:21.45 +71:29:45.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.296+/-0.027 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:10:21.41 +71:29:45.1: 11.59 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:10:21.41 +71:29:45.1: 11.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.59 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686496497359684608,2461335.6793,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686496497359684608 20261022.1793 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.32 13:15:10.77 +71:35:10.6
120.26470 45.41882 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687814158966217600 | 13:15:10.77 +71:35:10.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.224+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:10.77 +71:35:10.6: 11.57 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:10.77 +71:35:10.6: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.57 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687814158966217600,2461335.6793,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687814158966217600 20261022.1793 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.72 12:51:09.46 +72:54:30.7
122.96065 44.21971 galactic Dra Second-epoch detections are separated by 1.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:51:09.46 +72:54:30.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:51:09.46 +72:54:30.7: 13.84 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:51:09.46 +72:54:30.7: 13.82 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.55 15:25:13.93 +66:40:57.3
102.92411 43.99815 galactic UMi Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644762746820868096 | 15:25:13.84 +66:40:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.466+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:25:13.93 +66:40:57.3: 11.58 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:25:13.93 +66:40:57.3: 11.57 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644762746820868096,2461335.6793,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644762746820868096 20261022.1793 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.06 13:03:01.60 +72:23:53.6
121.69973 44.70229 galactic Dra Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688096527296069504 | 13:03:01.55 +72:23:53.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.622+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:03:01.60 +72:23:53.6: 11.55 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:03:01.60 +72:23:53.6: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688096527296069504,2461335.6793,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688096527296069504 20261022.1793 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.06 13:12:12.08 +72:17:46.1
120.71200 44.74251 galactic UMi Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688048080064883072 | 13:12:12.00 +72:17:46.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.402+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:12:12.08 +72:17:46.1: 11.54 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:12:12.08 +72:17:46.1: 11.52 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688048080064883072,2461335.6793,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688048080064883072 20261022.1793 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.64 13:34:51.12 +70:39:22.9
117.77734 46.03494 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686915754886174336 | 13:34:51.11 +70:39:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.328+/-0.035 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:34:51.12 +70:39:22.9: 11.53 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:34:51.12 +70:39:22.9: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.53 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686915754886174336,2461335.6793,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686915754886174336 20261022.1793 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.27 13:06:58.61 +71:54:42.0
121.22230 45.16497 galactic UMi Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686526321612604160 | 13:06:58.73 +71:54:41.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.279+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:58.61 +71:54:42.0: 11.52 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:58.61 +71:54:42.0: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686526321612604160,2461335.6793,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686526321612604160 20261022.1793 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.05 13:07:38.62 +72:57:40.7
121.27954 44.11491 galactic UMi Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688223138636477440 | 13:07:38.62 +72:57:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.627+/-0.025 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:38.62 +72:57:40.7: 11.47 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:38.62 +72:57:40.7: 11.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688223138636477440,2461335.6793,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688223138636477440 20261022.1793 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.06 12:53:53.44 +73:27:44.7
122.69064 43.66469 galactic Dra Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691220995744845440 | 12:53:53.33 +73:27:44.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.713+/-0.025 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:53:53.44 +73:27:44.7: 11.45 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:53:53.44 +73:27:44.7: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.45 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691220995744845440,2461335.6793,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691220995744845440 20261022.1793 10.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.27 12:58:13.25 +72:07:39.4
122.19614 44.99095 galactic Dra Second-epoch detections are separated by 0.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689589664086799360 | 12:58:13.30 +72:07:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.380+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:13.25 +72:07:39.4: 11.46 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:13.25 +72:07:39.4: 11.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.48 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689589664086799360,2461335.6793,10.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689589664086799360 20261022.1793 10.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.65 12:48:07.67 +73:06:03.1
123.26646 44.02524 galactic Dra Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:48:07.67 +73:06:03.1 (user input) | T | P | (position from user input) J-Ks=0.363+/-0.027 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:48:07.67 +73:06:03.1: 13.84 +/- 0.07 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:48:07.67 +73:06:03.1: 13.94 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.89 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.21 12:55:10.56 +73:41:29.7
122.57055 43.43405 galactic Dra Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691316305363376896 | 12:55:10.59 +73:41:29.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.296+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:55:10.56 +73:41:29.7: 11.46 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:55:10.56 +73:41:29.7: 11.48 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691316305363376896,2461335.6793,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691316305363376896 20261022.1793 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.46 13:19:24.05 +72:56:45.9
120.08642 44.02734 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688000285668921856 | 13:19:24.12 +72:56:46.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.445+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:24.05 +72:56:45.9: 11.44 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:24.05 +72:56:45.9: 11.44 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688000285668921856,2461335.6793,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688000285668921856 20261022.1793 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.04 12:48:42.43 +73:27:28.0
123.20063 43.66905 galactic Dra Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691206839532681344 | 12:48:42.38 +73:27:28.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:48:42.43 +73:27:28.0: 11.45 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:48:42.43 +73:27:28.0: 11.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691206839532681344,2461335.6793,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691206839532681344 20261022.1793 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.37 15:31:51.21 +65:47:40.0
101.38034 44.02736 galactic UMi Second-epoch detections are separated by 1.2" and 6.5 pix
The object was found in VSX 1" Gaia DR3 1644463537923339392
Type: ROT
# Max. Min./Amp. JD0 Period
11.240 G 11.280 G G
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:31:51.21 +65:47:40.0: 11.43 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:31:51.21 +65:47:40.0: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644463537923339392,2461335.6793,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644463537923339392 20261022.1793 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.83 13:33:35.69 +71:50:20.1
118.31471 44.90948 galactic UMi Second-epoch detections are separated by 1.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:33:35.69 +71:50:20.1 (user input) | T | P | (position from user input) J-Ks=0.467+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:33:35.69 +71:50:20.1: 13.81 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:33:35.69 +71:50:20.1: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.10 13:02:41.04 +73:16:08.6
121.81026 43.83469 galactic Dra Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691244807043471232 | 13:02:41.01 +73:16:08.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.611+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:02:41.04 +73:16:08.6: 11.41 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:02:41.04 +73:16:08.6: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.43 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691244807043471232,2461335.6793,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691244807043471232 20261022.1793 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.10 13:25:30.35 +72:11:17.3
119.27780 44.69761 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687882259967545216 | 13:25:30.32 +72:11:17.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.638+/-0.033 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:30.35 +72:11:17.3: 11.41 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:30.35 +72:11:17.3: 11.43 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.42 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687882259967545216,2461335.6793,10.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687882259967545216 20261022.1793 10.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.16 13:27:03.84 +71:21:44.7
118.88503 45.48486 galactic UMi Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687012924227115264 | 13:27:03.98 +71:21:45.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.513+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:03.84 +71:21:44.7: 11.41 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:03.84 +71:21:44.7: 11.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687012924227115264,2461335.6793,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687012924227115264 20261022.1793 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.78 13:24:19.97 +72:16:40.8
119.42451 44.62555 galactic UMi Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:24:19.97 +72:16:40.8 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:24:19.97 +72:16:40.8: 13.81 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:24:19.97 +72:16:40.8: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.04 12:55:27.64 +73:34:50.8
122.53975 43.54441 galactic Dra Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691313663959232128 | 12:55:27.74 +73:34:50.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.269+/-0.027 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:55:27.64 +73:34:50.8: 11.38 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:55:27.64 +73:34:50.8: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.37 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691313663959232128,2461335.6793,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691313663959232128 20261022.1793 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.36 12:41:37.94 +72:39:28.1
123.95527 44.45096 galactic Dra Second-epoch detections are separated by 0.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689853375079316224 | 12:41:37.80 +72:39:27.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.379+/-0.026 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:41:37.94 +72:39:28.1: 11.46 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:41:37.94 +72:39:28.1: 11.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.46 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689853375079316224,2461335.6793,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689853375079316224 20261022.1793 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.77 12:53:46.89 +72:39:27.3
122.68719 44.46955 galactic Dra Second-epoch detections are separated by 1.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:53:46.89 +72:39:27.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:53:46.89 +72:39:27.3: 13.79 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:53:46.89 +72:39:27.3: 13.83 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.73 13:21:38.79 +72:22:17.3
119.72915 44.56844 galactic UMi Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:21:38.79 +72:22:17.3 (user input) | T | P | (position from user input) J-Ks=0.297+/-0.036 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:38.79 +72:22:17.3: 13.76 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:38.79 +72:22:17.3: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.21 13:15:36.74 +71:31:36.6
120.20511 45.47321 galactic UMi Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687800621229298816 | 13:15:36.73 +71:31:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.278+/-0.027 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:36.74 +71:31:36.6: 11.36 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:36.74 +71:31:36.6: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687800621229298816,2461335.6793,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687800621229298816 20261022.1793 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.32 12:56:58.43 +72:04:42.6
122.32924 45.04327 galactic Dra Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689569494920376448 | 12:56:58.49 +72:04:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.267+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:58.43 +72:04:42.6: 11.35 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:58.43 +72:04:42.6: 11.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.35 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689569494920376448,2461335.6793,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689569494920376448 20261022.1793 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.55 12:50:43.42 +72:45:48.8
123.00593 44.36459 galactic Dra Second-epoch detections are separated by 2.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:50:43.42 +72:45:48.8 (user input) | T | P | (position from user input) J-Ks=0.355+/-0.035 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:50:43.42 +72:45:48.8: 13.76 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:50:43.42 +72:45:48.8: 13.86 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.88 12:59:29.29 +72:43:47.7
122.09602 44.38527 galactic Dra Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691112590770232704 | 12:59:29.30 +72:43:47.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.652+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:29.29 +72:43:47.7: 11.34 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:29.29 +72:43:47.7: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.35 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691112590770232704,2461335.6793,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691112590770232704 20261022.1793 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.62 13:09:38.74 +72:36:50.6
121.02834 44.44684 galactic UMi Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:09:38.74 +72:36:50.6 (user input) | T | P | (position from user input) J-Ks=0.451+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:09:38.74 +72:36:50.6: 13.78 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:09:38.74 +72:36:50.6: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.29 13:13:41.66 +71:25:39.4
120.40257 45.59118 galactic UMi Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686311092211454080 | 13:13:41.68 +71:25:39.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.638+/-0.025 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:13:41.66 +71:25:39.4: 11.34 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:13:41.66 +71:25:39.4: 11.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.35 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686311092211454080,2461335.6793,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686311092211454080 20261022.1793 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.93 12:57:59.23 +72:27:33.7
122.23825 44.66007 galactic Dra Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689604748011957248 | 12:57:59.18 +72:27:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.664+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:57:59.23 +72:27:33.7: 11.33 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:57:59.23 +72:27:33.7: 11.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.31 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689604748011957248,2461335.6793,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689604748011957248 20261022.1793 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.19 13:31:41.82 +71:09:49.5
118.30619 45.60119 galactic UMi Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686948877674751360 | 13:31:41.89 +71:09:49.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.256+/-0.025 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:31:41.82 +71:09:49.5: 11.34 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:31:41.82 +71:09:49.5: 11.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.35 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686948877674751360,2461335.6793,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686948877674751360 20261022.1793 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.36 13:32:11.93 +70:52:05.7
118.15425 45.88002 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was found in VSX 1" Gaia DR3 1686934137346978304
Type: ROT
# Max. Min./Amp. JD0 Period
11.100 G 11.150 G K
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:11.93 +70:52:05.7: 11.33 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:11.93 +70:52:05.7: 11.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686934137346978304,2461335.6793,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686934137346978304 20261022.1793 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.04 13:06:22.45 +73:06:01.7
121.42424 43.98403 galactic UMi Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688236921187184768 | 13:06:22.58 +73:06:00.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.264+/-0.024 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:22.45 +73:06:01.7: 11.30 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:22.45 +73:06:01.7: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688236921187184768,2461335.6793,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688236921187184768 20261022.1793 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.33 13:30:34.13 +70:47:33.1
118.31769 45.98354 galactic UMi Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686912971748139648 | 13:30:34.16 +70:47:33.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.655+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:30:34.13 +70:47:33.1: 11.30 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:30:34.13 +70:47:33.1: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686912971748139648,2461335.6793,10.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686912971748139648 20261022.1793 10.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.05 13:35:27.73 +71:16:15.3
117.92102 45.42658 galactic UMi Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687034914459696512 | 13:35:27.76 +71:16:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.693+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:35:27.73 +71:16:15.3: 11.29 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:35:27.73 +71:16:15.3: 11.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687034914459696512,2461335.6793,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687034914459696512 20261022.1793 10.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.37 13:13:31.62 +73:12:51.1
120.72448 43.81926 galactic UMi Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688208986719860096 | 13:13:31.68 +73:12:51.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.377+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:13:31.62 +73:12:51.1: 11.26 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:13:31.62 +73:12:51.1: 11.25 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.26 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688208986719860096,2461335.6793,10.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688208986719860096 20261022.1793 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.44 13:38:18.10 +71:59:08.1
117.86522 44.67876 galactic UMi Second-epoch detections are separated by 0.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687462761922286336 | 13:38:18.35 +71:59:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:38:18.10 +71:59:08.1: 11.27 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:38:18.10 +71:59:08.1: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687462761922286336,2461335.6793,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687462761922286336 20261022.1793 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.96 13:27:09.45 +71:37:01.0
118.94580 45.23383 galactic UMi Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687113770059337088 | 13:27:09.16 +71:37:01.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.378+/-0.044 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:09.45 +71:37:01.0: 11.25 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:09.45 +71:37:01.0: 11.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.24 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687113770059337088,2461335.6793,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687113770059337088 20261022.1793 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.04 13:06:37.92 +71:49:10.7
121.24919 45.25894 galactic UMi Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686524122589346560 | 13:06:37.94 +71:49:10.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.752+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:37.92 +71:49:10.7: 11.18 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:37.92 +71:49:10.7: 11.17 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686524122589346560,2461335.6793,10.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686524122589346560 20261022.1793 10.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.26 13:09:49.33 +71:29:36.3
120.85008 45.56045 galactic UMi Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686496325560993152 | 13:09:49.15 +71:29:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.314+/-0.027 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:09:49.33 +71:29:36.3: 11.17 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:09:49.33 +71:29:36.3: 11.16 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686496325560993152,2461335.6793,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686496325560993152 20261022.1793 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.93 12:56:48.04 +73:24:02.2
122.40200 43.72212 galactic Dra Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691170727447609472 | 12:56:48.06 +73:24:01.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.254+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:48.04 +73:24:02.2: 11.19 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:48.04 +73:24:02.2: 11.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.19 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691170727447609472,2461335.6793,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691170727447609472 20261022.1793 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.83 13:08:36.45 +72:34:01.6
121.13033 44.50103 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688072819076563456 | 13:08:36.38 +72:34:02.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.764+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:08:36.45 +72:34:01.6: 11.17 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:08:36.45 +72:34:01.6: 11.18 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.18 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688072819076563456,2461335.6793,9.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688072819076563456 20261022.1793 9.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.89 12:53:43.46 +73:41:35.5
122.71090 43.43408 galactic Dra Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691318096365487744 | 12:53:43.43 +73:41:35.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.574+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:53:43.46 +73:41:35.5: 11.15 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:53:43.46 +73:41:35.5: 11.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691318096365487744,2461335.6793,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691318096365487744 20261022.1793 9.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.79 12:58:13.32 +72:32:40.1
122.21781 44.57437 galactic Dra Second-epoch detections are separated by 0.3" and 7.5 pix
The object was found in VSX 7" Gaia DR3 1691106302938134016
Type: ROT
# Max. Min./Amp. JD0 Period
14.430 G 14.460 G K
ATTENTION: measured mag 9.79 is 4.6 mag brighter than the VSX record maximum brightness 14.43 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:13.32 +72:32:40.1: 11.16 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:13.32 +72:32:40.1: 11.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691106302938134016,2461335.6793,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691106302938134016 20261022.1793 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.14 15:30:26.56 +65:59:47.7
101.72534 44.01901 galactic UMi Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644481855959713280 | 15:30:26.56 +65:59:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.374+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:30:26.56 +65:59:47.7: 11.15 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:30:26.56 +65:59:47.7: 11.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644481855959713280,2461335.6793,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644481855959713280 20261022.1793 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.62 12:58:13.32 +72:38:48.0
122.22311 44.47225 galactic Dra Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:58:13.32 +72:38:48.0 (user input) | T | P | (position from user input) J-Ks=0.595+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:13.32 +72:38:48.0: 13.74 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:13.32 +72:38:48.0: 13.96 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.87 13:14:05.78 +72:23:39.7
120.52769 44.62796 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688052508175531392 | 13:14:05.82 +72:23:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.363+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:05.78 +72:23:39.7: 11.11 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:05.78 +72:23:39.7: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688052508175531392,2461335.6793,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688052508175531392 20261022.1793 9.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.91 15:30:36.25 +66:16:20.0
102.01400 43.83729 galactic UMi Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644700139081710720 | 15:30:36.22 +66:16:19.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.262+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:30:36.25 +66:16:20.0: 11.07 +/- 0.01 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:30:36.25 +66:16:20.0: 11.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.09 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644700139081710720,2461335.6793,9.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644700139081710720 20261022.1793 9.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.79 13:18:25.86 +71:56:30.8
119.97753 45.03120 galactic UMi Second-epoch detections are separated by 2.8" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:18:25.86 +71:56:30.8 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:25.86 +71:56:30.8: 13.70 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:25.86 +71:56:30.8: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.89 13:09:23.80 +71:46:20.2
120.93751 45.28636 galactic UMi Second-epoch detections are separated by 0.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686509657139491328 | 13:09:23.65 +71:46:20.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.799+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:09:23.80 +71:46:20.2: 11.05 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:09:23.80 +71:46:20.2: 11.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.05 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686509657139491328,2461335.6793,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686509657139491328 20261022.1793 9.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.16 13:30:17.47 +70:48:43.0
118.35581 45.96954 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686913792086669184 | 13:30:17.44 +70:48:43.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.653+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:30:17.47 +70:48:43.0: 11.07 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:30:17.47 +70:48:43.0: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686913792086669184,2461335.6793,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686913792086669184 20261022.1793 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.69 12:55:27.84 +72:59:31.0
122.52173 44.13310 galactic Dra Second-epoch detections are separated by 0.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691134993320291328 | 12:55:27.84 +72:59:31.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.596+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:55:27.84 +72:59:31.0: 11.04 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:55:27.84 +72:59:31.0: 11.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.04 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691134993320291328,2461335.6793,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691134993320291328 20261022.1793 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.94 13:26:11.11 +72:28:30.5
119.28197 44.40603 galactic UMi Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687927133785870080 | 13:26:11.04 +72:28:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.797+/-0.040 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:26:11.11 +72:28:30.5: 11.05 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:26:11.11 +72:28:30.5: 11.06 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.06 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687927133785870080,2461335.6793,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687927133785870080 20261022.1793 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.80 12:56:39.60 +73:24:41.5
122.41632 43.71150 galactic Dra Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691171483361131520 | 12:56:39.54 +73:24:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:39.60 +73:24:41.5: 11.03 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:39.60 +73:24:41.5: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691171483361131520,2461335.6793,9.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691171483361131520 20261022.1793 9.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.94 13:30:39.53 +72:06:57.0
118.71325 44.68976 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1687153696075307776 | 13:30:39.48 +72:06:57.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.376+/-0.036 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:30:39.53 +72:06:57.0: 11.04 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:30:39.53 +72:06:57.0: 11.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.04 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1687153696075307776,2461335.6793,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1687153696075307776 20261022.1793 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.65 13:05:35.49 +72:36:10.2
121.44980 44.48466 galactic UMi Second-epoch detections are separated by 1.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:05:35.49 +72:36:10.2 (user input) | T | P | (position from user input) J-Ks=0.370+/-0.035 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:05:35.49 +72:36:10.2: 13.70 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:05:35.49 +72:36:10.2: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.87 13:02:47.69 +72:07:41.9
121.70068 44.97279 galactic Dra Second-epoch detections are separated by 0.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1686591502036343936 | 13:02:47.63 +72:07:42.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.629+/-0.030 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:02:47.69 +72:07:41.9: 11.01 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:02:47.69 +72:07:41.9: 10.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.00 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1686591502036343936,2461335.6793,9.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1686591502036343936 20261022.1793 9.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.77 13:22:14.55 +71:53:42.1
119.55384 45.03063 galactic UMi Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687789866631131392 | 13:22:14.61 +71:53:41.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.282+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:22:14.55 +71:53:42.1: 11.02 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:22:14.55 +71:53:42.1: 11.03 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687789866631131392,2461335.6793,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687789866631131392 20261022.1793 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.77 13:02:47.64 +72:20:36.7
121.71966 44.75798 galactic Dra Second-epoch detections are separated by 0.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688095943180512896 | 13:02:47.65 +72:20:36.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1956PMcCO..13a....B AG+72 344 J-Ks=0.083+/-0.030 (A)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:02:47.64 +72:20:36.7: 11.01 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:02:47.64 +72:20:36.7: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.01 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688095943180512896,2461335.6793,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688095943180512896 20261022.1793 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.14 13:33:41.75 +72:13:21.9
118.42795 44.53409 galactic UMi Second-epoch detections are separated by 0.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687518940094081152 | 13:33:41.77 +72:13:22.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.148+/-0.034 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:33:41.75 +72:13:21.9: 11.01 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:33:41.75 +72:13:21.9: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687518940094081152,2461335.6793,10.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687518940094081152 20261022.1793 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.93 13:38:25.39 +71:21:43.9
117.62672 45.27896 galactic UMi Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687055976979845888 | 13:38:25.45 +71:21:43.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.327+/-0.025 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:38:25.39 +71:21:43.9: 10.99 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:38:25.39 +71:21:43.9: 10.98 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.98 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687055976979845888,2461335.6793,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687055976979845888 20261022.1793 9.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.82 13:05:17.21 +72:58:12.6
121.52017 44.12010 galactic UMi Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:05:17.21 +72:58:12.6 (user input) | T | P | (position from user input) J-Ks=0.693+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:05:17.21 +72:58:12.6: 13.71 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:05:17.21 +72:58:12.6: 13.84 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.71 13:01:32.26 +72:59:58.2
121.90404 44.10859 galactic Dra Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691146057156031616 | 13:01:32.32 +72:59:57.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.275+/-0.027 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:32.26 +72:59:58.2: 10.98 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:32.26 +72:59:58.2: 10.98 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.98 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691146057156031616,2461335.6793,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691146057156031616 20261022.1793 9.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.70 13:14:57.95 +72:09:22.5
120.39301 44.85583 galactic UMi Second-epoch detections are separated by 1.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:14:57.95 +72:09:22.5 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:57.95 +72:09:22.5: 13.70 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:57.95 +72:09:22.5: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.74 12:58:11.39 +72:24:21.6
122.21403 44.71284 galactic Dra Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689601208959399680 | 12:58:11.38 +72:24:21.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.385+/-0.027 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:11.39 +72:24:21.6: 10.97 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:11.39 +72:24:21.6: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.97 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689601208959399680,2461335.6793,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689601208959399680 20261022.1793 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.94 13:12:36.34 +71:37:05.6
120.55741 45.41231 galactic UMi Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687817423141872256 | 13:12:36.56 +71:37:05.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:12:36.34 +71:37:05.6: 10.98 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:12:36.34 +71:37:05.6: 10.97 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.98 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687817423141872256,2461335.6793,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687817423141872256 20261022.1793 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.67 13:13:45.43 +72:37:49.5
120.60363 44.39680 galactic UMi Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688153014706575488 | 13:13:45.49 +72:37:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.968+/-0.026 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:13:45.43 +72:37:49.5: 10.95 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:13:45.43 +72:37:49.5: 10.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.95 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688153014706575488,2461335.6793,9.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688153014706575488 20261022.1793 9.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.67 13:18:02.75 +71:58:55.7
120.02761 44.99576 galactic UMi Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687843089865904384 | 13:18:02.94 +71:58:55.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.363+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:02.75 +71:58:55.7: 10.94 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:02.75 +71:58:55.7: 10.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.95 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687843089865904384,2461335.6793,9.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687843089865904384 20261022.1793 9.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.77 13:14:45.15 +72:22:38.8
120.45551 44.63853 galactic UMi Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688052306312706176 | 13:14:45.18 +72:22:38.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.518+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:45.15 +72:22:38.8: 10.94 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:45.15 +72:22:38.8: 10.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.95 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688052306312706176,2461335.6793,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688052306312706176 20261022.1793 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.67 13:11:26.71 +72:26:15.0
120.81413 44.60839 galactic UMi Second-epoch detections are separated by 1.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688067562036545920 | 13:11:26.66 +72:26:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.825+/-0.034 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:11:26.71 +72:26:15.0: 10.93 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:11:26.71 +72:26:15.0: 10.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688067562036545920,2461335.6793,9.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688067562036545920 20261022.1793 9.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.61 13:12:40.00 +72:14:22.0
120.65326 44.79476 galactic UMi Second-epoch detections are separated by 1.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:12:40.00 +72:14:22.0 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.036 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:12:40.00 +72:14:22.0: 13.69 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:12:40.00 +72:14:22.0: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.65 12:44:23.09 +73:33:00.3
123.62097 43.56873 galactic Dra Second-epoch detections are separated by 1.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691398360714235904 | 12:44:23.13 +73:33:00.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.628+/-0.024 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:44:23.09 +73:33:00.3: 10.92 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:44:23.09 +73:33:00.3: 10.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691398360714235904,2461335.6793,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691398360714235904 20261022.1793 9.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.68 12:57:03.50 +73:13:07.1
122.36892 43.90347 galactic Dra Second-epoch detections are separated by 0.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691158804618982784 | 12:57:03.49 +73:13:07.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.309+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:57:03.50 +73:13:07.1: 10.90 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:57:03.50 +73:13:07.1: 10.89 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.90 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691158804618982784,2461335.6793,9.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691158804618982784 20261022.1793 9.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.60 12:58:10.36 +72:28:01.6
122.21901 44.65182 galactic Dra Second-epoch detections are separated by 0.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689604713652219008 | 12:58:10.35 +72:28:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.681+/-0.025 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:10.36 +72:28:01.6: 10.89 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:10.36 +72:28:01.6: 10.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.90 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689604713652219008,2461335.6793,9.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689604713652219008 20261022.1793 9.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.61 12:59:36.62 +73:07:19.6
122.10754 43.99306 galactic Dra Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691151309899576448 | 12:59:36.64 +73:07:19.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.336+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:36.62 +73:07:19.6: 10.89 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:36.62 +73:07:19.6: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.88 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691151309899576448,2461335.6793,9.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691151309899576448 20261022.1793 9.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.79 15:28:55.94 +66:26:17.9
102.33870 43.86652 galactic UMi Second-epoch detections are separated by 0.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644716361174025472 | 15:28:55.95 +66:26:17.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.288+/-0.032 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:28:55.94 +66:26:17.9: 10.89 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:28:55.94 +66:26:17.9: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.88 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644716361174025472,2461335.6793,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644716361174025472 20261022.1793 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.60 12:40:22.64 +73:16:32.8
124.03455 43.82879 galactic Dra Second-epoch detections are separated by 0.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689902097187882880 | 12:40:22.78 +73:16:32.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.266+/-0.021 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:40:22.64 +73:16:32.8: 10.92 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:40:22.64 +73:16:32.8: 10.91 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689902097187882880,2461335.6793,9.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689902097187882880 20261022.1793 9.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.88 13:14:58.52 +73:02:21.4
120.54993 43.97995 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688188851913137536 | 13:14:58.52 +73:02:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.763+/-0.026 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:14:58.52 +73:02:21.4: 10.86 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:14:58.52 +73:02:21.4: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688188851913137536,2461335.6793,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688188851913137536 20261022.1793 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.88 15:27:08.39 +66:24:52.0
102.46848 44.02130 galactic UMi Second-epoch detections are separated by 0.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644740790948461696 | 15:27:08.39 +66:24:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.783+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:27:08.39 +66:24:52.0: 10.87 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:27:08.39 +66:24:52.0: 10.86 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.87 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644740790948461696,2461335.6793,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644740790948461696 20261022.1793 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.73 13:26:05.25 +72:26:40.0
119.28401 44.43756 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687926515310577792 | 13:26:05.22 +72:26:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.330+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:26:05.25 +72:26:40.0: 10.83 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:26:05.25 +72:26:40.0: 10.83 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687926515310577792,2461335.6793,9.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687926515310577792 20261022.1793 9.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.69 13:02:01.45 +73:17:18.6
121.87751 43.81807 galactic Dra Second-epoch detections are separated by 1.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691245734756868992 | 13:02:01.57 +73:17:18.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1956PMcCO..13a....B AG+73 341 J-Ks=0.246+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:02:01.45 +73:17:18.6: 10.82 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:02:01.45 +73:17:18.6: 10.82 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.82 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691245734756868992,2461335.6793,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691245734756868992 20261022.1793 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.76 13:01:44.75 +72:30:31.8
121.84448 44.59765 galactic Dra Second-epoch detections are separated by 1.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:01:44.75 +72:30:31.8 (user input) | T | P | (position from user input) J-Ks=0.428+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:44.75 +72:30:31.8: 13.70 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:44.75 +72:30:31.8: 13.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.63 13:19:44.06 +71:48:17.9
119.80618 45.15115 galactic UMi Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:19:44.06 +71:48:17.9 (user input) | T | P | (position from user input) J-Ks=0.297+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:44.06 +71:48:17.9: 13.69 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:44.06 +71:48:17.9: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.74 13:25:49.95 +71:19:29.6
119.01258 45.54072 galactic UMi Second-epoch detections are separated by 1.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687009625692229632 | 13:25:49.89 +71:19:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.705+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:25:49.95 +71:19:29.6: 10.81 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:25:49.95 +71:19:29.6: 10.82 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.82 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687009625692229632,2461335.6793,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687009625692229632 20261022.1793 9.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.94 15:34:41.44 +66:38:48.3
102.08255 43.28567 galactic UMi Second-epoch detections are separated by 0.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644802909059370496 | 15:34:49.14 +66:38:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.623+/-0.025 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:34:41.44 +66:38:48.3: 10.78 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:34:41.44 +66:38:48.3: 10.79 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.79 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644802909059370496,2461335.6793,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644802909059370496 20261022.1793 9.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.69 13:27:35.12 +71:57:24.0
118.99403 44.89417 galactic UMi Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687875800336757120 | 13:27:35.10 +71:57:23.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.428+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:35.12 +71:57:24.0: 10.76 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:35.12 +71:57:24.0: 10.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.77 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687875800336757120,2461335.6793,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687875800336757120 20261022.1793 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.81 15:35:55.99 +66:40:56.0
102.02040 43.16589 galactic UMi Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644620699366588544 | 15:35:56.11 +66:40:55.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.395+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:35:55.99 +66:40:56.0: 10.75 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:35:55.99 +66:40:56.0: 10.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.75 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644620699366588544,2461335.6793,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644620699366588544 20261022.1793 9.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.77 15:27:00.65 +66:36:15.0
102.68446 43.91177 galactic UMi Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644746151067238528 | 15:27:00.78 +66:36:14.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.048+/-0.029 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:27:00.65 +66:36:15.0: 10.76 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:27:00.65 +66:36:15.0: 10.74 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.75 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644746151067238528,2461335.6793,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644746151067238528 20261022.1793 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.53 13:06:49.50 +72:59:51.6
121.36698 44.08380 galactic UMi Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688224242443721600 | 13:06:49.50 +72:59:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.827+/-0.031 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:06:49.50 +72:59:51.6: 10.71 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:06:49.50 +72:59:51.6: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.71 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688224242443721600,2461335.6793,9.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688224242443721600 20261022.1793 9.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.70 15:33:02.87 +65:39:21.6
101.12389 44.01231 galactic UMi Second-epoch detections are separated by 1.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644435092355019264 | 15:33:02.84 +65:39:22.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.880+/-0.035 (M)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:33:02.87 +65:39:21.6: 10.71 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:33:02.87 +65:39:21.6: 10.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.72 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644435092355019264,2461335.6793,9.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644435092355019264 20261022.1793 9.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.38 12:59:01.22 +72:57:48.4
122.15797 44.15341 galactic Dra Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691142930419839488 | 12:59:01.71 +72:57:47.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:59:01.22 +72:57:48.4: 10.67 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:59:01.22 +72:57:48.4: 10.65 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.66 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691142930419839488,2461335.6793,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691142930419839488 20261022.1793 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.47 13:07:33.81 +72:21:04.7
121.21287 44.72308 galactic UMi Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688040452203006080 | 13:07:33.87 +72:21:04.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.156+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:07:33.81 +72:21:04.7: 10.68 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:07:33.81 +72:21:04.7: 10.67 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.67 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688040452203006080,2461335.6793,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688040452203006080 20261022.1793 9.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.51 13:15:32.61 +72:25:15.8
120.38012 44.58757 galactic UMi Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687958985263417344 | 13:15:32.61 +72:25:15.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.414+/-0.038 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:15:32.61 +72:25:15.8: 10.65 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:15:32.61 +72:25:15.8: 10.62 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.63 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687958985263417344,2461335.6793,9.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687958985263417344 20261022.1793 9.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.69 13:21:04.85 +71:24:56.5
119.56865 45.51849 galactic UMi Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687752891257228288 | 13:21:04.79 +71:24:56.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.590+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:04.85 +71:24:56.5: 10.67 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:04.85 +71:24:56.5: 10.66 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.67 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687752891257228288,2461335.6793,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687752891257228288 20261022.1793 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.64 13:01:47.15 +72:18:24.1
121.82419 44.79929 galactic Dra Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:01:47.15 +72:18:24.1 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.035 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:47.15 +72:18:24.1: 13.66 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:47.15 +72:18:24.1: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.62 13:03:29.81 +72:40:31.1
121.67538 44.42351 galactic Dra Second-epoch detections are separated by 1.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:03:29.81 +72:40:31.1 (user input) | T | P | (position from user input) J-Ks=0.391+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:03:29.81 +72:40:31.1: 13.64 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:03:29.81 +72:40:31.1: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.62 13:02:40.92 +72:44:20.7
121.76560 44.36370 galactic Dra Second-epoch detections are separated by 2.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:02:40.92 +72:44:20.7 (user input) | T | P | (position from user input) J-Ks=0.656+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:02:40.92 +72:44:20.7: 13.67 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:02:40.92 +72:44:20.7: 13.58 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.63 13:17:58.18 +71:50:32.8
120.00706 45.13483 galactic UMi Second-epoch detections are separated by 2.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:17:58.18 +71:50:32.8 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:17:58.18 +71:50:32.8: 13.66 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:17:58.18 +71:50:32.8: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.47 12:56:31.37 +73:20:25.1
122.42716 43.78296 galactic Dra Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691168665863304832 | 12:56:31.34 +73:20:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.295+/-0.030 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:56:31.37 +73:20:25.1: 10.57 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:56:31.37 +73:20:25.1: 10.58 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.57 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691168665863304832,2461335.6793,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691168665863304832 20261022.1793 9.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.47 12:49:05.93 +73:14:01.5
123.16600 43.89344 galactic Dra Second-epoch detections are separated by 3.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:49:05.93 +73:14:01.5 (user input) | T | P | (position from user input) J-Ks=0.304+/-0.034 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:49:05.93 +73:14:01.5: 13.75 +/- 0.06 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:49:05.93 +73:14:01.5: 13.80 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.79 13:34:47.19 +71:51:11.5
118.19199 44.87397 galactic UMi Second-epoch detections are separated by 4.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:34:47.19 +71:51:11.5 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.037 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:34:47.19 +71:51:11.5: 13.65 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:34:47.19 +71:51:11.5: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.44 13:21:17.88 +72:33:25.2
119.80783 44.38967 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687975340499305344 | 13:21:17.88 +72:33:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1956PMcCO..13a....B AG+72 351 J-Ks=0.755+/-0.032 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:21:17.88 +72:33:25.2: 10.53 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:21:17.88 +72:33:25.2: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.53 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687975340499305344,2461335.6793,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687975340499305344 20261022.1793 9.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.44 15:38:54.93 +66:17:18.3
101.34391 43.15718 galactic UMi Second-epoch detections are separated by 1.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1644550815955436672 | 15:38:54.78 +66:17:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 15:38:54.93 +66:17:18.3: 10.48 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 15:38:54.93 +66:17:18.3: 10.48 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.48 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1644550815955436672,2461335.6793,9.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1644550815955436672 20261022.1793 9.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.24 12:36:37.68 +73:17:54.9
124.40496 43.78728 galactic Dra Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1689945493537486976 | 12:36:37.80 +73:17:54.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F8 1956PMcCO..13a....B AG+73 327 J-Ks=0.317+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:36:37.68 +73:17:54.9: 10.54 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:36:37.68 +73:17:54.9: 10.49 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.51 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1689945493537486976,2461335.6793,9.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1689945493537486976 20261022.1793 9.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.26 12:41:58.81 +73:10:55.9
123.88156 43.92861 galactic Dra Second-epoch detections are separated by 0.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689891823626099968 | 12:41:58.89 +73:10:55.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.234+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:41:58.81 +73:10:55.9: 10.52 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:41:58.81 +73:10:55.9: 10.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.51 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689891823626099968,2461335.6793,9.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689891823626099968 20261022.1793 9.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.38 13:18:56.85 +72:31:43.8
120.04549 44.44492 galactic UMi Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687963860050390400 | 13:18:56.77 +72:31:44.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K: 1956PMcCO..13a....B AG+72 349 J-Ks=0.798+/-0.032 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:56.85 +72:31:43.8: 10.44 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:56.85 +72:31:43.8: 10.46 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.45 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687963860050390400,2461335.6793,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687963860050390400 20261022.1793 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.28 12:51:43.52 +72:36:44.3
122.90181 44.51593 galactic Dra Second-epoch detections are separated by 0.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689663262646917248 | 12:51:43.71 +72:36:44.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.643+/-0.027 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:51:43.52 +72:36:44.3: 10.41 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:51:43.52 +72:36:44.3: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.41 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689663262646917248,2461335.6793,9.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689663262646917248 20261022.1793 9.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.26 12:46:24.81 +72:54:36.6
123.44689 44.21306 galactic Dra Second-epoch detections are separated by 0.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689685317302865152 | 12:46:24.95 +72:54:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1956PMcCO..13a....B AG+73 332 J-Ks=0.350+/-0.028 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:46:24.81 +72:54:36.6: 10.40 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:46:24.81 +72:54:36.6: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.40 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689685317302865152,2461335.6793,9.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689685317302865152 20261022.1793 9.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.23 13:09:41.33 +72:26:38.9
121.00017 44.61559 galactic UMi Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688062442435567488 | 13:09:41.33 +72:26:38.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.599+/-0.039 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:09:41.33 +72:26:38.9: 10.38 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:09:41.33 +72:26:38.9: 10.37 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.37 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688062442435567488,2461335.6793,9.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688062442435567488 20261022.1793 9.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.47 13:09:52.90 +73:14:32.3
121.09102 43.81996 galactic UMi Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688253413861607296 | 13:09:52.89 +73:14:32.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.661+/-0.047 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:09:52.90 +73:14:32.3: 10.39 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:09:52.90 +73:14:32.3: 10.38 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.39 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688253413861607296,2461335.6793,9.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688253413861607296 20261022.1793 9.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.24 12:41:01.06 +73:24:48.5
123.96012 43.69397 galactic Dra Second-epoch detections are separated by 0.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689904124412454784 | 12:41:01.36 +73:24:48.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:41:01.06 +73:24:48.5: 10.42 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:41:01.06 +73:24:48.5: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.41 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689904124412454784,2461335.6793,9.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689904124412454784 20261022.1793 9.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.78 13:34:15.49 +72:07:44.6
118.33884 44.61534 galactic UMi Second-epoch detections are separated by 2.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:34:15.49 +72:07:44.6 (user input) | T | P | (position from user input) J-Ks=0.685+/-0.034 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:34:15.49 +72:07:44.6: 13.64 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:34:15.49 +72:07:44.6: 13.67 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.54 13:11:46.15 +72:34:35.4
120.80158 44.46756 galactic UMi Second-epoch detections are separated by 3.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:11:46.15 +72:34:35.4 (user input) | T | P | (position from user input) J-Ks=0.355+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:11:46.15 +72:34:35.4: 13.61 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:11:46.15 +72:34:35.4: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.14 12:48:40.12 +73:32:19.5
123.20276 43.58804 galactic Dra Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691230960069585664 | 12:48:40.14 +73:32:19.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956PMcCO..13a....B AG+73 334 J-Ks=0.311+/-0.031 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:48:40.12 +73:32:19.5: 10.28 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:48:40.12 +73:32:19.5: 10.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.27 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691230960069585664,2461335.6793,9.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691230960069585664 20261022.1793 9.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.61 12:50:59.23 +72:44:33.4
122.97870 44.38560 galactic Dra Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:50:59.23 +72:44:33.4 (user input) | T | P | (position from user input) J-Ks=0.356+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:50:59.23 +72:44:33.4: 13.63 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:50:59.23 +72:44:33.4: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.23 13:17:46.16 +71:43:15.4
120.00399 45.25731 galactic UMi Second-epoch detections are separated by 0.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687807458817203584 | 13:17:46.23 +71:43:15.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956PMcCO..13a....B AG+71 385 J-Ks=0.284+/-0.029 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:17:46.16 +71:43:15.4: 10.24 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:17:46.16 +71:43:15.4: 10.24 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.24 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687807458817203584,2461335.6793,9.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687807458817203584 20261022.1793 9.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.06 12:36:31.04 +73:19:07.8
124.41369 43.76646 galactic Dra Second-epoch detections are separated by 0.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689946627408854528 | 12:36:31.17 +73:19:07.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 wl 1956PMcCO..13a....B AG+73 326 J-Ks=8.661+/- (unrealisitic color!)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:36:31.04 +73:19:07.8: 10.31 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:36:31.04 +73:19:07.8: 10.25 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.28 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689946627408854528,2461335.6793,9.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689946627408854528 20261022.1793 9.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.79 13:30:29.24 +72:00:25.8
118.69884 44.79874 galactic UMi Second-epoch detections are separated by 3.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:30:29.24 +72:00:25.8 (user input) | T | P | (position from user input) J-Ks=0.397+/-0.049 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:30:29.24 +72:00:25.8: 13.64 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:30:29.24 +72:00:25.8: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.20 13:27:29.93 +71:42:32.6
118.93420 45.13824 galactic UMi Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1687115934722858240 | 13:27:29.90 +71:42:32.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.280+/-0.026 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:27:29.93 +71:42:32.6: 10.22 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:27:29.93 +71:42:32.6: 10.20 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.21 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1687115934722858240,2461335.6793,9.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1687115934722858240 20261022.1793 9.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 9.12 13:02:55.03 +72:18:40.8
121.70368 44.78953 galactic Dra Second-epoch detections are separated by 0.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688094396992318464 | 13:02:54.97 +72:18:40.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1926MeUpp..11....1L BD+73 580 J-Ks=0.194+/-0.028 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:02:55.03 +72:18:40.8: 10.18 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:02:55.03 +72:18:40.8: 10.19 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.19 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688094396992318464,2461335.6793,9.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688094396992318464 20261022.1793 9.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.54 13:16:34.92 +72:40:37.4
120.31997 44.32345 galactic UMi Second-epoch detections are separated by 1.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:16:34.92 +72:40:37.4 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:16:34.92 +72:40:37.4: 13.62 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:16:34.92 +72:40:37.4: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.73 13:10:07.70 +71:50:50.2
120.86757 45.20598 galactic UMi Second-epoch detections are separated by 2.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:10:07.70 +71:50:50.2 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.031 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:10:07.70 +71:50:50.2: 13.62 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:10:07.70 +71:50:50.2: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 8.92 12:58:07.13 +72:57:47.8
122.24992 44.15613 galactic Dra Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1691154475291341824 | 12:58:07.08 +72:57:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1956PMcCO..13a....B AG+73 340 J-Ks=0.633+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:58:07.13 +72:57:47.8: 9.93 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:58:07.13 +72:57:47.8: 9.95 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.94 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1691154475291341824,2461335.6793,8.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1691154475291341824 20261022.1793 8.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.55 13:23:59.13 +71:50:27.0
119.35151 45.06047 galactic UMi Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:23:59.13 +71:50:27.0 (user input) | T | P | (position from user input) J-Ks=0.395+/-0.029 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:59.13 +71:50:27.0: 13.59 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:59.13 +71:50:27.0: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 8.86 12:47:42.19 +73:04:40.0
123.31002 44.04773 galactic Dra Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1689693911533146496 | 12:47:42.11 +73:04:40.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: K2 1956PMcCO..13a....B AG+73 333 J-Ks=0.619+/-0.040 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:47:42.19 +73:04:40.0: 9.90 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:47:42.19 +73:04:40.0: 9.91 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.91 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1689693911533146496,2461335.6793,8.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1689693911533146496 20261022.1793 8.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.60 13:01:08.37 +72:19:37.4
121.89482 44.78165 galactic Dra Second-epoch detections are separated by 1.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:01:08.37 +72:19:37.4 (user input) | T | P | (position from user input) J-Ks=0.406+/-0.030 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:01:08.37 +72:19:37.4: 13.60 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:01:08.37 +72:19:37.4: 13.60 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.54 12:54:52.75 +72:45:42.9
122.57532 44.36395 galactic Dra Second-epoch detections are separated by 0.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:54:52.75 +72:45:42.9 (user input) | T | P | (position from user input) J-Ks=0.448+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:54:52.75 +72:45:42.9: 13.59 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:54:52.75 +72:45:42.9: 13.62 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 8.71 13:04:25.11 +72:51:34.8
121.59768 44.23494 galactic UMi Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1688139030292411776 | 13:04:25.14 +72:51:35.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.760+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:04:25.11 +72:51:34.8: 9.63 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:04:25.11 +72:51:34.8: 9.64 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.63 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688139030292411776,2461335.6793,8.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688139030292411776 20261022.1793 8.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 8.66 12:41:58.30 +72:57:48.6
123.89797 44.14699 galactic Dra Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1689864610713296896 | 12:41:59.07 +72:57:49.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2V 1950ApJ...111..221W BD+73 566
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:41:58.30 +72:57:48.6: 9.61 +/- 0.00 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:41:58.30 +72:57:48.6: 9.60 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.61 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1689864610713296896,2461335.6793,8.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1689864610713296896 20261022.1793 8.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.61 13:11:09.70 +72:48:43.1
120.90016 44.23839 galactic UMi Second-epoch detections are separated by 4.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:11:09.70 +72:48:43.1 (user input) | T | P | (position from user input) J-Ks=0.636+/-0.036 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:11:09.70 +72:48:43.1: 13.58 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:11:09.70 +72:48:43.1: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.76 13:18:01.59 +72:23:16.1
120.11270 44.59461 galactic UMi Second-epoch detections are separated by 1.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:18:01.59 +72:23:16.1 (user input) | T | P | (position from user input) J-Ks=0.306+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:01.59 +72:23:16.1: 13.57 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:01.59 +72:23:16.1: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.62 13:32:43.17 +71:44:41.0
118.37850 45.01677 galactic UMi Second-epoch detections are separated by 2.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1687127342155960448 | 13:32:43.17 +71:44:41.0 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.468+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:32:43.17 +71:44:41.0: 13.57 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:32:43.17 +71:44:41.0: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1687127342155960448,2461335.6793,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 1687127342155960448 20261022.1793 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.46 13:11:25.29 +72:08:18.4
120.77066 44.90585 galactic UMi Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:11:25.29 +72:08:18.4 (user input) | T | P | (position from user input) J-Ks=0.570+/-0.031 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:11:25.29 +72:08:18.4: 13.58 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:11:25.29 +72:08:18.4: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.73 13:18:23.28 +72:39:40.8
120.13076 44.32005 galactic UMi Second-epoch detections are separated by 2.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:18:23.28 +72:39:40.8 (user input) | T | P | (position from user input) J-Ks=0.329+/-0.034 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:18:23.28 +72:39:40.8: 13.56 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:18:23.28 +72:39:40.8: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.54 13:10:21.80 +72:48:47.9
120.98222 44.24323 galactic UMi Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:10:21.80 +72:48:47.9 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.032 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:10:21.80 +72:48:47.9: 13.57 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:10:21.80 +72:48:47.9: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.63 13:11:49.43 +72:19:25.6
120.75648 44.71826 galactic UMi Second-epoch detections are separated by 2.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:11:49.43 +72:19:25.6 (user input) | T | P | (position from user input) J-Ks=0.315+/-0.033 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:11:49.43 +72:19:25.6: 13.54 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:11:49.43 +72:19:25.6: 13.61 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 10.98 12:48:57.79 +72:53:58.7
123.18579 44.22739 galactic Dra Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:48:57.79 +72:53:58.7 (user input) | T | P | (position from user input) J-Ks=0.593+/-0.029 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:48:57.79 +72:53:58.7: 13.10 +/- 0.03 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:48:57.79 +72:53:58.7: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.38 12:54:54.16 +72:37:19.8
122.56919 44.50364 galactic Dra Second-epoch detections are separated by 0.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 12:54:54.16 +72:37:19.8 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.033 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 12:54:54.16 +72:37:19.8: 13.56 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 12:54:54.16 +72:37:19.8: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.42 13:03:42.54 +72:51:11.4
121.66987 44.24500 galactic Dra Second-epoch detections are separated by 0.4" and 7.3 pix
The object was found in VSX 1" Gaia DR3 1688138824134022784
Type: ROT
# Max. Min./Amp. JD0 Period
13.160 G 13.190 G G
The object was not found in astcheck.
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:03:42.54 +72:51:11.4: 13.55 +/- 0.05 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:03:42.54 +72:51:11.4: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1688138824134022784,2461335.6793,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1688138824134022784 20261022.1793 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.74 13:23:15.12 +72:02:51.7
119.48205 44.86684 galactic UMi Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:23:15.12 +72:02:51.7 (user input) | T | P | (position from user input) J-Ks=0.306+/-0.035 (F)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:23:15.12 +72:02:51.7: 13.59 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:23:15.12 +72:02:51.7: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.68 13:28:48.74 +71:58:22.8
118.86736 44.85912 galactic UMi Second-epoch detections are separated by 1.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:28:48.74 +71:58:22.8 (user input) | T | P | (position from user input) J-Ks=0.356+/-0.035 (G)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:28:48.74 +71:58:22.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:28:48.74 +71:58:22.8: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 22.1793 2461335.6793 11.55 13:19:28.26 +71:37:18.8
119.79487 45.33522 galactic UMi Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 13:19:28.26 +71:37:18.8 (user input) | T | P | (position from user input) J-Ks=0.563+/-0.028 (K)
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits at 13:19:28.26 +71:37:18.8: 13.53 +/- 0.04 detection
Forced photometry on wcs_UMi-02-Q1b1x1_2026-04-19_03-49-38_20.00sec_-4.90C_LIGHT_0660.fits at 13:19:28.26 +71:37:18.8: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461335.6793,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20261022.1793 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461149.86733143 19.04.2026 08:48:47.436 /data_ssd/NMW-TexasTech/reference_imgs/UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits
First image: 2461149.86733143 19.04.2026 08:48:47.436 /data_ssd/NMW-TexasTech/reference_imgs/UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits
Last image: 2461335.67955111 22.10.2026 04:18:23.216 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_UMi-02-Q1b1x1_231918_TTUQ1b1x1_1257846_KU7UCfPg/fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7505
Objects passed selection criteria: 7438
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 4092.25
Average stars matched: 4001 (97.7702 %)
Memory usage VmPeak: 233808 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 21 23:20:34 CDT 2026
Host name: tau
############################################################
ERROR: large change in astrometric-star counts between the two new images (q3: 40 -> 54, 25.926% > 20%; fd_UMi-02-Q1b1x1_2026-10-21_23-17-32_20.00sec_0.00C_LIGHTs_0145.fits vs fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461149.86733143 19.04.2026 08:48:47.436 /data_ssd/NMW-TexasTech/reference_imgs/UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits
First image: 2461149.86733143 19.04.2026 08:48:47.436 /data_ssd/NMW-TexasTech/reference_imgs/UMi-02-Q1b1x1_2026-04-19_03-48-47_20.00sec_-4.90C_LIGHT_0659.fits
Last image: 2461335.67955111 22.10.2026 04:18:23.216 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_UMi-02-Q1b1x1_231918_TTUQ1b1x1_1257846_KU7UCfPg/fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 675
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.07
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 38233
Objects passed selection criteria: 38053
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 22264
Average stars matched: 21479.8 (96.4775 %)
Memory usage VmPeak: 261568 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 21 23:21:26 CDT 2026
Host name: tau
############################################################
**** FOUND 13:32:31.59 +72:01:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52986_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
The candidate 52986_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146 did not pass the final checks
**** FOUND 13:13:31.46 +72:46:42.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 10530_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10530_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13529_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13529_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08918_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08918_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10474_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10474_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11632_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11632_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10951_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10951_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07594_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07594_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12960_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12960_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09998_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09998_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 33765_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 33765_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15785_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15785_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11090_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11090_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14131_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14131_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15301_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15301_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11149_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11149_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12234_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12234_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10184_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10184_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13932_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13932_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13510_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13510_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 17448_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 17448_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11712_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11712_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15078_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15078_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13148_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13148_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 34167_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 34167_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15521_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15521_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11756_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11756_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16224_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16224_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 18791_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 18791_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07945_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07945_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07932_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
The candidate 07932_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146 did not pass the final checks
**** FOUND 13:23:23.82 +72:39:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33452_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 33452_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15589_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15589_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15748_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15748_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12736_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12736_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16512_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16512_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12317_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12317_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10036_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10036_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14116_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14116_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14071_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14071_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15223_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15223_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01662_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01662_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09735_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09735_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15683_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15683_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03139_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03139_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10185_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10185_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04871_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04871_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12639_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12639_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13834_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
The candidate 13834_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146 did not pass the final checks
**** FOUND 13:37:37.56 +71:27:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10471_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10471_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04438_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04438_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05090_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05090_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04424_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04424_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05077_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05077_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03405_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03405_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06862_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06862_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07823_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07823_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06506_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06506_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04047_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04047_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03268_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03268_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05166_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05166_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06168_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06168_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12164_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12164_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12658_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12658_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10368_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10368_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02672_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02672_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06599_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06599_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05559_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05559_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11700_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11700_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10915_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10915_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04722_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04722_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04657_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04657_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10669_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10669_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07576_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07576_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08031_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08031_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06335_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06335_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12422_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12422_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09183_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09183_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03341_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03341_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01655_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01655_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08494_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08494_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14996_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14996_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13548_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13548_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02543_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02543_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13219_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13219_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09531_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09531_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07859_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07859_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12815_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12815_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14192_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14192_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12568_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12568_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11863_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11863_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04690_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04690_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08916_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08916_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02748_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02748_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09399_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09399_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01431_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01431_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11191_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11191_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10673_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10673_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07186_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07186_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10672_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10672_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09560_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09560_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09167_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09167_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02414_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02414_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12393_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12393_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10314_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10314_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04541_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04541_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08735_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08735_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09762_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09762_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05167_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05167_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14534_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14534_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06427_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06427_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12394_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12394_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09967_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09967_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08353_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08353_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05379_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05379_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01818_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01818_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09010_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09010_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03292_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03292_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11262_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11262_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07596_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07596_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07386_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07386_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11526_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11526_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 50236_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 50236_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02247_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02247_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10284_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10284_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01336_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01336_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01224_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01224_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11162_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11162_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07901_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07901_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08124_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08124_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03316_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03316_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05677_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05677_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04292_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04292_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12900_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12900_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06900_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06900_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12883_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12883_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11658_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11658_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13205_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13205_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05736_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05736_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11943_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11943_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10031_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10031_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02725_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02725_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08388_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08388_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07412_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07412_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05995_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05995_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05473_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05473_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07716_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07716_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04299_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04299_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10817_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10817_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10836_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10836_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03166_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03166_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06133_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06133_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 34587_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 34587_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09009_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09009_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15243_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15243_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05406_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05406_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02537_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02537_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07711_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07711_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11757_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11757_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07987_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07987_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06985_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06985_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13617_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13617_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04353_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04353_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05472_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05472_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07005_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07005_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06978_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06978_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09318_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09318_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09075_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09075_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08804_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08804_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06559_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06559_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15879_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15879_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05611_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05611_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02931_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02931_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07111_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07111_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08586_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08586_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12901_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12901_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09209_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09209_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14305_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14305_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14920_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14920_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02189_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02189_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02805_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02805_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07500_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07500_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12944_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12944_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11125_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11125_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08537_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08537_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09578_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09578_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07335_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07335_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14606_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14606_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02425_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02425_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10807_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10807_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12757_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12757_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02784_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02784_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 34087_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 34087_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03110_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03110_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09561_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09561_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12601_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12601_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04886_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04886_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04366_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04366_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10551_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10551_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05175_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05175_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10285_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10285_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10301_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10301_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16552_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16552_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03388_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03388_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10695_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10695_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12707_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12707_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01483_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01483_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01357_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01357_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04053_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04053_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05797_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05797_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02385_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02385_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08712_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08712_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11096_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11096_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14017_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14017_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05144_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05144_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11913_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11913_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10624_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10624_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09051_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09051_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01593_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01593_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07178_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07178_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01565_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01565_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 18157_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 18157_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01111_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01111_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14428_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14428_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06152_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06152_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 36889_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 36889_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02721_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02721_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06669_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06669_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13304_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13304_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09579_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09579_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10758_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10758_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01810_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01810_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08565_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08565_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08908_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08908_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06160_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06160_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08341_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08341_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06471_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06471_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15315_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15315_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03497_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03497_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08830_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08830_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11635_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11635_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06786_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06786_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03052_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03052_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08711_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08711_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13019_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13019_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07877_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07877_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16529_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16529_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16102_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16102_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08250_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08250_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14526_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14526_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07798_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07798_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12370_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12370_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06045_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06045_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04786_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04786_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14513_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14513_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10576_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10576_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15439_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15439_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05664_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05664_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02506_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02506_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12764_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12764_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05584_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05584_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04479_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04479_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01938_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01938_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11563_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11563_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14238_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14238_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13076_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13076_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07774_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07774_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12692_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12692_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09757_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09757_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 00958_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 00958_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03937_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03937_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03874_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03874_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 00773_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 00773_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10057_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10057_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07197_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07197_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10773_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10773_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02338_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02338_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02569_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02569_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08859_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08859_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11254_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11254_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 36716_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 36716_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01588_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01588_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 36510_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 36510_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11737_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11737_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08089_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08089_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05453_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05453_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10209_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10209_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10518_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10518_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09280_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09280_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 00827_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 00827_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09918_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09918_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04279_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04279_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04729_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04729_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10469_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10469_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01844_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01844_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02451_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02451_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 36534_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 36534_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13516_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13516_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03340_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03340_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06905_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06905_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11161_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11161_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12646_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12646_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04540_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04540_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12807_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12807_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06840_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06840_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03608_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03608_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05693_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05693_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06017_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06017_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10880_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10880_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15665_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15665_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04392_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04392_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03735_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03735_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06409_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06409_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07804_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07804_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02103_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02103_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12776_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12776_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05319_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05319_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01757_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01757_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10846_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10846_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09503_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09503_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14574_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14574_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07227_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07227_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09656_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09656_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 17042_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 17042_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03678_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03678_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04188_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04188_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01073_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01073_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07193_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07193_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07864_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07864_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02369_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02369_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12806_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12806_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11511_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11511_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15214_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15214_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16573_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16573_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 17610_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 17610_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 33159_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 33159_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08149_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08149_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03420_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03420_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11553_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11553_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10901_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10901_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05368_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05368_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05766_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05766_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12838_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12838_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07743_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07743_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16008_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16008_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01351_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
The candidate 01351_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146 did not pass the final checks
**** FOUND 12:44:38.34 +73:24:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09881_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09881_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06306_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06306_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13222_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13222_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08400_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08400_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12028_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12028_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04578_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04578_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03931_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03931_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13607_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13607_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12448_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12448_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16056_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16056_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08639_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08639_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07132_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07132_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13250_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13250_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08276_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08276_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03175_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03175_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02260_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02260_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10772_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10772_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03859_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03859_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13636_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13636_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08267_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08267_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07198_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07198_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07784_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07784_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05246_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05246_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01318_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01318_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11401_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11401_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11459_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11459_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11484_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11484_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07669_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07669_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 36246_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 36246_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06351_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06351_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16608_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16608_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06293_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06293_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03776_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03776_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 00686_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 00686_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09957_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09957_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04975_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04975_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13314_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13314_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06087_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06087_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05911_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05911_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05767_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05767_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15205_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15205_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15097_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15097_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08509_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08509_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15692_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15692_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06833_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06833_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14728_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14728_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08484_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08484_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10735_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10735_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01812_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01812_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 37998_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 37998_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07127_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07127_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09624_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09624_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01154_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01154_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15199_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15199_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 37548_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 37548_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08041_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08041_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02102_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02102_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06062_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06062_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12825_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12825_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02964_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02964_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13003_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13003_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03556_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03556_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04297_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04297_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12206_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12206_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14814_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14814_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05849_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05849_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12617_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12617_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10223_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10223_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05622_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05622_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04248_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04248_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09657_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09657_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12737_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12737_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02131_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02131_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07546_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07546_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 00930_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 00930_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01510_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01510_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07170_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07170_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07529_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07529_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14508_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14508_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10137_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10137_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 35413_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 35413_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08966_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08966_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03774_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03774_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10046_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10046_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02719_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02719_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 38110_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 38110_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16141_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16141_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03236_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03236_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04277_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04277_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04217_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04217_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06470_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06470_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 35329_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 35329_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 36326_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 36326_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11168_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11168_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09326_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09326_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01626_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01626_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 37989_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 37989_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10349_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10349_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 27801_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 27801_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 38231_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 38231_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12210_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12210_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03149_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03149_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09908_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09908_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01835_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01835_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10835_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10835_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 37260_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 37260_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12888_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12888_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07442_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07442_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02613_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02613_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13232_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13232_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07374_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07374_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09602_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09602_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11733_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11733_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15865_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
The candidate 15865_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146 did not pass the final checks
**** FOUND 13:40:21.66 +71:00:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08710_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08710_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04888_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04888_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03713_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03713_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 27381_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 27381_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09675_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09675_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11921_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11921_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12543_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12543_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04513_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04513_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01679_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01679_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12423_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12423_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06980_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06980_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05068_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05068_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13786_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13786_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05841_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05841_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02412_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02412_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08002_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08002_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07185_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07185_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15192_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15192_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10433_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10433_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01366_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01366_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 34593_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 34593_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09760_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09760_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08063_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08063_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01549_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01549_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08703_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08703_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13261_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13261_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08381_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08381_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01859_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01859_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07915_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07915_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05933_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05933_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16562_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16562_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02746_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02746_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03546_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03546_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11363_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11363_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11457_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11457_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03869_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03869_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 36995_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 36995_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06995_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06995_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08340_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08340_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16952_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16952_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09317_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09317_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05342_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05342_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02070_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02070_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07522_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07522_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02817_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02817_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01391_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01391_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06395_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06395_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01547_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01547_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 34269_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 34269_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12039_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12039_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03683_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03683_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09866_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09866_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13435_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13435_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09499_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09499_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01822_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01822_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03575_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03575_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05096_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05096_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08943_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08943_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11726_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11726_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07574_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07574_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04347_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04347_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05390_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05390_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06878_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06878_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11970_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11970_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06224_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06224_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04703_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
The candidate 04703_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146 did not pass the final checks
**** FOUND 13:04:55.64 +73:02:57.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 14611_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14611_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15886_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15886_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04683_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04683_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 16094_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 16094_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14464_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14464_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04870_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04870_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11657_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11657_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12380_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12380_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09640_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09640_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11301_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11301_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02568_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02568_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06860_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06860_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01241_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01241_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05951_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05951_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 34830_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 34830_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05625_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05625_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08118_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08118_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 35947_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 35947_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10375_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10375_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10090_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10090_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 15977_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 15977_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03966_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03966_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08795_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08795_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02536_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02536_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10593_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10593_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06513_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06513_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08052_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08052_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10815_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10815_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07177_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07177_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10366_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10366_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 14248_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 14248_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05106_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05106_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04583_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04583_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09203_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09203_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06419_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06419_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11066_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11066_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07107_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07107_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10079_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10079_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08248_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08248_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07681_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07681_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08640_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08640_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 00759_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 00759_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03266_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03266_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06219_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06219_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03896_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03896_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 36453_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 36453_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01240_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01240_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05663_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05663_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 36159_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 36159_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08914_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08914_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03519_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03519_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06498_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06498_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11069_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11069_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 13454_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 13454_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 37816_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 37816_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11026_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11026_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 38087_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 38087_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 36834_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 36834_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05100_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05100_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 33684_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 33684_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04443_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04443_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07626_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07626_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08121_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08121_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12669_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12669_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07274_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07274_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06077_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06077_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05737_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05737_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10737_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10737_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02763_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02763_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02428_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02428_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12068_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12068_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08087_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08087_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 36851_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 36851_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 00675_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 00675_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01727_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01727_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07974_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07974_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04922_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04922_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03202_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03202_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07441_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07441_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04416_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04416_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 00803_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 00803_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10893_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10893_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07229_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07229_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 01239_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 01239_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04446_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04446_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11138_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11138_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 00589_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 00589_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11095_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11095_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12015_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12015_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07291_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07291_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07259_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07259_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 09940_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 09940_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04309_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04309_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11261_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11261_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02733_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02733_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07120_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07120_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 04800_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 04800_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05271_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05271_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 02318_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 02318_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06282_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06282_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08559_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08559_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 12341_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 12341_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08932_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08932_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 07461_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 07461_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 06195_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 06195_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 08251_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 08251_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 03607_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 03607_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05326_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05326_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 05419_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 05419_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 10354_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 10354_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11140_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11140_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
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Considering the candidate 11745_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
Preparing report for the candidate 11745_fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146
make_report_in_HTML.sh Phase 2 (HTML assembly): 55s
make_report_in_HTML.sh TOTAL: 1254s
Prepared the HTML report for the field UMi-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
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13:22:58.81 +71:33:49.3
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13:31:21.37 +71:29:17.8
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13:26:01.91 +71:22:30.4
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13:25:49.95 +71:19:29.6
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15:34:39.02 +65:26:07.3
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15:31:51.21 +65:47:40.0
15:36:12.29 +65:44:49.7
15:30:30.75 +65:56:33.3
15:30:26.56 +65:59:47.7
15:26:54.39 +66:13:17.5
15:26:38.72 +66:13:52.6
15:30:36.25 +66:16:20.0
15:27:08.39 +66:24:52.0
15:24:45.65 +66:30:17.5
15:29:40.01 +66:22:09.7
15:28:55.94 +66:26:17.9
15:28:57.10 +66:27:31.1
15:28:35.36 +66:28:09.1
15:27:01.80 +66:33:21.5
15:27:00.65 +66:36:15.0
15:38:54.93 +66:17:18.3
15:28:43.89 +66:32:41.9
15:25:13.93 +66:40:57.3
15:38:50.47 +66:21:18.4
15:26:36.25 +66:47:00.3
15:34:41.44 +66:38:48.3
15:32:04.15 +66:44:42.6
15:34:42.38 +66:40:58.8
15:35:55.99 +66:40:56.0
15:33:52.91 +66:43:08.2
15:33:00.32 +66:46:59.1
13:04:26.86 +72:50:34.0
Source monitoring: NOT measuring the monitored positions on the field UMi-02-Q1b1x1 - the transient search raised a processing error: ERROR: large change in astrometric-star counts between the two new images (q3: 40 -> 54, 25.926% > 20%; fd_UMi-02-Q1b1x1_2026-10-21_23-17-32_20.00sec_0.00C_LIGHTs_0145.fits vs fd_UMi-02-Q1b1x1_2026-10-21_23-18-23_20.00sec_-0.00C_LIGHTs_0146.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
Source monitoring: the monitored positions on the field UMi-02-Q1b1x1 are recorded as run_error (rejected by this run, never measured later)
########### Completed UMi-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
13:21:36.40 +71:58:07.4
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12:54:52.75 +72:45:42.9
13:04:25.11 +72:51:34.8
12:41:58.30 +72:57:48.6
13:11:09.70 +72:48:43.1
13:18:01.59 +72:23:16.1
13:32:43.17 +71:44:41.0
13:11:25.29 +72:08:18.4
13:18:23.28 +72:39:40.8
13:10:21.80 +72:48:47.9
13:11:49.43 +72:19:25.6
12:48:57.79 +72:53:58.7
12:54:54.16 +72:37:19.8
13:03:42.54 +72:51:11.4
13:23:15.12 +72:02:51.7
13:28:48.74 +71:58:22.8
13:19:28.26 +71:37:18.8
###################################################################################
13:21:36.40 +71:58:07.4 -- not an asteroid (will add it to exclusion list)
13:32:08.94 +71:25:13.3 -- not an asteroid (will add it to exclusion list)
13:14:17.41 +72:12:56.4 -- not an asteroid (will add it to exclusion list)
13:19:33.78 +71:55:20.3 -- not an asteroid (will add it to exclusion list)
13:20:10.61 +71:38:59.2 -- not an asteroid (will add it to exclusion list)
13:32:39.82 +72:03:58.1 -- not an asteroid (will add it to exclusion list)
13:13:30.12 +72:30:27.1 -- not an asteroid (will add it to exclusion list)
13:35:06.68 +71:37:16.2 -- not an asteroid (will add it to exclusion list)
13:28:50.89 +72:13:38.2 -- not an asteroid (will add it to exclusion list)
15:37:01.65 +65:32:17.8 -- not an asteroid (will add it to exclusion list)
13:40:12.72 +71:01:57.3 -- not an asteroid (will add it to exclusion list)
13:16:09.04 +71:42:06.3 -- not an asteroid (will add it to exclusion list)
13:39:59.05 +71:25:10.6 -- not an asteroid (will add it to exclusion list)
13:39:22.44 +71:07:42.1 -- not an asteroid (will add it to exclusion list)
13:32:34.71 +72:01:22.6 -- not an asteroid (will add it to exclusion list)
13:19:56.41 +71:30:15.9 -- not an asteroid (will add it to exclusion list)
13:35:24.95 +72:17:30.1 -- not an asteroid (will add it to exclusion list)
13:35:29.66 +71:23:40.1 -- not an asteroid (will add it to exclusion list)
13:28:43.51 +71:22:13.7 -- not an asteroid (will add it to exclusion list)
13:34:39.39 +70:31:39.6 -- not an asteroid (will add it to exclusion list)
13:36:35.78 +71:56:58.8 -- not an asteroid (will add it to exclusion list)
13:25:33.26 +70:55:51.6 -- not an asteroid (will add it to exclusion list)
13:34:40.95 +71:34:31.7 -- not an asteroid (will add it to exclusion list)
15:34:06.07 +65:42:32.3 -- not an asteroid (will add it to exclusion list)
13:32:41.35 +70:58:12.1 -- not an asteroid (will add it to exclusion list)
13:27:33.94 +71:46:45.9 -- not an asteroid (will add it to exclusion list)
13:25:31.63 +70:40:09.0 -- not an asteroid (will add it to exclusion list)
13:39:16.57 +70:16:48.5 -- not an asteroid (will add it to exclusion list)
13:23:20.53 +72:39:07.6 -- not an asteroid (will add it to exclusion list)
15:36:58.16 +65:28:47.1 -- not an asteroid (will add it to exclusion list)
13:38:08.95 +71:03:09.2 -- not an asteroid (will add it to exclusion list)
13:38:35.67 +71:01:20.0 -- not an asteroid (will add it to exclusion list)
13:28:02.22 +71:33:15.8 -- not an asteroid (will add it to exclusion list)
13:28:23.57 +70:39:09.1 -- not an asteroid (will add it to exclusion list)
13:22:58.81 +71:33:49.3 -- not an asteroid (will add it to exclusion list)
13:29:09.79 +72:14:06.7 -- not an asteroid (will add it to exclusion list)
13:37:40.30 +71:23:59.4 -- not an asteroid (will add it to exclusion list)
13:36:41.40 +71:23:59.0 -- not an asteroid (will add it to exclusion list)
13:35:24.47 +71:05:40.9 -- not an asteroid (will add it to exclusion list)
12:51:17.47 +73:31:33.0 -- not an asteroid (will add it to exclusion list)
13:15:56.81 +72:02:25.8 -- not an asteroid (will add it to exclusion list)
13:41:41.88 +71:05:34.0 -- not an asteroid (will add it to exclusion list)
12:47:50.85 +72:59:34.6 -- not an asteroid (will add it to exclusion list)
13:16:27.07 +71:56:08.2 -- not an asteroid (will add it to exclusion list)
12:50:18.37 +72:36:12.5 -- not an asteroid (will add it to exclusion list)
13:21:30.41 +71:27:07.9 -- not an asteroid (will add it to exclusion list)
13:13:50.51 +71:48:33.2 -- not an asteroid (will add it to exclusion list)
12:58:42.59 +72:58:36.9 -- not an asteroid (will add it to exclusion list)
13:00:01.80 +72:50:19.0 -- not an asteroid (will add it to exclusion list)
12:51:25.91 +72:45:38.4 -- not an asteroid (will add it to exclusion list)
13:03:40.05 +72:56:33.0 -- not an asteroid (will add it to exclusion list)
13:01:23.83 +73:19:03.4 -- not an asteroid (will add it to exclusion list)
13:13:32.47 +72:42:16.1 -- not an asteroid (will add it to exclusion list)
13:05:33.68 +72:16:21.0 -- not an asteroid (will add it to exclusion list)
13:07:25.77 +72:39:06.8 -- not an asteroid (will add it to exclusion list)
13:04:26.17 +73:14:02.6 -- not an asteroid (will add it to exclusion list)
12:48:47.38 +72:59:37.4 -- not an asteroid (will add it to exclusion list)
12:56:27.99 +72:42:58.8 -- not an asteroid (will add it to exclusion list)
13:07:20.98 +72:44:49.8 -- not an asteroid (will add it to exclusion list)
13:21:59.20 +71:34:54.7 -- not an asteroid (will add it to exclusion list)
13:24:16.16 +71:30:22.0 -- not an asteroid (will add it to exclusion list)
13:10:44.22 +71:45:25.8 -- not an asteroid (will add it to exclusion list)
12:57:25.78 +73:24:36.7 -- not an asteroid (will add it to exclusion list)
13:08:33.28 +72:39:18.9 -- not an asteroid (will add it to exclusion list)
13:07:33.55 +72:54:30.0 -- not an asteroid (will add it to exclusion list)
13:14:10.93 +71:30:50.6 -- not an asteroid (will add it to exclusion list)
13:24:01.15 +71:55:46.8 -- not an asteroid (will add it to exclusion list)
12:55:04.45 +72:47:32.2 -- not an asteroid (will add it to exclusion list)
13:00:49.89 +72:58:31.6 -- not an asteroid (will add it to exclusion list)
13:26:30.90 +72:01:59.4 -- not an asteroid (will add it to exclusion list)
13:06:08.59 +72:20:50.3 -- not an asteroid (will add it to exclusion list)
13:18:15.77 +72:31:25.4 -- not an asteroid (will add it to exclusion list)
13:06:42.04 +72:40:56.5 -- not an asteroid (will add it to exclusion list)
13:23:54.43 +71:33:11.7 -- not an asteroid (will add it to exclusion list)
13:15:46.85 +72:10:09.7 -- not an asteroid (will add it to exclusion list)
12:57:44.81 +73:14:08.2 -- not an asteroid (will add it to exclusion list)
12:44:20.10 +73:18:22.2 -- not an asteroid (will add it to exclusion list)
13:08:31.68 +72:09:36.8 -- not an asteroid (will add it to exclusion list)
13:32:42.39 +71:06:13.9 -- not an asteroid (will add it to exclusion list)
13:32:16.86 +71:26:19.0 -- not an asteroid (will add it to exclusion list)
12:48:18.74 +73:10:12.2 -- not an asteroid (will add it to exclusion list)
13:34:15.26 +71:33:17.2 -- not an asteroid (will add it to exclusion list)
13:24:02.37 +72:15:55.0 -- not an asteroid (will add it to exclusion list)
13:05:42.21 +72:16:06.7 -- not an asteroid (will add it to exclusion list)
13:36:16.68 +71:41:24.7 -- not an asteroid (will add it to exclusion list)
13:20:55.33 +71:03:56.8 -- not an asteroid (will add it to exclusion list)
13:29:32.39 +71:37:49.6 -- not an asteroid (will add it to exclusion list)
13:37:44.01 +71:56:18.1 -- not an asteroid (will add it to exclusion list)
12:54:20.09 +72:46:51.1 -- not an asteroid (will add it to exclusion list)
13:13:17.73 +72:11:14.5 -- not an asteroid (will add it to exclusion list)
12:50:31.15 +73:11:01.3 -- not an asteroid (will add it to exclusion list)
13:15:47.45 +72:07:13.3 -- not an asteroid (will add it to exclusion list)
12:40:05.33 +73:13:28.7 -- not an asteroid (will add it to exclusion list)
13:20:46.11 +71:47:47.1 -- not an asteroid (will add it to exclusion list)
13:09:22.55 +71:38:50.5 -- not an asteroid (will add it to exclusion list)
13:01:03.11 +72:18:20.9 -- not an asteroid (will add it to exclusion list)
13:15:15.15 +71:47:14.5 -- not an asteroid (will add it to exclusion list)
13:11:11.35 +71:58:03.5 -- not an asteroid (will add it to exclusion list)
13:21:19.87 +72:18:09.9 -- not an asteroid (will add it to exclusion list)
12:55:17.14 +73:24:59.2 -- not an asteroid (will add it to exclusion list)
13:21:16.99 +71:30:26.7 -- not an asteroid (will add it to exclusion list)
13:10:52.40 +71:46:07.1 -- not an asteroid (will add it to exclusion list)
13:07:29.03 +73:10:26.5 -- not an asteroid (will add it to exclusion list)
13:17:40.41 +72:20:00.1 -- not an asteroid (will add it to exclusion list)
13:16:59.46 +72:03:29.2 -- not an asteroid (will add it to exclusion list)
12:58:30.58 +72:46:28.4 -- not an asteroid (will add it to exclusion list)
13:36:15.70 +71:16:33.1 -- not an asteroid (will add it to exclusion list)
13:16:11.35 +72:52:41.5 -- not an asteroid (will add it to exclusion list)
13:24:46.70 +71:35:06.3 -- not an asteroid (will add it to exclusion list)
13:21:23.84 +72:06:14.9 -- not an asteroid (will add it to exclusion list)
13:22:55.68 +72:32:11.9 -- not an asteroid (will add it to exclusion list)
12:59:27.31 +72:44:42.9 -- not an asteroid (will add it to exclusion list)
12:57:30.88 +73:39:04.8 -- not an asteroid (will add it to exclusion list)
13:04:18.31 +71:56:04.9 -- not an asteroid (will add it to exclusion list)
12:41:38.63 +72:44:23.5 -- not an asteroid (will add it to exclusion list)
13:28:20.72 +71:55:35.1 -- not an asteroid (will add it to exclusion list)
13:07:18.75 +72:22:07.7 -- not an asteroid (will add it to exclusion list)
13:14:20.50 +72:35:29.9 -- not an asteroid (will add it to exclusion list)
13:21:39.25 +71:43:36.0 -- not an asteroid (will add it to exclusion list)
13:04:26.86 +72:50:34.0 -- not an asteroid (will add it to exclusion list)
12:47:02.63 +73:12:57.3 -- not an asteroid (will add it to exclusion list)
13:27:41.73 +72:08:56.9 -- not an asteroid (will add it to exclusion list)
12:43:48.66 +73:22:47.2 -- not an asteroid (will add it to exclusion list)
12:50:10.58 +73:36:21.6 -- not an asteroid (will add it to exclusion list)
13:21:14.53 +71:48:45.1 -- not an asteroid (will add it to exclusion list)
13:12:39.08 +72:25:47.2 -- not an asteroid (will add it to exclusion list)
13:12:16.25 +72:21:42.9 -- not an asteroid (will add it to exclusion list)
12:54:54.68 +73:09:36.4 -- not an asteroid (will add it to exclusion list)
13:12:34.95 +72:59:46.7 -- not an asteroid (will add it to exclusion list)
12:52:55.29 +72:50:35.1 -- not an asteroid (will add it to exclusion list)
13:26:50.22 +71:29:45.5 -- not an asteroid (will add it to exclusion list)
13:06:03.28 +72:30:52.9 -- not an asteroid (will add it to exclusion list)
13:34:11.36 +71:38:15.8 -- not an asteroid (will add it to exclusion list)
13:21:39.33 +71:41:36.8 -- not an asteroid (will add it to exclusion list)
13:23:26.11 +71:20:57.7 -- not an asteroid (will add it to exclusion list)
13:00:41.05 +72:40:50.2 -- not an asteroid (will add it to exclusion list)
13:28:32.68 +71:45:48.2 -- not an asteroid (will add it to exclusion list)
13:16:26.32 +71:58:12.7 -- not an asteroid (will add it to exclusion list)
12:41:39.35 +72:54:10.6 -- not an asteroid (will add it to exclusion list)
13:06:30.73 +72:08:40.3 -- not an asteroid (will add it to exclusion list)
13:08:06.85 +72:26:10.3 -- not an asteroid (will add it to exclusion list)
13:13:03.94 +72:55:30.5 -- not an asteroid (will add it to exclusion list)
12:58:03.43 +72:40:46.8 -- not an asteroid (will add it to exclusion list)
13:15:16.78 +72:31:47.3 -- not an asteroid (will add it to exclusion list)
13:01:49.98 +73:05:38.2 -- not an asteroid (will add it to exclusion list)
13:18:02.85 +71:49:01.7 -- not an asteroid (will add it to exclusion list)
13:32:15.12 +72:06:01.5 -- not an asteroid (will add it to exclusion list)
13:04:41.75 +73:27:59.1 -- not an asteroid (will add it to exclusion list)
13:01:01.23 +72:35:09.9 -- not an asteroid (will add it to exclusion list)
15:36:12.29 +65:44:49.7 -- not an asteroid (will add it to exclusion list)
13:15:22.65 +72:12:29.8 -- not an asteroid (will add it to exclusion list)
13:25:41.60 +70:54:24.1 -- not an asteroid (will add it to exclusion list)
12:55:10.52 +72:36:54.7 -- not an asteroid (will add it to exclusion list)
12:58:33.33 +73:28:20.1 -- not an asteroid (will add it to exclusion list)
13:20:38.91 +72:39:08.2 -- not an asteroid (will add it to exclusion list)
13:19:51.40 +71:37:45.7 -- not an asteroid (will add it to exclusion list)
13:20:15.71 +72:34:31.1 -- not an asteroid (will add it to exclusion list)
13:20:46.24 +72:50:03.0 -- not an asteroid (will add it to exclusion list)
13:23:33.99 +71:14:51.7 -- not an asteroid (will add it to exclusion list)
13:02:01.31 +73:04:44.8 -- not an asteroid (will add it to exclusion list)
12:57:13.79 +72:39:06.6 -- not an asteroid (will add it to exclusion list)
12:58:19.98 +72:16:20.8 -- not an asteroid (will add it to exclusion list)
13:14:32.87 +72:41:53.3 -- not an asteroid (will add it to exclusion list)
13:21:29.70 +72:15:42.4 -- not an asteroid (will add it to exclusion list)
13:23:03.77 +72:21:31.9 -- not an asteroid (will add it to exclusion list)
13:16:37.10 +72:17:29.9 -- not an asteroid (will add it to exclusion list)
12:58:02.55 +72:22:52.0 -- not an asteroid (will add it to exclusion list)
13:35:04.47 +70:56:11.1 -- not an asteroid (will add it to exclusion list)
13:00:16.10 +72:41:56.2 -- not an asteroid (will add it to exclusion list)
13:04:04.51 +73:30:49.2 -- not an asteroid (will add it to exclusion list)
13:08:37.09 +72:31:21.5 -- not an asteroid (will add it to exclusion list)
13:22:50.13 +72:28:43.5 -- not an asteroid (will add it to exclusion list)
13:23:26.14 +71:25:54.5 -- not an asteroid (will add it to exclusion list)
13:28:54.98 +72:25:59.5 -- not an asteroid (will add it to exclusion list)
13:22:57.92 +71:04:38.9 -- not an asteroid (will add it to exclusion list)
13:24:12.23 +70:57:15.2 -- not an asteroid (will add it to exclusion list)
13:00:06.20 +73:36:25.2 -- not an asteroid (will add it to exclusion list)
12:49:44.61 +73:08:59.7 -- not an asteroid (will add it to exclusion list)
13:16:54.28 +72:37:21.5 -- not an asteroid (will add it to exclusion list)
13:25:00.45 +71:26:31.6 -- not an asteroid (will add it to exclusion list)
13:26:39.43 +71:55:52.2 -- not an asteroid (will add it to exclusion list)
13:05:55.27 +72:05:29.6 -- not an asteroid (will add it to exclusion list)
13:17:31.63 +72:07:02.2 -- not an asteroid (will add it to exclusion list)
13:06:34.93 +72:25:03.3 -- not an asteroid (will add it to exclusion list)
13:29:23.30 +71:07:50.6 -- not an asteroid (will add it to exclusion list)
12:49:19.10 +73:14:08.8 -- not an asteroid (will add it to exclusion list)
13:29:10.08 +72:02:46.5 -- not an asteroid (will add it to exclusion list)
13:28:38.58 +71:33:53.7 -- not an asteroid (will add it to exclusion list)
13:00:02.15 +73:26:50.1 -- not an asteroid (will add it to exclusion list)
15:34:52.40 +65:39:51.3 -- not an asteroid (will add it to exclusion list)
12:51:40.12 +73:07:19.8 -- not an asteroid (will add it to exclusion list)
13:24:51.51 +72:16:27.4 -- not an asteroid (will add it to exclusion list)
13:39:02.21 +71:46:34.8 -- not an asteroid (will add it to exclusion list)
12:49:02.47 +72:33:11.0 -- not an asteroid (will add it to exclusion list)
13:09:59.18 +73:16:31.0 -- not an asteroid (will add it to exclusion list)
13:29:14.34 +72:06:34.7 -- not an asteroid (will add it to exclusion list)
12:56:55.90 +72:43:26.2 -- not an asteroid (will add it to exclusion list)
13:30:18.59 +72:11:50.2 -- not an asteroid (will add it to exclusion list)
13:27:04.28 +72:07:49.8 -- not an asteroid (will add it to exclusion list)
13:44:18.84 +70:54:55.5 -- not an asteroid (will add it to exclusion list)
12:53:47.77 +73:06:29.5 -- not an asteroid (will add it to exclusion list)
13:18:32.27 +71:51:10.9 -- not an asteroid (will add it to exclusion list)
13:25:07.60 +71:30:29.7 -- not an asteroid (will add it to exclusion list)
12:53:37.32 +73:38:13.3 -- not an asteroid (will add it to exclusion list)
12:46:02.58 +73:26:50.2 -- not an asteroid (will add it to exclusion list)
12:45:47.38 +72:40:57.0 -- not an asteroid (will add it to exclusion list)
13:00:03.31 +72:38:31.1 -- not an asteroid (will add it to exclusion list)
12:51:43.56 +73:19:25.6 -- not an asteroid (will add it to exclusion list)
13:21:11.75 +72:24:54.3 -- not an asteroid (will add it to exclusion list)
13:32:54.13 +72:02:59.2 -- not an asteroid (will add it to exclusion list)
13:33:55.24 +71:21:23.3 -- not an asteroid (will add it to exclusion list)
13:02:11.40 +72:52:54.1 -- not an asteroid (will add it to exclusion list)
13:26:11.69 +71:43:24.4 -- not an asteroid (will add it to exclusion list)
13:25:51.17 +72:01:49.7 -- not an asteroid (will add it to exclusion list)
13:10:56.33 +72:05:25.6 -- not an asteroid (will add it to exclusion list)
12:44:07.35 +73:18:47.2 -- not an asteroid (will add it to exclusion list)
13:05:21.53 +72:25:45.3 -- not an asteroid (will add it to exclusion list)
12:42:32.14 +73:16:03.8 -- not an asteroid (will add it to exclusion list)
13:36:46.97 +70:23:25.7 -- not an asteroid (will add it to exclusion list)
12:38:00.58 +73:14:46.5 -- not an asteroid (will add it to exclusion list)
13:34:29.57 +71:15:58.4 -- not an asteroid (will add it to exclusion list)
13:07:43.13 +72:45:32.8 -- not an asteroid (will add it to exclusion list)
15:28:43.89 +66:32:41.9 -- not an asteroid (will add it to exclusion list)
12:56:54.39 +73:23:00.8 -- not an asteroid (will add it to exclusion list)
12:59:27.94 +72:23:49.7 -- not an asteroid (will add it to exclusion list)
13:26:01.91 +71:22:30.4 -- not an asteroid (will add it to exclusion list)
13:32:45.22 +72:24:54.7 -- not an asteroid (will add it to exclusion list)
13:30:35.62 +72:05:15.3 -- not an asteroid (will add it to exclusion list)
12:57:46.68 +73:39:23.0 -- not an asteroid (will add it to exclusion list)
13:11:07.42 +72:13:00.7 -- not an asteroid (will add it to exclusion list)
13:15:02.19 +72:13:36.0 -- not an asteroid (will add it to exclusion list)
13:13:55.31 +72:54:06.9 -- not an asteroid (will add it to exclusion list)
13:01:07.46 +72:00:39.1 -- not an asteroid (will add it to exclusion list)
13:01:27.38 +72:29:55.0 -- not an asteroid (will add it to exclusion list)
13:25:38.02 +70:53:08.5 -- not an asteroid (will add it to exclusion list)
13:03:23.25 +73:20:26.6 -- not an asteroid (will add it to exclusion list)
13:26:52.74 +72:29:14.7 -- not an asteroid (will add it to exclusion list)
13:19:07.73 +71:38:23.1 -- not an asteroid (will add it to exclusion list)
13:08:39.58 +72:36:27.7 -- not an asteroid (will add it to exclusion list)
13:01:54.63 +73:25:18.7 -- not an asteroid (will add it to exclusion list)
13:21:38.43 +72:25:09.0 -- not an asteroid (will add it to exclusion list)
13:28:19.69 +71:29:48.9 -- not an asteroid (will add it to exclusion list)
13:18:41.07 +72:34:08.8 -- not an asteroid (will add it to exclusion list)
13:33:08.25 +70:43:28.4 -- not an asteroid (will add it to exclusion list)
13:44:18.13 +71:01:29.2 -- not an asteroid (will add it to exclusion list)
13:22:51.32 +72:33:44.9 -- not an asteroid (will add it to exclusion list)
13:40:17.14 +71:20:14.4 -- not an asteroid (will add it to exclusion list)
12:59:18.43 +72:06:04.4 -- not an asteroid (will add it to exclusion list)
13:34:59.54 +71:46:21.3 -- not an asteroid (will add it to exclusion list)
13:01:13.53 +72:36:59.1 -- not an asteroid (will add it to exclusion list)
12:59:48.61 +72:54:01.2 -- not an asteroid (will add it to exclusion list)
13:29:26.24 +71:09:19.0 -- not an asteroid (will add it to exclusion list)
13:16:44.77 +71:50:45.0 -- not an asteroid (will add it to exclusion list)
13:31:41.30 +70:58:43.2 -- not an asteroid (will add it to exclusion list)
13:04:27.57 +72:47:52.2 -- not an asteroid (will add it to exclusion list)
13:00:22.15 +73:31:39.7 -- not an asteroid (will add it to exclusion list)
13:22:19.72 +71:26:12.9 -- not an asteroid (will add it to exclusion list)
13:08:16.60 +72:54:34.7 -- not an asteroid (will add it to exclusion list)
12:58:14.71 +72:56:30.5 -- not an asteroid (will add it to exclusion list)
12:59:55.35 +73:40:22.7 -- not an asteroid (will add it to exclusion list)
13:20:06.04 +71:40:53.7 -- not an asteroid (will add it to exclusion list)
13:31:48.45 +71:15:56.7 -- not an asteroid (will add it to exclusion list)
13:32:13.19 +71:33:08.7 -- not an asteroid (will add it to exclusion list)
12:58:42.80 +72:05:27.3 -- not an asteroid (will add it to exclusion list)
13:19:37.39 +71:23:41.3 -- not an asteroid (will add it to exclusion list)
13:33:04.68 +72:21:22.5 -- not an asteroid (will add it to exclusion list)
12:43:15.10 +73:28:01.8 -- not an asteroid (will add it to exclusion list)
12:51:36.05 +72:53:33.5 -- not an asteroid (will add it to exclusion list)
13:03:17.60 +73:14:32.6 -- not an asteroid (will add it to exclusion list)
12:49:19.04 +73:42:45.5 -- not an asteroid (will add it to exclusion list)
13:19:54.76 +72:02:26.1 -- not an asteroid (will add it to exclusion list)
13:01:39.47 +72:18:56.2 -- not an asteroid (will add it to exclusion list)
13:17:03.17 +71:48:26.8 -- not an asteroid (will add it to exclusion list)
12:42:13.46 +73:02:14.2 -- not an asteroid (will add it to exclusion list)
12:39:30.60 +72:52:10.6 -- not an asteroid (will add it to exclusion list)
13:25:23.90 +72:27:25.4 -- not an asteroid (will add it to exclusion list)
13:36:53.39 +72:04:01.7 -- not an asteroid (will add it to exclusion list)
15:27:01.80 +66:33:21.5 -- not an asteroid (will add it to exclusion list)
13:01:11.16 +73:48:31.4 -- not an asteroid (will add it to exclusion list)
15:28:57.10 +66:27:31.1 -- not an asteroid (will add it to exclusion list)
13:27:37.84 +71:47:18.5 -- not an asteroid (will add it to exclusion list)
13:00:10.37 +72:03:17.6 -- not an asteroid (will add it to exclusion list)
12:49:00.94 +72:24:24.9 -- not an asteroid (will add it to exclusion list)
13:20:36.16 +72:00:44.9 -- not an asteroid (will add it to exclusion list)
13:31:41.01 +72:09:42.0 -- not an asteroid (will add it to exclusion list)
13:27:08.57 +72:23:21.6 -- not an asteroid (will add it to exclusion list)
12:37:56.18 +73:19:38.4 -- not an asteroid (will add it to exclusion list)
13:06:53.34 +71:45:28.9 -- not an asteroid (will add it to exclusion list)
13:00:19.85 +73:03:09.9 -- not an asteroid (will add it to exclusion list)
13:05:50.96 +73:04:52.6 -- not an asteroid (will add it to exclusion list)
13:22:48.03 +72:00:00.3 -- not an asteroid (will add it to exclusion list)
12:58:30.90 +73:39:51.8 -- not an asteroid (will add it to exclusion list)
12:44:20.69 +73:04:03.1 -- not an asteroid (will add it to exclusion list)
15:28:35.36 +66:28:09.1 -- not an asteroid (will add it to exclusion list)
13:32:26.42 +71:26:46.4 -- not an asteroid (will add it to exclusion list)
13:00:17.61 +73:18:02.6 -- not an asteroid (will add it to exclusion list)
12:59:09.66 +72:19:15.5 -- not an asteroid (will add it to exclusion list)
13:15:10.93 +71:40:05.6 -- not an asteroid (will add it to exclusion list)
13:33:40.87 +71:40:50.5 -- not an asteroid (will add it to exclusion list)
13:11:40.69 +73:16:13.9 -- not an asteroid (will add it to exclusion list)
13:37:38.92 +71:42:32.2 -- not an asteroid (will add it to exclusion list)
13:14:57.57 +72:44:33.8 -- not an asteroid (will add it to exclusion list)
12:53:05.28 +73:01:37.1 -- not an asteroid (will add it to exclusion list)
13:10:07.76 +72:55:54.2 -- not an asteroid (will add it to exclusion list)
13:01:32.18 +72:37:38.2 -- not an asteroid (will add it to exclusion list)
13:31:33.28 +72:04:33.9 -- not an asteroid (will add it to exclusion list)
13:35:27.28 +70:59:16.7 -- not an asteroid (will add it to exclusion list)
12:56:30.64 +72:54:58.5 -- not an asteroid (will add it to exclusion list)
12:50:07.55 +72:52:27.4 -- not an asteroid (will add it to exclusion list)
13:18:38.01 +72:55:44.6 -- not an asteroid (will add it to exclusion list)
13:12:41.18 +72:27:00.4 -- not an asteroid (will add it to exclusion list)
12:49:08.21 +73:19:04.7 -- not an asteroid (will add it to exclusion list)
13:22:57.38 +71:26:45.7 -- not an asteroid (will add it to exclusion list)
13:14:05.92 +73:07:24.7 -- not an asteroid (will add it to exclusion list)
12:52:18.39 +73:31:17.5 -- not an asteroid (will add it to exclusion list)
13:12:34.00 +71:40:43.6 -- not an asteroid (will add it to exclusion list)
13:19:40.86 +72:10:33.9 -- not an asteroid (will add it to exclusion list)
13:35:54.74 +71:15:19.2 -- not an asteroid (will add it to exclusion list)
13:06:48.64 +72:26:55.8 -- not an asteroid (will add it to exclusion list)
13:18:21.95 +72:06:23.4 -- not an asteroid (will add it to exclusion list)
13:30:10.78 +70:33:21.9 -- not an asteroid (will add it to exclusion list)
12:45:53.95 +72:47:08.0 -- not an asteroid (will add it to exclusion list)
12:50:00.76 +72:46:21.6 -- not an asteroid (will add it to exclusion list)
12:44:45.40 +73:28:34.8 -- not an asteroid (will add it to exclusion list)
13:00:11.37 +72:16:50.2 -- not an asteroid (will add it to exclusion list)
13:05:36.91 +72:15:20.6 -- not an asteroid (will add it to exclusion list)
13:01:36.16 +73:35:42.3 -- not an asteroid (will add it to exclusion list)
13:35:52.59 +71:40:36.9 -- not an asteroid (will add it to exclusion list)
13:19:53.73 +71:41:05.4 -- not an asteroid (will add it to exclusion list)
13:26:06.62 +70:54:58.2 -- not an asteroid (will add it to exclusion list)
13:36:03.99 +70:46:41.7 -- not an asteroid (will add it to exclusion list)
13:36:22.02 +70:31:25.0 -- not an asteroid (will add it to exclusion list)
15:34:39.02 +65:26:07.3 -- not an asteroid (will add it to exclusion list)
13:15:22.53 +72:25:33.6 -- not an asteroid (will add it to exclusion list)
12:56:33.26 +73:10:21.6 -- not an asteroid (will add it to exclusion list)
13:28:28.14 +71:51:10.9 -- not an asteroid (will add it to exclusion list)
13:17:18.56 +71:47:13.1 -- not an asteroid (will add it to exclusion list)
12:52:58.53 +72:33:10.8 -- not an asteroid (will add it to exclusion list)
12:56:38.70 +72:33:07.3 -- not an asteroid (will add it to exclusion list)
13:17:43.98 +71:18:39.2 -- not an asteroid (will add it to exclusion list)
13:24:28.41 +72:43:10.4 -- not an asteroid (will add it to exclusion list)
13:41:40.94 +71:00:43.9 -- not an asteroid (will add it to exclusion list)
13:31:53.93 +72:18:53.8 -- not an asteroid (will add it to exclusion list)
12:59:18.60 +72:30:03.5 -- not an asteroid (will add it to exclusion list)
13:26:16.50 +71:23:52.9 -- not an asteroid (will add it to exclusion list)
13:19:01.41 +72:26:20.4 -- not an asteroid (will add it to exclusion list)
13:36:55.68 +71:52:42.9 -- not an asteroid (will add it to exclusion list)
13:02:01.61 +73:01:21.9 -- not an asteroid (will add it to exclusion list)
13:02:29.57 +73:12:00.8 -- not an asteroid (will add it to exclusion list)
13:29:17.60 +71:21:49.5 -- not an asteroid (will add it to exclusion list)
13:23:07.70 +71:31:41.0 -- not an asteroid (will add it to exclusion list)
13:34:09.85 +70:52:16.0 -- not an asteroid (will add it to exclusion list)
13:05:00.73 +72:02:27.4 -- not an asteroid (will add it to exclusion list)
13:03:11.12 +72:22:32.4 -- not an asteroid (will add it to exclusion list)
13:31:21.37 +71:29:17.8 -- not an asteroid (will add it to exclusion list)
13:27:38.60 +72:38:45.3 -- not an asteroid (will add it to exclusion list)
13:04:13.52 +73:26:41.2 -- not an asteroid (will add it to exclusion list)
12:45:58.85 +73:10:10.9 -- not an asteroid (will add it to exclusion list)
13:18:09.50 +71:49:40.9 -- not an asteroid (will add it to exclusion list)
13:03:45.65 +73:15:30.2 -- not an asteroid (will add it to exclusion list)
13:19:41.36 +71:09:37.0 -- not an asteroid (will add it to exclusion list)
13:24:14.75 +72:35:07.8 -- not an asteroid (will add it to exclusion list)
13:18:21.78 +72:43:44.6 -- not an asteroid (will add it to exclusion list)
13:07:22.13 +72:19:13.5 -- not an asteroid (will add it to exclusion list)
13:05:51.80 +72:56:33.8 -- not an asteroid (will add it to exclusion list)
12:51:30.25 +73:37:03.7 -- not an asteroid (will add it to exclusion list)
13:13:05.96 +71:33:21.9 -- not an asteroid (will add it to exclusion list)
13:18:46.50 +71:40:22.8 -- not an asteroid (will add it to exclusion list)
13:31:08.93 +71:54:52.0 -- not an asteroid (will add it to exclusion list)
13:11:44.00 +72:27:30.6 -- not an asteroid (will add it to exclusion list)
15:24:45.65 +66:30:17.5 -- not an asteroid (will add it to exclusion list)
13:15:10.86 +72:52:25.2 -- not an asteroid (will add it to exclusion list)
13:29:49.76 +70:39:17.3 -- not an asteroid (will add it to exclusion list)
12:59:44.93 +72:30:12.4 -- not an asteroid (will add it to exclusion list)
12:46:58.60 +72:47:21.7 -- not an asteroid (will add it to exclusion list)
12:55:49.65 +73:55:36.1 -- not an asteroid (will add it to exclusion list)
13:23:10.50 +72:08:04.6 -- not an asteroid (will add it to exclusion list)
13:06:57.13 +73:02:16.2 -- not an asteroid (will add it to exclusion list)
13:19:13.86 +71:13:27.3 -- not an asteroid (will add it to exclusion list)
13:07:52.38 +72:45:41.7 -- not an asteroid (will add it to exclusion list)
12:57:19.87 +72:31:46.3 -- not an asteroid (will add it to exclusion list)
13:06:36.56 +72:49:26.6 -- not an asteroid (will add it to exclusion list)
13:21:49.45 +70:49:22.6 -- not an asteroid (will add it to exclusion list)
13:38:05.54 +71:09:31.5 -- not an asteroid (will add it to exclusion list)
13:24:56.71 +72:31:35.0 -- not an asteroid (will add it to exclusion list)
13:26:41.44 +70:49:07.7 -- not an asteroid (will add it to exclusion list)
13:18:29.52 +72:49:05.2 -- not an asteroid (will add it to exclusion list)
13:19:44.63 +70:53:44.4 -- not an asteroid (will add it to exclusion list)
13:18:14.35 +72:23:50.7 -- not an asteroid (will add it to exclusion list)
13:17:12.36 +71:49:01.2 -- not an asteroid (will add it to exclusion list)
14:39:51.55 +74:45:02.0 -- not an asteroid (will add it to exclusion list)
15:34:42.38 +66:40:58.8 -- not an asteroid (will add it to exclusion list)
13:10:18.32 +72:33:22.9 -- not an asteroid (will add it to exclusion list)
13:18:04.43 +72:06:32.9 -- not an asteroid (will add it to exclusion list)
12:48:33.08 +73:34:19.1 -- not an asteroid (will add it to exclusion list)
13:25:08.75 +70:54:00.5 -- not an asteroid (will add it to exclusion list)
15:26:36.25 +66:47:00.3 -- not an asteroid (will add it to exclusion list)
13:27:45.33 +72:42:13.4 -- not an asteroid (will add it to exclusion list)
12:41:03.28 +73:03:01.2 -- not an asteroid (will add it to exclusion list)
13:14:10.04 +72:55:43.6 -- not an asteroid (will add it to exclusion list)
13:41:15.65 +71:45:19.4 -- not an asteroid (will add it to exclusion list)
13:00:41.70 +73:25:05.1 -- not an asteroid (will add it to exclusion list)
13:37:37.74 +71:39:49.9 -- not an asteroid (will add it to exclusion list)
12:50:06.99 +72:56:48.7 -- not an asteroid (will add it to exclusion list)
13:01:30.73 +73:04:14.0 -- not an asteroid (will add it to exclusion list)
13:29:43.86 +71:43:13.0 -- not an asteroid (will add it to exclusion list)
13:39:12.41 +71:14:33.8 -- not an asteroid (will add it to exclusion list)
13:10:26.21 +72:53:39.7 -- not an asteroid (will add it to exclusion list)
13:28:10.62 +71:35:05.1 -- not an asteroid (will add it to exclusion list)
13:32:57.25 +72:14:56.1 -- not an asteroid (will add it to exclusion list)
12:57:51.79 +72:37:22.5 -- not an asteroid (will add it to exclusion list)
13:02:14.65 +73:06:46.4 -- not an asteroid (will add it to exclusion list)
13:33:28.39 +72:24:10.2 -- not an asteroid (will add it to exclusion list)
13:30:42.83 +71:36:15.4 -- not an asteroid (will add it to exclusion list)
12:41:12.12 +73:02:35.7 -- not an asteroid (will add it to exclusion list)
13:01:57.32 +72:14:01.6 -- not an asteroid (will add it to exclusion list)
12:42:14.93 +73:26:26.7 -- not an asteroid (will add it to exclusion list)
12:58:57.08 +73:46:23.7 -- not an asteroid (will add it to exclusion list)
13:18:09.40 +72:43:37.2 -- not an asteroid (will add it to exclusion list)
13:25:21.16 +72:46:50.2 -- not an asteroid (will add it to exclusion list)
13:20:48.31 +70:58:12.0 -- not an asteroid (will add it to exclusion list)
13:19:41.80 +72:00:39.5 -- not an asteroid (will add it to exclusion list)
15:26:38.72 +66:13:52.6 -- not an asteroid (will add it to exclusion list)
13:12:08.64 +72:08:20.0 -- not an asteroid (will add it to exclusion list)
12:53:33.98 +72:58:24.2 -- not an asteroid (will add it to exclusion list)
13:32:14.74 +72:16:35.6 -- not an asteroid (will add it to exclusion list)
12:46:55.10 +73:04:47.9 -- not an asteroid (will add it to exclusion list)
15:33:52.91 +66:43:08.2 -- not an asteroid (will add it to exclusion list)
13:28:32.66 +70:44:48.1 -- not an asteroid (will add it to exclusion list)
12:55:19.61 +73:11:10.9 -- not an asteroid (will add it to exclusion list)
12:53:41.96 +72:51:35.4 -- not an asteroid (will add it to exclusion list)
13:04:49.66 +73:10:44.9 -- not an asteroid (will add it to exclusion list)
13:18:36.11 +72:54:37.6 -- not an asteroid (will add it to exclusion list)
15:26:54.39 +66:13:17.5 -- not an asteroid (will add it to exclusion list)
15:29:40.01 +66:22:09.7 -- not an asteroid (will add it to exclusion list)
13:21:42.11 +71:49:32.8 -- not an asteroid (will add it to exclusion list)
13:19:02.60 +72:12:15.6 -- not an asteroid (will add it to exclusion list)
12:57:40.47 +73:42:17.3 -- not an asteroid (will add it to exclusion list)
15:32:04.15 +66:44:42.6 -- not an asteroid (will add it to exclusion list)
13:12:59.50 +71:49:15.5 -- not an asteroid (will add it to exclusion list)
13:57:59.75 +65:11:33.9 -- not an asteroid (will add it to exclusion list)
15:33:00.32 +66:46:59.1 -- not an asteroid (will add it to exclusion list)
13:22:13.66 +71:33:59.2 -- not an asteroid (will add it to exclusion list)
12:47:27.60 +72:58:59.4 -- not an asteroid (will add it to exclusion list)
13:28:28.78 +72:14:26.9 -- not an asteroid (will add it to exclusion list)
12:42:15.51 +73:10:27.4 -- not an asteroid (will add it to exclusion list)
13:16:48.08 +71:47:22.9 -- not an asteroid (will add it to exclusion list)
15:38:50.47 +66:21:18.4 -- not an asteroid (will add it to exclusion list)
13:14:51.04 +71:13:37.0 -- not an asteroid (will add it to exclusion list)
13:07:36.05 +72:24:14.1 -- not an asteroid (will add it to exclusion list)
12:42:23.11 +72:56:59.5 -- not an asteroid (will add it to exclusion list)
13:31:47.08 +71:30:01.6 -- not an asteroid (will add it to exclusion list)
13:16:37.02 +72:38:14.7 -- not an asteroid (will add it to exclusion list)
13:12:11.60 +71:58:43.3 -- not an asteroid (will add it to exclusion list)
13:28:19.91 +71:48:42.0 -- not an asteroid (will add it to exclusion list)
13:19:14.09 +72:21:29.2 -- not an asteroid (will add it to exclusion list)
12:55:48.29 +72:45:00.8 -- not an asteroid (will add it to exclusion list)
12:56:35.85 +73:05:53.9 -- not an asteroid (will add it to exclusion list)
13:59:20.65 +65:04:45.3 -- not an asteroid (will add it to exclusion list)
13:23:03.11 +72:12:04.0 -- not an asteroid (will add it to exclusion list)
13:15:58.55 +71:29:31.8 -- not an asteroid (will add it to exclusion list)
13:29:41.97 +71:38:00.1 -- not an asteroid (will add it to exclusion list)
12:47:59.90 +72:38:01.7 -- not an asteroid (will add it to exclusion list)
12:40:39.87 +73:09:49.0 -- not an asteroid (will add it to exclusion list)
13:27:49.33 +71:38:22.9 -- not an asteroid (will add it to exclusion list)
13:07:29.14 +72:31:57.2 -- not an asteroid (will add it to exclusion list)
13:06:14.57 +73:00:50.9 -- not an asteroid (will add it to exclusion list)
13:18:59.42 +71:06:15.0 -- not an asteroid (will add it to exclusion list)
12:53:21.40 +72:25:56.1 -- not an asteroid (will add it to exclusion list)
12:59:42.36 +73:31:47.8 -- not an asteroid (will add it to exclusion list)
13:04:04.32 +72:11:18.2 -- not an asteroid (will add it to exclusion list)
12:59:58.49 +72:16:01.9 -- not an asteroid (will add it to exclusion list)
13:31:30.72 +71:01:18.8 -- not an asteroid (will add it to exclusion list)
13:20:15.34 +71:56:49.3 -- not an asteroid (will add it to exclusion list)
12:56:04.03 +73:44:00.0 -- not an asteroid (will add it to exclusion list)
15:30:30.75 +65:56:33.3 -- not an asteroid (will add it to exclusion list)
13:28:23.40 +72:16:58.8 -- not an asteroid (will add it to exclusion list)
13:09:35.39 +72:18:19.3 -- not an asteroid (will add it to exclusion list)
12:46:13.38 +73:23:53.6 -- not an asteroid (will add it to exclusion list)
13:05:01.67 +72:01:12.2 -- not an asteroid (will add it to exclusion list)
13:23:48.95 +71:20:01.3 -- not an asteroid (will add it to exclusion list)
13:19:54.31 +72:27:35.2 -- not an asteroid (will add it to exclusion list)
12:53:30.40 +73:30:54.2 -- not an asteroid (will add it to exclusion list)
13:15:25.65 +72:28:57.1 -- not an asteroid (will add it to exclusion list)
12:57:01.28 +72:31:02.8 -- not an asteroid (will add it to exclusion list)
13:35:11.50 +70:45:22.3 -- not an asteroid (will add it to exclusion list)
12:42:14.72 +72:54:27.9 -- not an asteroid (will add it to exclusion list)
12:45:16.50 +72:47:01.5 -- not an asteroid (will add it to exclusion list)
13:10:21.41 +71:29:45.1 -- not an asteroid (will add it to exclusion list)
13:15:10.77 +71:35:10.6 -- not an asteroid (will add it to exclusion list)
12:51:09.46 +72:54:30.7 -- not an asteroid (will add it to exclusion list)
15:25:13.93 +66:40:57.3 -- not an asteroid (will add it to exclusion list)
13:03:01.60 +72:23:53.6 -- not an asteroid (will add it to exclusion list)
13:12:12.08 +72:17:46.1 -- not an asteroid (will add it to exclusion list)
13:34:51.12 +70:39:22.9 -- not an asteroid (will add it to exclusion list)
13:06:58.61 +71:54:42.0 -- not an asteroid (will add it to exclusion list)
13:07:38.62 +72:57:40.7 -- not an asteroid (will add it to exclusion list)
12:53:53.44 +73:27:44.7 -- not an asteroid (will add it to exclusion list)
12:58:13.25 +72:07:39.4 -- not an asteroid (will add it to exclusion list)
12:48:07.67 +73:06:03.1 -- not an asteroid (will add it to exclusion list)
12:55:10.56 +73:41:29.7 -- not an asteroid (will add it to exclusion list)
13:19:24.05 +72:56:45.9 -- not an asteroid (will add it to exclusion list)
12:48:42.43 +73:27:28.0 -- not an asteroid (will add it to exclusion list)
15:31:51.21 +65:47:40.0 -- not an asteroid (will add it to exclusion list)
13:33:35.69 +71:50:20.1 -- not an asteroid (will add it to exclusion list)
13:02:41.04 +73:16:08.6 -- not an asteroid (will add it to exclusion list)
13:25:30.35 +72:11:17.3 -- not an asteroid (will add it to exclusion list)
13:27:03.84 +71:21:44.7 -- not an asteroid (will add it to exclusion list)
13:24:19.97 +72:16:40.8 -- not an asteroid (will add it to exclusion list)
12:55:27.64 +73:34:50.8 -- not an asteroid (will add it to exclusion list)
12:41:37.94 +72:39:28.1 -- not an asteroid (will add it to exclusion list)
12:53:46.89 +72:39:27.3 -- not an asteroid (will add it to exclusion list)
13:21:38.79 +72:22:17.3 -- not an asteroid (will add it to exclusion list)
13:15:36.74 +71:31:36.6 -- not an asteroid (will add it to exclusion list)
12:56:58.43 +72:04:42.6 -- not an asteroid (will add it to exclusion list)
12:50:43.42 +72:45:48.8 -- not an asteroid (will add it to exclusion list)
12:59:29.29 +72:43:47.7 -- not an asteroid (will add it to exclusion list)
13:09:38.74 +72:36:50.6 -- not an asteroid (will add it to exclusion list)
13:13:41.66 +71:25:39.4 -- not an asteroid (will add it to exclusion list)
12:57:59.23 +72:27:33.7 -- not an asteroid (will add it to exclusion list)
13:31:41.82 +71:09:49.5 -- not an asteroid (will add it to exclusion list)
13:32:11.93 +70:52:05.7 -- not an asteroid (will add it to exclusion list)
13:06:22.45 +73:06:01.7 -- not an asteroid (will add it to exclusion list)
13:30:34.13 +70:47:33.1 -- not an asteroid (will add it to exclusion list)
13:35:27.73 +71:16:15.3 -- not an asteroid (will add it to exclusion list)
13:13:31.62 +73:12:51.1 -- not an asteroid (will add it to exclusion list)
13:38:18.10 +71:59:08.1 -- not an asteroid (will add it to exclusion list)
13:27:09.45 +71:37:01.0 -- not an asteroid (will add it to exclusion list)
13:06:37.92 +71:49:10.7 -- not an asteroid (will add it to exclusion list)
13:09:49.33 +71:29:36.3 -- not an asteroid (will add it to exclusion list)
12:56:48.04 +73:24:02.2 -- not an asteroid (will add it to exclusion list)
13:08:36.45 +72:34:01.6 -- not an asteroid (will add it to exclusion list)
12:53:43.46 +73:41:35.5 -- not an asteroid (will add it to exclusion list)
12:58:13.32 +72:32:40.1 -- not an asteroid (will add it to exclusion list)
15:30:26.56 +65:59:47.7 -- not an asteroid (will add it to exclusion list)
12:58:13.32 +72:38:48.0 -- not an asteroid (will add it to exclusion list)
13:14:05.78 +72:23:39.7 -- not an asteroid (will add it to exclusion list)
15:30:36.25 +66:16:20.0 -- not an asteroid (will add it to exclusion list)
13:18:25.86 +71:56:30.8 -- not an asteroid (will add it to exclusion list)
13:09:23.80 +71:46:20.2 -- not an asteroid (will add it to exclusion list)
13:30:17.47 +70:48:43.0 -- not an asteroid (will add it to exclusion list)
12:55:27.84 +72:59:31.0 -- not an asteroid (will add it to exclusion list)
13:26:11.11 +72:28:30.5 -- not an asteroid (will add it to exclusion list)
12:56:39.60 +73:24:41.5 -- not an asteroid (will add it to exclusion list)
13:30:39.53 +72:06:57.0 -- not an asteroid (will add it to exclusion list)
13:05:35.49 +72:36:10.2 -- not an asteroid (will add it to exclusion list)
13:02:47.69 +72:07:41.9 -- not an asteroid (will add it to exclusion list)
13:22:14.55 +71:53:42.1 -- not an asteroid (will add it to exclusion list)
13:02:47.64 +72:20:36.7 -- not an asteroid (will add it to exclusion list)
13:33:41.75 +72:13:21.9 -- not an asteroid (will add it to exclusion list)
13:38:25.39 +71:21:43.9 -- not an asteroid (will add it to exclusion list)
13:05:17.21 +72:58:12.6 -- not an asteroid (will add it to exclusion list)
13:01:32.26 +72:59:58.2 -- not an asteroid (will add it to exclusion list)
13:14:57.95 +72:09:22.5 -- not an asteroid (will add it to exclusion list)
12:58:11.39 +72:24:21.6 -- not an asteroid (will add it to exclusion list)
13:12:36.34 +71:37:05.6 -- not an asteroid (will add it to exclusion list)
13:13:45.43 +72:37:49.5 -- not an asteroid (will add it to exclusion list)
13:18:02.75 +71:58:55.7 -- not an asteroid (will add it to exclusion list)
13:14:45.15 +72:22:38.8 -- not an asteroid (will add it to exclusion list)
13:11:26.71 +72:26:15.0 -- not an asteroid (will add it to exclusion list)
13:12:40.00 +72:14:22.0 -- not an asteroid (will add it to exclusion list)
12:44:23.09 +73:33:00.3 -- not an asteroid (will add it to exclusion list)
12:57:03.50 +73:13:07.1 -- not an asteroid (will add it to exclusion list)
12:58:10.36 +72:28:01.6 -- not an asteroid (will add it to exclusion list)
12:59:36.62 +73:07:19.6 -- not an asteroid (will add it to exclusion list)
15:28:55.94 +66:26:17.9 -- not an asteroid (will add it to exclusion list)
12:40:22.64 +73:16:32.8 -- not an asteroid (will add it to exclusion list)
13:14:58.52 +73:02:21.4 -- not an asteroid (will add it to exclusion list)
15:27:08.39 +66:24:52.0 -- not an asteroid (will add it to exclusion list)
13:26:05.25 +72:26:40.0 -- not an asteroid (will add it to exclusion list)
13:02:01.45 +73:17:18.6 -- not an asteroid (will add it to exclusion list)
13:01:44.75 +72:30:31.8 -- not an asteroid (will add it to exclusion list)
13:19:44.06 +71:48:17.9 -- not an asteroid (will add it to exclusion list)
13:25:49.95 +71:19:29.6 -- not an asteroid (will add it to exclusion list)
15:34:41.44 +66:38:48.3 -- not an asteroid (will add it to exclusion list)
13:27:35.12 +71:57:24.0 -- not an asteroid (will add it to exclusion list)
15:35:55.99 +66:40:56.0 -- not an asteroid (will add it to exclusion list)
15:27:00.65 +66:36:15.0 -- not an asteroid (will add it to exclusion list)
13:06:49.50 +72:59:51.6 -- not an asteroid (will add it to exclusion list)
15:33:02.87 +65:39:21.6 -- not an asteroid (will add it to exclusion list)
12:59:01.22 +72:57:48.4 -- not an asteroid (will add it to exclusion list)
13:07:33.81 +72:21:04.7 -- not an asteroid (will add it to exclusion list)
13:15:32.61 +72:25:15.8 -- not an asteroid (will add it to exclusion list)
13:21:04.85 +71:24:56.5 -- not an asteroid (will add it to exclusion list)
13:01:47.15 +72:18:24.1 -- not an asteroid (will add it to exclusion list)
13:03:29.81 +72:40:31.1 -- not an asteroid (will add it to exclusion list)
13:02:40.92 +72:44:20.7 -- not an asteroid (will add it to exclusion list)
13:17:58.18 +71:50:32.8 -- not an asteroid (will add it to exclusion list)
12:56:31.37 +73:20:25.1 -- not an asteroid (will add it to exclusion list)
12:49:05.93 +73:14:01.5 -- not an asteroid (will add it to exclusion list)
13:34:47.19 +71:51:11.5 -- not an asteroid (will add it to exclusion list)
13:21:17.88 +72:33:25.2 -- not an asteroid (will add it to exclusion list)
15:38:54.93 +66:17:18.3 -- not an asteroid (will add it to exclusion list)
12:36:37.68 +73:17:54.9 -- not an asteroid (will add it to exclusion list)
12:41:58.81 +73:10:55.9 -- not an asteroid (will add it to exclusion list)
13:18:56.85 +72:31:43.8 -- not an asteroid (will add it to exclusion list)
12:51:43.52 +72:36:44.3 -- not an asteroid (will add it to exclusion list)
12:46:24.81 +72:54:36.6 -- not an asteroid (will add it to exclusion list)
13:09:41.33 +72:26:38.9 -- not an asteroid (will add it to exclusion list)
13:09:52.90 +73:14:32.3 -- not an asteroid (will add it to exclusion list)
12:41:01.06 +73:24:48.5 -- not an asteroid (will add it to exclusion list)
13:34:15.49 +72:07:44.6 -- not an asteroid (will add it to exclusion list)
13:11:46.15 +72:34:35.4 -- not an asteroid (will add it to exclusion list)
12:48:40.12 +73:32:19.5 -- not an asteroid (will add it to exclusion list)
12:50:59.23 +72:44:33.4 -- not an asteroid (will add it to exclusion list)
13:17:46.16 +71:43:15.4 -- not an asteroid (will add it to exclusion list)
12:36:31.04 +73:19:07.8 -- not an asteroid (will add it to exclusion list)
13:30:29.24 +72:00:25.8 -- not an asteroid (will add it to exclusion list)
13:27:29.93 +71:42:32.6 -- not an asteroid (will add it to exclusion list)
13:02:55.03 +72:18:40.8 -- not an asteroid (will add it to exclusion list)
13:16:34.92 +72:40:37.4 -- not an asteroid (will add it to exclusion list)
13:10:07.70 +71:50:50.2 -- not an asteroid (will add it to exclusion list)
12:58:07.13 +72:57:47.8 -- not an asteroid (will add it to exclusion list)
13:23:59.13 +71:50:27.0 -- not an asteroid (will add it to exclusion list)
12:47:42.19 +73:04:40.0 -- not an asteroid (will add it to exclusion list)
13:01:08.37 +72:19:37.4 -- not an asteroid (will add it to exclusion list)
12:54:52.75 +72:45:42.9 -- not an asteroid (will add it to exclusion list)
13:04:25.11 +72:51:34.8 -- not an asteroid (will add it to exclusion list)
12:41:58.30 +72:57:48.6 -- not an asteroid (will add it to exclusion list)
13:11:09.70 +72:48:43.1 -- not an asteroid (will add it to exclusion list)
13:18:01.59 +72:23:16.1 -- not an asteroid (will add it to exclusion list)
13:32:43.17 +71:44:41.0 -- not an asteroid (will add it to exclusion list)
13:11:25.29 +72:08:18.4 -- not an asteroid (will add it to exclusion list)
13:18:23.28 +72:39:40.8 -- not an asteroid (will add it to exclusion list)
13:10:21.80 +72:48:47.9 -- not an asteroid (will add it to exclusion list)
13:11:49.43 +72:19:25.6 -- not an asteroid (will add it to exclusion list)
12:48:57.79 +72:53:58.7 -- not an asteroid (will add it to exclusion list)
12:54:54.16 +72:37:19.8 -- not an asteroid (will add it to exclusion list)
13:03:42.54 +72:51:11.4 -- not an asteroid (will add it to exclusion list)
13:23:15.12 +72:02:51.7 -- not an asteroid (will add it to exclusion list)
13:28:48.74 +71:58:22.8 -- not an asteroid (will add it to exclusion list)
13:19:28.26 +71:37:18.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
12:36:31.04 +73:19:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:36:37.68 +73:17:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:37:56.18 +73:19:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:38:00.58 +73:14:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:39:30.60 +72:52:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:05.33 +73:13:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:22.64 +73:16:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:40:39.87 +73:09:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:01.06 +73:24:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:03.28 +73:03:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:12.12 +73:02:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:37.94 +72:39:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:38.63 +72:44:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:39.35 +72:54:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:58.30 +72:57:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:41:58.81 +73:10:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:13.46 +73:02:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:14.72 +72:54:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:14.93 +73:26:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:15.51 +73:10:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:23.11 +72:56:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:42:32.14 +73:16:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:43:15.10 +73:28:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:43:48.66 +73:22:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:07.35 +73:18:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:20.10 +73:18:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:20.69 +73:04:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:23.09 +73:33:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:44:45.40 +73:28:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:16.50 +72:47:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:47.38 +72:40:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:53.95 +72:47:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:45:58.85 +73:10:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:02.58 +73:26:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:13.38 +73:23:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:24.81 +72:54:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:55.10 +73:04:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:46:58.60 +72:47:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:02.63 +73:12:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:27.60 +72:58:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:42.19 +73:04:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:50.85 +72:59:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:47:59.90 +72:38:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:07.67 +73:06:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:18.74 +73:10:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:33.08 +73:34:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:40.12 +73:32:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:42.43 +73:27:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:47.38 +72:59:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:48:57.79 +72:53:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:00.94 +72:24:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:02.47 +72:33:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:05.93 +73:14:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:08.21 +73:19:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:19.04 +73:42:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:19.10 +73:14:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:49:44.61 +73:08:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:00.76 +72:46:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:06.99 +72:56:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:07.55 +72:52:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:10.58 +73:36:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:18.37 +72:36:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:31.15 +73:11:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:43.42 +72:45:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:50:59.23 +72:44:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:09.46 +72:54:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:17.47 +73:31:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:25.91 +72:45:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:30.25 +73:37:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:36.05 +72:53:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:40.12 +73:07:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:43.52 +72:36:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:51:43.56 +73:19:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:18.39 +73:31:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:55.29 +72:50:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:52:58.53 +72:33:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:05.28 +73:01:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:21.40 +72:25:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:30.40 +73:30:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:33.98 +72:58:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:37.32 +73:38:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:41.96 +72:51:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:43.46 +73:41:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:46.89 +72:39:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:47.77 +73:06:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:53:53.44 +73:27:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:54:20.09 +72:46:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:54:52.75 +72:45:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:54:54.16 +72:37:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:54:54.68 +73:09:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:55:04.45 +72:47:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:55:10.52 +72:36:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:55:10.56 +73:41:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:55:17.14 +73:24:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:55:19.61 +73:11:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:55:27.64 +73:34:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:55:27.84 +72:59:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:55:48.29 +72:45:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:55:49.65 +73:55:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:04.03 +73:44:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:27.99 +72:42:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:30.64 +72:54:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:31.37 +73:20:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:33.26 +73:10:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:35.85 +73:05:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:38.70 +72:33:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:39.60 +73:24:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:48.04 +73:24:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:54.39 +73:23:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:55.90 +72:43:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:56:58.43 +72:04:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:01.28 +72:31:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:03.50 +73:13:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:13.79 +72:39:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:19.87 +72:31:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:25.78 +73:24:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:30.88 +73:39:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:40.47 +73:42:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:44.81 +73:14:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:46.68 +73:39:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:51.79 +72:37:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:57:59.23 +72:27:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:02.55 +72:22:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:03.43 +72:40:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:07.13 +72:57:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:10.36 +72:28:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:11.39 +72:24:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:13.25 +72:07:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:13.32 +72:32:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:13.32 +72:38:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:14.71 +72:56:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:19.98 +72:16:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:30.58 +72:46:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:30.90 +73:39:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:33.33 +73:28:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:42.59 +72:58:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:42.80 +72:05:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
12:58:57.08 +73:46:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:01.22 +72:57:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:09.66 +72:19:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:18.43 +72:06:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:18.60 +72:30:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:27.31 +72:44:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:27.94 +72:23:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:29.29 +72:43:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:36.62 +73:07:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:42.36 +73:31:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:44.93 +72:30:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:48.61 +72:54:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:55.35 +73:40:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
12:59:58.49 +72:16:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:01.80 +72:50:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:02.15 +73:26:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:03.31 +72:38:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:06.20 +73:36:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:10.37 +72:03:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:11.37 +72:16:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:16.10 +72:41:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:17.61 +73:18:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:19.85 +73:03:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:22.15 +73:31:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:41.05 +72:40:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:41.70 +73:25:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:00:49.89 +72:58:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:01.23 +72:35:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:03.11 +72:18:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:07.46 +72:00:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:08.37 +72:19:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:11.16 +73:48:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:13.53 +72:36:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:23.83 +73:19:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:27.38 +72:29:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:30.73 +73:04:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:32.18 +72:37:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:32.26 +72:59:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:36.16 +73:35:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:39.47 +72:18:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:44.75 +72:30:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:47.15 +72:18:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:49.98 +73:05:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:54.63 +73:25:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:01:57.32 +72:14:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:01.31 +73:04:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:01.45 +73:17:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:01.61 +73:01:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:11.40 +72:52:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:14.65 +73:06:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:29.57 +73:12:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:40.92 +72:44:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:41.04 +73:16:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:47.64 +72:20:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:47.69 +72:07:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:02:55.03 +72:18:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:03:01.60 +72:23:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:03:11.12 +72:22:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:03:17.60 +73:14:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:03:23.25 +73:20:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:03:29.81 +72:40:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:03:40.05 +72:56:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:03:42.54 +72:51:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:03:45.65 +73:15:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:04:04.32 +72:11:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:04:04.51 +73:30:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:04:13.52 +73:26:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:04:18.31 +71:56:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:04:25.11 +72:51:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:04:26.17 +73:14:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:04:26.86 +72:50:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:04:27.57 +72:47:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:04:41.75 +73:27:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:04:49.66 +73:10:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:05:00.73 +72:02:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:05:01.67 +72:01:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:05:17.21 +72:58:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:05:21.53 +72:25:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:05:33.68 +72:16:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:05:35.49 +72:36:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:05:36.91 +72:15:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:05:42.21 +72:16:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:05:50.96 +73:04:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:05:51.80 +72:56:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:05:55.27 +72:05:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:03.28 +72:30:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:08.59 +72:20:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:14.57 +73:00:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:22.45 +73:06:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:30.73 +72:08:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:34.93 +72:25:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:36.56 +72:49:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:37.92 +71:49:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:42.04 +72:40:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:48.64 +72:26:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:49.50 +72:59:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:53.34 +71:45:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:57.13 +73:02:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:06:58.61 +71:54:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:18.75 +72:22:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:20.98 +72:44:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:22.13 +72:19:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:25.77 +72:39:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:29.03 +73:10:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:29.14 +72:31:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:33.55 +72:54:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:33.81 +72:21:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:36.05 +72:24:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:38.62 +72:57:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:43.13 +72:45:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:07:52.38 +72:45:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:08:06.85 +72:26:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:08:16.60 +72:54:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:08:31.68 +72:09:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:08:33.28 +72:39:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:08:36.45 +72:34:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:08:37.09 +72:31:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:08:39.58 +72:36:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:09:22.55 +71:38:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:09:23.80 +71:46:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:09:35.39 +72:18:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:09:38.74 +72:36:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:09:41.33 +72:26:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:09:49.33 +71:29:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:09:52.90 +73:14:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:09:59.18 +73:16:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:10:07.70 +71:50:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:10:07.76 +72:55:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:10:18.32 +72:33:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:10:21.41 +71:29:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:10:21.80 +72:48:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:10:26.21 +72:53:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:10:44.22 +71:45:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:10:52.40 +71:46:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:10:56.33 +72:05:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:07.42 +72:13:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:09.70 +72:48:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:11.35 +71:58:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:25.29 +72:08:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:26.71 +72:26:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:40.69 +73:16:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:44.00 +72:27:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:46.15 +72:34:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:11:49.43 +72:19:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:08.64 +72:08:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:11.60 +71:58:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:12.08 +72:17:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:16.25 +72:21:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:34.00 +71:40:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:34.95 +72:59:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:36.34 +71:37:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:39.08 +72:25:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:40.00 +72:14:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:41.18 +72:27:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:12:59.50 +71:49:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:03.94 +72:55:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:05.96 +71:33:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:17.73 +72:11:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:30.12 +72:30:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:31.62 +73:12:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:32.47 +72:42:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:41.66 +71:25:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:45.43 +72:37:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:50.51 +71:48:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:13:55.31 +72:54:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:05.78 +72:23:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:05.92 +73:07:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:10.04 +72:55:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:10.93 +71:30:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:17.41 +72:12:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:20.50 +72:35:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:32.87 +72:41:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:45.15 +72:22:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:51.04 +71:13:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:57.57 +72:44:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:57.95 +72:09:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:14:58.52 +73:02:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:02.19 +72:13:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:10.77 +71:35:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:10.86 +72:52:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:10.93 +71:40:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:15.15 +71:47:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:16.78 +72:31:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:22.53 +72:25:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:22.65 +72:12:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:25.65 +72:28:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:32.61 +72:25:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:36.74 +71:31:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:46.85 +72:10:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:47.45 +72:07:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:56.81 +72:02:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:15:58.55 +71:29:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:09.04 +71:42:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:11.35 +72:52:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:26.32 +71:58:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:27.07 +71:56:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:34.92 +72:40:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:37.02 +72:38:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:37.10 +72:17:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:44.77 +71:50:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:48.08 +71:47:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:54.28 +72:37:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:16:59.46 +72:03:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:03.17 +71:48:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:12.36 +71:49:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:18.56 +71:47:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:31.63 +72:07:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:40.41 +72:20:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:43.98 +71:18:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:46.16 +71:43:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:17:58.18 +71:50:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:01.59 +72:23:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:02.75 +71:58:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:02.85 +71:49:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:04.43 +72:06:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:09.40 +72:43:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:09.50 +71:49:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:14.35 +72:23:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:15.77 +72:31:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:21.78 +72:43:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:21.95 +72:06:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:23.28 +72:39:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:25.86 +71:56:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:29.52 +72:49:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:32.27 +71:51:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:36.11 +72:54:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:38.01 +72:55:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:41.07 +72:34:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:46.50 +71:40:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:56.85 +72:31:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:18:59.42 +71:06:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:01.41 +72:26:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:02.60 +72:12:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:07.73 +71:38:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:13.86 +71:13:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:14.09 +72:21:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:24.05 +72:56:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:28.26 +71:37:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:33.78 +71:55:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:37.39 +71:23:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:40.86 +72:10:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:41.36 +71:09:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:41.80 +72:00:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:44.06 +71:48:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:44.63 +70:53:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:51.40 +71:37:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:53.73 +71:41:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:54.31 +72:27:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:54.76 +72:02:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:19:56.41 +71:30:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:06.04 +71:40:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:10.61 +71:38:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:15.34 +71:56:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:15.71 +72:34:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:36.16 +72:00:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:38.91 +72:39:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:46.11 +71:47:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:46.24 +72:50:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:48.31 +70:58:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:20:55.33 +71:03:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:04.85 +71:24:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:11.75 +72:24:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:14.53 +71:48:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:16.99 +71:30:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:17.88 +72:33:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:19.87 +72:18:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:23.84 +72:06:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:29.70 +72:15:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:30.41 +71:27:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:36.40 +71:58:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:38.43 +72:25:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:38.79 +72:22:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:39.25 +71:43:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:39.33 +71:41:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:42.11 +71:49:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:49.45 +70:49:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:21:59.20 +71:34:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:13.66 +71:33:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:14.55 +71:53:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:19.72 +71:26:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:48.03 +72:00:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:50.13 +72:28:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:51.32 +72:33:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:55.68 +72:32:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:57.38 +71:26:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:57.92 +71:04:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:22:58.81 +71:33:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:03.11 +72:12:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:03.77 +72:21:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:07.70 +71:31:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:10.50 +72:08:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:15.12 +72:02:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:20.53 +72:39:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:26.11 +71:20:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:26.14 +71:25:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:33.99 +71:14:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:48.95 +71:20:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:54.43 +71:33:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:23:59.13 +71:50:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:01.15 +71:55:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:02.37 +72:15:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:12.23 +70:57:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:14.75 +72:35:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:16.16 +71:30:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:19.97 +72:16:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:28.41 +72:43:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:46.70 +71:35:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:51.51 +72:16:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:24:56.71 +72:31:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:00.45 +71:26:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:07.60 +71:30:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:08.75 +70:54:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:21.16 +72:46:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:23.90 +72:27:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:30.35 +72:11:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:31.63 +70:40:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:33.26 +70:55:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:38.02 +70:53:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:41.60 +70:54:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:49.95 +71:19:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:25:51.17 +72:01:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:01.91 +71:22:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:05.25 +72:26:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:06.62 +70:54:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:11.11 +72:28:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:11.69 +71:43:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:16.50 +71:23:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:30.90 +72:01:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:39.43 +71:55:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:41.44 +70:49:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:50.22 +71:29:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:26:52.74 +72:29:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:03.84 +71:21:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:04.28 +72:07:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:08.57 +72:23:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:09.45 +71:37:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:29.93 +71:42:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:33.94 +71:46:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:35.12 +71:57:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:37.84 +71:47:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:38.60 +72:38:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:41.73 +72:08:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:45.33 +72:42:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:27:49.33 +71:38:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:02.22 +71:33:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:10.62 +71:35:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:19.69 +71:29:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:19.91 +71:48:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:20.72 +71:55:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:23.40 +72:16:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:23.57 +70:39:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:28.14 +71:51:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:28.78 +72:14:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:32.66 +70:44:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:32.68 +71:45:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:38.58 +71:33:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:43.51 +71:22:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:48.74 +71:58:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:50.89 +72:13:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:28:54.98 +72:25:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:09.79 +72:14:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:10.08 +72:02:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:14.34 +72:06:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:17.60 +71:21:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:23.30 +71:07:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:26.24 +71:09:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:32.39 +71:37:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:41.97 +71:38:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:43.86 +71:43:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:29:49.76 +70:39:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:10.78 +70:33:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:17.47 +70:48:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:18.59 +72:11:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:29.24 +72:00:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:34.13 +70:47:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:35.62 +72:05:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:39.53 +72:06:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:30:42.83 +71:36:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:08.93 +71:54:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:21.37 +71:29:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:30.72 +71:01:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:33.28 +72:04:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:41.01 +72:09:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:41.30 +70:58:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:41.82 +71:09:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:47.08 +71:30:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:48.45 +71:15:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:31:53.93 +72:18:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:08.94 +71:25:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:11.93 +70:52:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:13.19 +71:33:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:14.74 +72:16:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:15.12 +72:06:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:16.86 +71:26:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:26.42 +71:26:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:34.71 +72:01:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:39.82 +72:03:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:41.35 +70:58:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:42.39 +71:06:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:43.17 +71:44:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:45.22 +72:24:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:54.13 +72:02:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:32:57.25 +72:14:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:04.68 +72:21:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:08.25 +70:43:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:28.39 +72:24:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:35.69 +71:50:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:40.87 +71:40:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:41.75 +72:13:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:33:55.24 +71:21:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:09.85 +70:52:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:11.36 +71:38:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:15.26 +71:33:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:15.49 +72:07:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:29.57 +71:15:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:39.39 +70:31:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:40.95 +71:34:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:47.19 +71:51:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:51.12 +70:39:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:34:59.54 +71:46:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:04.47 +70:56:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:06.68 +71:37:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:11.50 +70:45:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:24.47 +71:05:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:24.95 +72:17:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:27.28 +70:59:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:27.73 +71:16:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:29.66 +71:23:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:52.59 +71:40:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:35:54.74 +71:15:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:03.99 +70:46:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:15.70 +71:16:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:16.68 +71:41:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:22.02 +70:31:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:35.78 +71:56:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:41.40 +71:23:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:46.97 +70:23:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:53.39 +72:04:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
13:36:55.68 +71:52:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:37:37.74 +71:39:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:37:38.92 +71:42:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:37:40.30 +71:23:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:37:44.01 +71:56:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:38:05.54 +71:09:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:38:08.95 +71:03:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:38:18.10 +71:59:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:38:25.39 +71:21:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:38:35.67 +71:01:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:39:02.21 +71:46:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:39:12.41 +71:14:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
13:39:16.57 +70:16:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:39:22.44 +71:07:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
13:39:59.05 +71:25:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
13:40:12.72 +71:01:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
13:40:17.14 +71:20:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:41:15.65 +71:45:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
13:41:40.94 +71:00:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:41:41.88 +71:05:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
13:44:18.13 +71:01:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
13:44:18.84 +70:54:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
13:57:59.75 +65:11:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
13:59:20.65 +65:04:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
14:39:51.55 +74:45:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:24:45.65 +66:30:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:25:13.93 +66:40:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:26:36.25 +66:47:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:26:38.72 +66:13:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:26:54.39 +66:13:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:27:00.65 +66:36:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:27:01.80 +66:33:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:27:08.39 +66:24:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:28:35.36 +66:28:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:28:43.89 +66:32:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:28:55.94 +66:26:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:28:57.10 +66:27:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:29:40.01 +66:22:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:30:26.56 +65:59:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:30:30.75 +65:56:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:30:36.25 +66:16:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:31:51.21 +65:47:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:32:04.15 +66:44:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:33:00.32 +66:46:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:33:02.87 +65:39:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:33:52.91 +66:43:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:34:06.07 +65:42:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:34:39.02 +65:26:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:34:41.44 +66:38:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:34:42.38 +66:40:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:34:52.40 +65:39:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:35:55.99 +66:40:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:36:12.29 +65:44:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:36:58.16 +65:28:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:37:01.65 +65:32:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:38:50.47 +66:21:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:38:54.93 +66:17:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
12:36:31.04 +73:19:07.8 -- not a known variable star
12:36:37.68 +73:17:54.9 -- not a known variable star
12:37:56.18 +73:19:38.4 -- not a known variable star
12:38:00.58 +73:14:46.5 -- not a known variable star
12:39:30.60 +72:52:10.6 -- not a known variable star
12:40:05.33 +73:13:28.7 -- not a known variable star
12:40:22.64 +73:16:32.8 -- not a known variable star
12:40:39.87 +73:09:49.0 -- not a known variable star
12:41:01.06 +73:24:48.5 -- not a known variable star
12:41:03.28 +73:03:01.2 -- not a known variable star
12:41:12.12 +73:02:35.7 -- not a known variable star
12:41:37.94 +72:39:28.1 -- not a known variable star
12:41:38.63 +72:44:23.5 -- not a known variable star
12:41:39.35 +72:54:10.6 -- not a known variable star
12:41:58.30 +72:57:48.6 -- not a known variable star
12:41:58.81 +73:10:55.9 -- not a known variable star
12:42:13.46 +73:02:14.2 -- not a known variable star
12:42:14.72 +72:54:27.9 -- not a known variable star
12:42:14.93 +73:26:26.7 -- not a known variable star
12:42:15.51 +73:10:27.4 -- not a known variable star
12:42:23.11 +72:56:59.5 -- not a known variable star
12:42:32.14 +73:16:03.8 -- not a known variable star
12:43:15.10 +73:28:01.8 -- not a known variable star
12:43:48.66 +73:22:47.2 -- not a known variable star
12:44:07.35 +73:18:47.2 -- not a known variable star
12:44:20.10 +73:18:22.2 -- not a known variable star
12:44:20.69 +73:04:03.1 -- not a known variable star
12:44:23.09 +73:33:00.3 -- not a known variable star
12:44:45.40 +73:28:34.8 -- not a known variable star
12:45:16.50 +72:47:01.5 -- not a known variable star
12:45:47.38 +72:40:57.0 -- not a known variable star
12:45:53.95 +72:47:08.0 -- not a known variable star
12:45:58.85 +73:10:10.9 -- not a known variable star
12:46:02.58 +73:26:50.2 -- not a known variable star
12:46:13.38 +73:23:53.6 -- not a known variable star
12:46:24.81 +72:54:36.6 -- not a known variable star
12:46:55.10 +73:04:47.9 -- not a known variable star
12:46:58.60 +72:47:21.7 -- not a known variable star
12:47:02.63 +73:12:57.3 -- not a known variable star
12:47:27.60 +72:58:59.4 -- not a known variable star
12:47:42.19 +73:04:40.0 -- not a known variable star
12:47:50.85 +72:59:34.6 -- not a known variable star
12:47:59.90 +72:38:01.7 -- not a known variable star
12:48:07.67 +73:06:03.1 -- not a known variable star
12:48:18.74 +73:10:12.2 -- not a known variable star
12:48:33.08 +73:34:19.1 -- not a known variable star
12:48:40.12 +73:32:19.5 -- not a known variable star
12:48:42.43 +73:27:28.0 -- not a known variable star
12:48:47.38 +72:59:37.4 -- not a known variable star
12:48:57.79 +72:53:58.7 -- not a known variable star
12:49:00.94 +72:24:24.9 -- not a known variable star
12:49:02.47 +72:33:11.0 -- not a known variable star
12:49:05.93 +73:14:01.5 -- not a known variable star
12:49:08.21 +73:19:04.7 -- not a known variable star
12:49:19.04 +73:42:45.5 -- a known variable star
12:49:19.10 +73:14:08.8 -- not a known variable star
12:49:44.61 +73:08:59.7 -- not a known variable star
12:50:00.76 +72:46:21.6 -- not a known variable star
12:50:06.99 +72:56:48.7 -- not a known variable star
12:50:07.55 +72:52:27.4 -- not a known variable star
12:50:10.58 +73:36:21.6 -- not a known variable star
12:50:18.37 +72:36:12.5 -- not a known variable star
12:50:31.15 +73:11:01.3 -- not a known variable star
12:50:43.42 +72:45:48.8 -- not a known variable star
12:50:59.23 +72:44:33.4 -- not a known variable star
12:51:09.46 +72:54:30.7 -- not a known variable star
12:51:17.47 +73:31:33.0 -- not a known variable star
12:51:25.91 +72:45:38.4 -- not a known variable star
12:51:30.25 +73:37:03.7 -- not a known variable star
12:51:36.05 +72:53:33.5 -- not a known variable star
12:51:40.12 +73:07:19.8 -- not a known variable star
12:51:43.52 +72:36:44.3 -- not a known variable star
12:51:43.56 +73:19:25.6 -- not a known variable star
12:52:18.39 +73:31:17.5 -- not a known variable star
12:52:55.29 +72:50:35.1 -- not a known variable star
12:52:58.53 +72:33:10.8 -- not a known variable star
12:53:05.28 +73:01:37.1 -- not a known variable star
12:53:21.40 +72:25:56.1 -- not a known variable star
12:53:30.40 +73:30:54.2 -- not a known variable star
12:53:33.98 +72:58:24.2 -- not a known variable star
12:53:37.32 +73:38:13.3 -- not a known variable star
12:53:41.96 +72:51:35.4 -- not a known variable star
12:53:43.46 +73:41:35.5 -- not a known variable star
12:53:46.89 +72:39:27.3 -- not a known variable star
12:53:47.77 +73:06:29.5 -- not a known variable star
12:53:53.44 +73:27:44.7 -- not a known variable star
12:54:20.09 +72:46:51.1 -- not a known variable star
12:54:52.75 +72:45:42.9 -- not a known variable star
12:54:54.16 +72:37:19.8 -- not a known variable star
12:54:54.68 +73:09:36.4 -- not a known variable star
12:55:04.45 +72:47:32.2 -- not a known variable star
12:55:10.52 +72:36:54.7 -- not a known variable star
12:55:10.56 +73:41:29.7 -- not a known variable star
12:55:17.14 +73:24:59.2 -- not a known variable star
12:55:19.61 +73:11:10.9 -- not a known variable star
12:55:27.64 +73:34:50.8 -- not a known variable star
12:55:27.84 +72:59:31.0 -- not a known variable star
12:55:48.29 +72:45:00.8 -- not a known variable star
12:55:49.65 +73:55:36.1 -- not a known variable star
12:56:04.03 +73:44:00.0 -- not a known variable star
12:56:27.99 +72:42:58.8 -- not a known variable star
12:56:30.64 +72:54:58.5 -- not a known variable star
12:56:31.37 +73:20:25.1 -- not a known variable star
12:56:33.26 +73:10:21.6 -- not a known variable star
12:56:35.85 +73:05:53.9 -- not a known variable star
12:56:38.70 +72:33:07.3 -- not a known variable star
12:56:39.60 +73:24:41.5 -- not a known variable star
12:56:48.04 +73:24:02.2 -- not a known variable star
12:56:54.39 +73:23:00.8 -- not a known variable star
12:56:55.90 +72:43:26.2 -- not a known variable star
12:56:58.43 +72:04:42.6 -- not a known variable star
12:57:01.28 +72:31:02.8 -- not a known variable star
12:57:03.50 +73:13:07.1 -- not a known variable star
12:57:13.79 +72:39:06.6 -- not a known variable star
12:57:19.87 +72:31:46.3 -- not a known variable star
12:57:25.78 +73:24:36.7 -- not a known variable star
12:57:30.88 +73:39:04.8 -- not a known variable star
12:57:40.47 +73:42:17.3 -- not a known variable star
12:57:44.81 +73:14:08.2 -- not a known variable star
12:57:46.68 +73:39:23.0 -- not a known variable star
12:57:51.79 +72:37:22.5 -- not a known variable star
12:57:59.23 +72:27:33.7 -- not a known variable star
12:58:02.55 +72:22:52.0 -- not a known variable star
12:58:03.43 +72:40:46.8 -- not a known variable star
12:58:07.13 +72:57:47.8 -- not a known variable star
12:58:10.36 +72:28:01.6 -- not a known variable star
12:58:11.39 +72:24:21.6 -- not a known variable star
12:58:13.25 +72:07:39.4 -- not a known variable star
12:58:13.32 +72:32:40.1 -- a known variable star
12:58:13.32 +72:38:48.0 -- not a known variable star
12:58:14.71 +72:56:30.5 -- not a known variable star
12:58:19.98 +72:16:20.8 -- not a known variable star
12:58:30.58 +72:46:28.4 -- not a known variable star
12:58:30.90 +73:39:51.8 -- not a known variable star
12:58:33.33 +73:28:20.1 -- not a known variable star
12:58:42.59 +72:58:36.9 -- not a known variable star
12:58:42.80 +72:05:27.3 -- not a known variable star
12:58:57.08 +73:46:23.7 -- not a known variable star
12:59:01.22 +72:57:48.4 -- not a known variable star
12:59:09.66 +72:19:15.5 -- not a known variable star
12:59:18.43 +72:06:04.4 -- not a known variable star
12:59:18.60 +72:30:03.5 -- not a known variable star
12:59:27.31 +72:44:42.9 -- not a known variable star
12:59:27.94 +72:23:49.7 -- not a known variable star
12:59:29.29 +72:43:47.7 -- not a known variable star
12:59:36.62 +73:07:19.6 -- not a known variable star
12:59:42.36 +73:31:47.8 -- not a known variable star
12:59:44.93 +72:30:12.4 -- not a known variable star
12:59:48.61 +72:54:01.2 -- not a known variable star
12:59:55.35 +73:40:22.7 -- not a known variable star
12:59:58.49 +72:16:01.9 -- not a known variable star
13:00:01.80 +72:50:19.0 -- not a known variable star
13:00:02.15 +73:26:50.1 -- not a known variable star
13:00:03.31 +72:38:31.1 -- not a known variable star
13:00:06.20 +73:36:25.2 -- not a known variable star
13:00:10.37 +72:03:17.6 -- not a known variable star
13:00:11.37 +72:16:50.2 -- not a known variable star
13:00:16.10 +72:41:56.2 -- not a known variable star
13:00:17.61 +73:18:02.6 -- not a known variable star
13:00:19.85 +73:03:09.9 -- not a known variable star
13:00:22.15 +73:31:39.7 -- not a known variable star
13:00:41.05 +72:40:50.2 -- not a known variable star
13:00:41.70 +73:25:05.1 -- not a known variable star
13:00:49.89 +72:58:31.6 -- not a known variable star
13:01:01.23 +72:35:09.9 -- a known variable star
13:01:03.11 +72:18:20.9 -- not a known variable star
13:01:07.46 +72:00:39.1 -- not a known variable star
13:01:08.37 +72:19:37.4 -- not a known variable star
13:01:11.16 +73:48:31.4 -- not a known variable star
13:01:13.53 +72:36:59.1 -- not a known variable star
13:01:23.83 +73:19:03.4 -- not a known variable star
13:01:27.38 +72:29:55.0 -- not a known variable star
13:01:30.73 +73:04:14.0 -- not a known variable star
13:01:32.18 +72:37:38.2 -- not a known variable star
13:01:32.26 +72:59:58.2 -- not a known variable star
13:01:36.16 +73:35:42.3 -- not a known variable star
13:01:39.47 +72:18:56.2 -- not a known variable star
13:01:44.75 +72:30:31.8 -- not a known variable star
13:01:47.15 +72:18:24.1 -- not a known variable star
13:01:49.98 +73:05:38.2 -- not a known variable star
13:01:54.63 +73:25:18.7 -- not a known variable star
13:01:57.32 +72:14:01.6 -- not a known variable star
13:02:01.31 +73:04:44.8 -- not a known variable star
13:02:01.45 +73:17:18.6 -- not a known variable star
13:02:01.61 +73:01:21.9 -- not a known variable star
13:02:11.40 +72:52:54.1 -- not a known variable star
13:02:14.65 +73:06:46.4 -- not a known variable star
13:02:29.57 +73:12:00.8 -- not a known variable star
13:02:40.92 +72:44:20.7 -- not a known variable star
13:02:41.04 +73:16:08.6 -- not a known variable star
13:02:47.64 +72:20:36.7 -- not a known variable star
13:02:47.69 +72:07:41.9 -- not a known variable star
13:02:55.03 +72:18:40.8 -- not a known variable star
13:03:01.60 +72:23:53.6 -- not a known variable star
13:03:11.12 +72:22:32.4 -- not a known variable star
13:03:17.60 +73:14:32.6 -- not a known variable star
13:03:23.25 +73:20:26.6 -- not a known variable star
13:03:29.81 +72:40:31.1 -- not a known variable star
13:03:40.05 +72:56:33.0 -- a known variable star
13:03:42.54 +72:51:11.4 -- a known variable star
13:03:45.65 +73:15:30.2 -- not a known variable star
13:04:04.32 +72:11:18.2 -- not a known variable star
13:04:04.51 +73:30:49.2 -- not a known variable star
13:04:13.52 +73:26:41.2 -- not a known variable star
13:04:18.31 +71:56:04.9 -- not a known variable star
13:04:25.11 +72:51:34.8 -- not a known variable star
13:04:26.17 +73:14:02.6 -- not a known variable star
13:04:26.86 +72:50:34.0 -- not a known variable star
13:04:27.57 +72:47:52.2 -- not a known variable star
13:04:41.75 +73:27:59.1 -- not a known variable star
13:04:49.66 +73:10:44.9 -- not a known variable star
13:05:00.73 +72:02:27.4 -- not a known variable star
13:05:01.67 +72:01:12.2 -- not a known variable star
13:05:17.21 +72:58:12.6 -- not a known variable star
13:05:21.53 +72:25:45.3 -- not a known variable star
13:05:33.68 +72:16:21.0 -- not a known variable star
13:05:35.49 +72:36:10.2 -- not a known variable star
13:05:36.91 +72:15:20.6 -- not a known variable star
13:05:42.21 +72:16:06.7 -- not a known variable star
13:05:50.96 +73:04:52.6 -- not a known variable star
13:05:51.80 +72:56:33.8 -- not a known variable star
13:05:55.27 +72:05:29.6 -- not a known variable star
13:06:03.28 +72:30:52.9 -- not a known variable star
13:06:08.59 +72:20:50.3 -- not a known variable star
13:06:14.57 +73:00:50.9 -- not a known variable star
13:06:22.45 +73:06:01.7 -- not a known variable star
13:06:30.73 +72:08:40.3 -- not a known variable star
13:06:34.93 +72:25:03.3 -- not a known variable star
13:06:36.56 +72:49:26.6 -- not a known variable star
13:06:37.92 +71:49:10.7 -- not a known variable star
13:06:42.04 +72:40:56.5 -- not a known variable star
13:06:48.64 +72:26:55.8 -- not a known variable star
13:06:49.50 +72:59:51.6 -- not a known variable star
13:06:53.34 +71:45:28.9 -- not a known variable star
13:06:57.13 +73:02:16.2 -- not a known variable star
13:06:58.61 +71:54:42.0 -- not a known variable star
13:07:18.75 +72:22:07.7 -- not a known variable star
13:07:20.98 +72:44:49.8 -- not a known variable star
13:07:22.13 +72:19:13.5 -- not a known variable star
13:07:25.77 +72:39:06.8 -- not a known variable star
13:07:29.03 +73:10:26.5 -- not a known variable star
13:07:29.14 +72:31:57.2 -- not a known variable star
13:07:33.55 +72:54:30.0 -- not a known variable star
13:07:33.81 +72:21:04.7 -- not a known variable star
13:07:36.05 +72:24:14.1 -- not a known variable star
13:07:38.62 +72:57:40.7 -- not a known variable star
13:07:43.13 +72:45:32.8 -- not a known variable star
13:07:52.38 +72:45:41.7 -- not a known variable star
13:08:06.85 +72:26:10.3 -- not a known variable star
13:08:16.60 +72:54:34.7 -- not a known variable star
13:08:31.68 +72:09:36.8 -- not a known variable star
13:08:33.28 +72:39:18.9 -- not a known variable star
13:08:36.45 +72:34:01.6 -- not a known variable star
13:08:37.09 +72:31:21.5 -- a known variable star
13:08:39.58 +72:36:27.7 -- not a known variable star
13:09:22.55 +71:38:50.5 -- not a known variable star
13:09:23.80 +71:46:20.2 -- not a known variable star
13:09:35.39 +72:18:19.3 -- not a known variable star
13:09:38.74 +72:36:50.6 -- not a known variable star
13:09:41.33 +72:26:38.9 -- not a known variable star
13:09:49.33 +71:29:36.3 -- not a known variable star
13:09:52.90 +73:14:32.3 -- not a known variable star
13:09:59.18 +73:16:31.0 -- not a known variable star
13:10:07.70 +71:50:50.2 -- not a known variable star
13:10:07.76 +72:55:54.2 -- not a known variable star
13:10:18.32 +72:33:22.9 -- not a known variable star
13:10:21.41 +71:29:45.1 -- not a known variable star
13:10:21.80 +72:48:47.9 -- not a known variable star
13:10:26.21 +72:53:39.7 -- not a known variable star
13:10:44.22 +71:45:25.8 -- not a known variable star
13:10:52.40 +71:46:07.1 -- not a known variable star
13:10:56.33 +72:05:25.6 -- not a known variable star
13:11:07.42 +72:13:00.7 -- not a known variable star
13:11:09.70 +72:48:43.1 -- not a known variable star
13:11:11.35 +71:58:03.5 -- not a known variable star
13:11:25.29 +72:08:18.4 -- not a known variable star
13:11:26.71 +72:26:15.0 -- not a known variable star
13:11:40.69 +73:16:13.9 -- not a known variable star
13:11:44.00 +72:27:30.6 -- not a known variable star
13:11:46.15 +72:34:35.4 -- not a known variable star
13:11:49.43 +72:19:25.6 -- not a known variable star
13:12:08.64 +72:08:20.0 -- not a known variable star
13:12:11.60 +71:58:43.3 -- not a known variable star
13:12:12.08 +72:17:46.1 -- not a known variable star
13:12:16.25 +72:21:42.9 -- not a known variable star
13:12:34.00 +71:40:43.6 -- not a known variable star
13:12:34.95 +72:59:46.7 -- not a known variable star
13:12:36.34 +71:37:05.6 -- not a known variable star
13:12:39.08 +72:25:47.2 -- not a known variable star
13:12:40.00 +72:14:22.0 -- not a known variable star
13:12:41.18 +72:27:00.4 -- not a known variable star
13:12:59.50 +71:49:15.5 -- not a known variable star
13:13:03.94 +72:55:30.5 -- not a known variable star
13:13:05.96 +71:33:21.9 -- not a known variable star
13:13:17.73 +72:11:14.5 -- not a known variable star
13:13:30.12 +72:30:27.1 -- not a known variable star
13:13:31.62 +73:12:51.1 -- not a known variable star
13:13:32.47 +72:42:16.1 -- not a known variable star
13:13:41.66 +71:25:39.4 -- not a known variable star
13:13:45.43 +72:37:49.5 -- not a known variable star
13:13:50.51 +71:48:33.2 -- not a known variable star
13:13:55.31 +72:54:06.9 -- not a known variable star
13:14:05.78 +72:23:39.7 -- not a known variable star
13:14:05.92 +73:07:24.7 -- not a known variable star
13:14:10.04 +72:55:43.6 -- not a known variable star
13:14:10.93 +71:30:50.6 -- not a known variable star
13:14:17.41 +72:12:56.4 -- not a known variable star
13:14:20.50 +72:35:29.9 -- not a known variable star
13:14:32.87 +72:41:53.3 -- not a known variable star
13:14:45.15 +72:22:38.8 -- not a known variable star
13:14:51.04 +71:13:37.0 -- not a known variable star
13:14:57.57 +72:44:33.8 -- not a known variable star
13:14:57.95 +72:09:22.5 -- not a known variable star
13:14:58.52 +73:02:21.4 -- not a known variable star
13:15:02.19 +72:13:36.0 -- a known variable star
13:15:10.77 +71:35:10.6 -- not a known variable star
13:15:10.86 +72:52:25.2 -- not a known variable star
13:15:10.93 +71:40:05.6 -- a known variable star
13:15:15.15 +71:47:14.5 -- not a known variable star
13:15:16.78 +72:31:47.3 -- not a known variable star
13:15:22.53 +72:25:33.6 -- not a known variable star
13:15:22.65 +72:12:29.8 -- not a known variable star
13:15:25.65 +72:28:57.1 -- not a known variable star
13:15:32.61 +72:25:15.8 -- not a known variable star
13:15:36.74 +71:31:36.6 -- not a known variable star
13:15:46.85 +72:10:09.7 -- not a known variable star
13:15:47.45 +72:07:13.3 -- not a known variable star
13:15:56.81 +72:02:25.8 -- not a known variable star
13:15:58.55 +71:29:31.8 -- not a known variable star
13:16:09.04 +71:42:06.3 -- not a known variable star
13:16:11.35 +72:52:41.5 -- not a known variable star
13:16:26.32 +71:58:12.7 -- not a known variable star
13:16:27.07 +71:56:08.2 -- a known variable star
13:16:34.92 +72:40:37.4 -- not a known variable star
13:16:37.02 +72:38:14.7 -- not a known variable star
13:16:37.10 +72:17:29.9 -- not a known variable star
13:16:44.77 +71:50:45.0 -- not a known variable star
13:16:48.08 +71:47:22.9 -- not a known variable star
13:16:54.28 +72:37:21.5 -- a known variable star
13:16:59.46 +72:03:29.2 -- not a known variable star
13:17:03.17 +71:48:26.8 -- a known variable star
13:17:12.36 +71:49:01.2 -- not a known variable star
13:17:18.56 +71:47:13.1 -- not a known variable star
13:17:31.63 +72:07:02.2 -- not a known variable star
13:17:40.41 +72:20:00.1 -- not a known variable star
13:17:43.98 +71:18:39.2 -- not a known variable star
13:17:46.16 +71:43:15.4 -- not a known variable star
13:17:58.18 +71:50:32.8 -- not a known variable star
13:18:01.59 +72:23:16.1 -- not a known variable star
13:18:02.75 +71:58:55.7 -- not a known variable star
13:18:02.85 +71:49:01.7 -- not a known variable star
13:18:04.43 +72:06:32.9 -- not a known variable star
13:18:09.40 +72:43:37.2 -- not a known variable star
13:18:09.50 +71:49:40.9 -- not a known variable star
13:18:14.35 +72:23:50.7 -- not a known variable star
13:18:15.77 +72:31:25.4 -- not a known variable star
13:18:21.78 +72:43:44.6 -- not a known variable star
13:18:21.95 +72:06:23.4 -- not a known variable star
13:18:23.28 +72:39:40.8 -- not a known variable star
13:18:25.86 +71:56:30.8 -- not a known variable star
13:18:29.52 +72:49:05.2 -- not a known variable star
13:18:32.27 +71:51:10.9 -- not a known variable star
13:18:36.11 +72:54:37.6 -- not a known variable star
13:18:38.01 +72:55:44.6 -- not a known variable star
13:18:41.07 +72:34:08.8 -- not a known variable star
13:18:46.50 +71:40:22.8 -- a known variable star
13:18:56.85 +72:31:43.8 -- not a known variable star
13:18:59.42 +71:06:15.0 -- not a known variable star
13:19:01.41 +72:26:20.4 -- not a known variable star
13:19:02.60 +72:12:15.6 -- not a known variable star
13:19:07.73 +71:38:23.1 -- not a known variable star
13:19:13.86 +71:13:27.3 -- not a known variable star
13:19:14.09 +72:21:29.2 -- not a known variable star
13:19:24.05 +72:56:45.9 -- not a known variable star
13:19:28.26 +71:37:18.8 -- not a known variable star
13:19:33.78 +71:55:20.3 -- not a known variable star
13:19:37.39 +71:23:41.3 -- not a known variable star
13:19:40.86 +72:10:33.9 -- not a known variable star
13:19:41.36 +71:09:37.0 -- not a known variable star
13:19:41.80 +72:00:39.5 -- not a known variable star
13:19:44.06 +71:48:17.9 -- not a known variable star
13:19:44.63 +70:53:44.4 -- not a known variable star
13:19:51.40 +71:37:45.7 -- not a known variable star
13:19:53.73 +71:41:05.4 -- not a known variable star
13:19:54.31 +72:27:35.2 -- not a known variable star
13:19:54.76 +72:02:26.1 -- not a known variable star
13:19:56.41 +71:30:15.9 -- not a known variable star
13:20:06.04 +71:40:53.7 -- not a known variable star
13:20:10.61 +71:38:59.2 -- not a known variable star
13:20:15.34 +71:56:49.3 -- not a known variable star
13:20:15.71 +72:34:31.1 -- not a known variable star
13:20:36.16 +72:00:44.9 -- not a known variable star
13:20:38.91 +72:39:08.2 -- not a known variable star
13:20:46.11 +71:47:47.1 -- a known variable star
13:20:46.24 +72:50:03.0 -- not a known variable star
13:20:48.31 +70:58:12.0 -- not a known variable star
13:20:55.33 +71:03:56.8 -- not a known variable star
13:21:04.85 +71:24:56.5 -- not a known variable star
13:21:11.75 +72:24:54.3 -- not a known variable star
13:21:14.53 +71:48:45.1 -- a known variable star
13:21:16.99 +71:30:26.7 -- not a known variable star
13:21:17.88 +72:33:25.2 -- not a known variable star
13:21:19.87 +72:18:09.9 -- not a known variable star
13:21:23.84 +72:06:14.9 -- a known variable star
13:21:29.70 +72:15:42.4 -- not a known variable star
13:21:30.41 +71:27:07.9 -- not a known variable star
13:21:36.40 +71:58:07.4 -- not a known variable star
13:21:38.43 +72:25:09.0 -- not a known variable star
13:21:38.79 +72:22:17.3 -- not a known variable star
13:21:39.25 +71:43:36.0 -- not a known variable star
13:21:39.33 +71:41:36.8 -- not a known variable star
13:21:42.11 +71:49:32.8 -- a known variable star
13:21:49.45 +70:49:22.6 -- a known variable star
13:21:59.20 +71:34:54.7 -- not a known variable star
13:22:13.66 +71:33:59.2 -- not a known variable star
13:22:14.55 +71:53:42.1 -- not a known variable star
13:22:19.72 +71:26:12.9 -- not a known variable star
13:22:48.03 +72:00:00.3 -- not a known variable star
13:22:50.13 +72:28:43.5 -- not a known variable star
13:22:51.32 +72:33:44.9 -- not a known variable star
13:22:55.68 +72:32:11.9 -- not a known variable star
13:22:57.38 +71:26:45.7 -- not a known variable star
13:22:57.92 +71:04:38.9 -- not a known variable star
13:22:58.81 +71:33:49.3 -- not a known variable star
13:23:03.11 +72:12:04.0 -- not a known variable star
13:23:03.77 +72:21:31.9 -- not a known variable star
13:23:07.70 +71:31:41.0 -- not a known variable star
13:23:10.50 +72:08:04.6 -- not a known variable star
13:23:15.12 +72:02:51.7 -- not a known variable star
13:23:20.53 +72:39:07.6 -- not a known variable star
13:23:26.11 +71:20:57.7 -- not a known variable star
13:23:26.14 +71:25:54.5 -- not a known variable star
13:23:33.99 +71:14:51.7 -- not a known variable star
13:23:48.95 +71:20:01.3 -- not a known variable star
13:23:54.43 +71:33:11.7 -- not a known variable star
13:23:59.13 +71:50:27.0 -- not a known variable star
13:24:01.15 +71:55:46.8 -- not a known variable star
13:24:02.37 +72:15:55.0 -- not a known variable star
13:24:12.23 +70:57:15.2 -- not a known variable star
13:24:14.75 +72:35:07.8 -- not a known variable star
13:24:16.16 +71:30:22.0 -- not a known variable star
13:24:19.97 +72:16:40.8 -- not a known variable star
13:24:28.41 +72:43:10.4 -- not a known variable star
13:24:46.70 +71:35:06.3 -- not a known variable star
13:24:51.51 +72:16:27.4 -- not a known variable star
13:24:56.71 +72:31:35.0 -- not a known variable star
13:25:00.45 +71:26:31.6 -- not a known variable star
13:25:07.60 +71:30:29.7 -- not a known variable star
13:25:08.75 +70:54:00.5 -- not a known variable star
13:25:21.16 +72:46:50.2 -- not a known variable star
13:25:23.90 +72:27:25.4 -- not a known variable star
13:25:30.35 +72:11:17.3 -- not a known variable star
13:25:31.63 +70:40:09.0 -- not a known variable star
13:25:33.26 +70:55:51.6 -- not a known variable star
13:25:38.02 +70:53:08.5 -- a known variable star
13:25:41.60 +70:54:24.1 -- not a known variable star
13:25:49.95 +71:19:29.6 -- not a known variable star
13:25:51.17 +72:01:49.7 -- not a known variable star
13:26:01.91 +71:22:30.4 -- not a known variable star
13:26:05.25 +72:26:40.0 -- not a known variable star
13:26:06.62 +70:54:58.2 -- not a known variable star
13:26:11.11 +72:28:30.5 -- not a known variable star
13:26:11.69 +71:43:24.4 -- not a known variable star
13:26:16.50 +71:23:52.9 -- not a known variable star
13:26:30.90 +72:01:59.4 -- not a known variable star
13:26:39.43 +71:55:52.2 -- not a known variable star
13:26:41.44 +70:49:07.7 -- not a known variable star
13:26:50.22 +71:29:45.5 -- not a known variable star
13:26:52.74 +72:29:14.7 -- a known variable star
13:27:03.84 +71:21:44.7 -- not a known variable star
13:27:04.28 +72:07:49.8 -- not a known variable star
13:27:08.57 +72:23:21.6 -- not a known variable star
13:27:09.45 +71:37:01.0 -- not a known variable star
13:27:29.93 +71:42:32.6 -- not a known variable star
13:27:33.94 +71:46:45.9 -- not a known variable star
13:27:35.12 +71:57:24.0 -- not a known variable star
13:27:37.84 +71:47:18.5 -- not a known variable star
13:27:38.60 +72:38:45.3 -- a known variable star
13:27:41.73 +72:08:56.9 -- a known variable star
13:27:45.33 +72:42:13.4 -- not a known variable star
13:27:49.33 +71:38:22.9 -- not a known variable star
13:28:02.22 +71:33:15.8 -- not a known variable star
13:28:10.62 +71:35:05.1 -- not a known variable star
13:28:19.69 +71:29:48.9 -- not a known variable star
13:28:19.91 +71:48:42.0 -- not a known variable star
13:28:20.72 +71:55:35.1 -- not a known variable star
13:28:23.40 +72:16:58.8 -- not a known variable star
13:28:23.57 +70:39:09.1 -- not a known variable star
13:28:28.14 +71:51:10.9 -- not a known variable star
13:28:28.78 +72:14:26.9 -- not a known variable star
13:28:32.66 +70:44:48.1 -- not a known variable star
13:28:32.68 +71:45:48.2 -- not a known variable star
13:28:38.58 +71:33:53.7 -- not a known variable star
13:28:43.51 +71:22:13.7 -- not a known variable star
13:28:48.74 +71:58:22.8 -- not a known variable star
13:28:50.89 +72:13:38.2 -- not a known variable star
13:28:54.98 +72:25:59.5 -- not a known variable star
13:29:09.79 +72:14:06.7 -- not a known variable star
13:29:10.08 +72:02:46.5 -- not a known variable star
13:29:14.34 +72:06:34.7 -- not a known variable star
13:29:17.60 +71:21:49.5 -- not a known variable star
13:29:23.30 +71:07:50.6 -- not a known variable star
13:29:26.24 +71:09:19.0 -- not a known variable star
13:29:32.39 +71:37:49.6 -- not a known variable star
13:29:41.97 +71:38:00.1 -- not a known variable star
13:29:43.86 +71:43:13.0 -- not a known variable star
13:29:49.76 +70:39:17.3 -- not a known variable star
13:30:10.78 +70:33:21.9 -- not a known variable star
13:30:17.47 +70:48:43.0 -- not a known variable star
13:30:18.59 +72:11:50.2 -- not a known variable star
13:30:29.24 +72:00:25.8 -- not a known variable star
13:30:34.13 +70:47:33.1 -- not a known variable star
13:30:35.62 +72:05:15.3 -- a known variable star
13:30:39.53 +72:06:57.0 -- not a known variable star
13:30:42.83 +71:36:15.4 -- not a known variable star
13:31:08.93 +71:54:52.0 -- not a known variable star
13:31:21.37 +71:29:17.8 -- not a known variable star
13:31:30.72 +71:01:18.8 -- not a known variable star
13:31:33.28 +72:04:33.9 -- not a known variable star
13:31:41.01 +72:09:42.0 -- not a known variable star
13:31:41.30 +70:58:43.2 -- a known variable star
13:31:41.82 +71:09:49.5 -- not a known variable star
13:31:47.08 +71:30:01.6 -- not a known variable star
13:31:48.45 +71:15:56.7 -- not a known variable star
13:31:53.93 +72:18:53.8 -- not a known variable star
13:32:08.94 +71:25:13.3 -- not a known variable star
13:32:11.93 +70:52:05.7 -- a known variable star
13:32:13.19 +71:33:08.7 -- not a known variable star
13:32:14.74 +72:16:35.6 -- not a known variable star
13:32:15.12 +72:06:01.5 -- not a known variable star
13:32:16.86 +71:26:19.0 -- not a known variable star
13:32:26.42 +71:26:46.4 -- not a known variable star
13:32:34.71 +72:01:22.6 -- not a known variable star
13:32:39.82 +72:03:58.1 -- not a known variable star
13:32:41.35 +70:58:12.1 -- not a known variable star
13:32:42.39 +71:06:13.9 -- not a known variable star
13:32:43.17 +71:44:41.0 -- not a known variable star
13:32:45.22 +72:24:54.7 -- not a known variable star
13:32:54.13 +72:02:59.2 -- not a known variable star
13:32:57.25 +72:14:56.1 -- not a known variable star
13:33:04.68 +72:21:22.5 -- not a known variable star
13:33:08.25 +70:43:28.4 -- not a known variable star
13:33:28.39 +72:24:10.2 -- not a known variable star
13:33:35.69 +71:50:20.1 -- not a known variable star
13:33:40.87 +71:40:50.5 -- not a known variable star
13:33:41.75 +72:13:21.9 -- not a known variable star
13:33:55.24 +71:21:23.3 -- not a known variable star
13:34:09.85 +70:52:16.0 -- not a known variable star
13:34:11.36 +71:38:15.8 -- not a known variable star
13:34:15.26 +71:33:17.2 -- not a known variable star
13:34:15.49 +72:07:44.6 -- not a known variable star
13:34:29.57 +71:15:58.4 -- not a known variable star
13:34:39.39 +70:31:39.6 -- not a known variable star
13:34:40.95 +71:34:31.7 -- not a known variable star
13:34:47.19 +71:51:11.5 -- not a known variable star
13:34:51.12 +70:39:22.9 -- not a known variable star
13:34:59.54 +71:46:21.3 -- not a known variable star
13:35:04.47 +70:56:11.1 -- not a known variable star
13:35:06.68 +71:37:16.2 -- not a known variable star
13:35:11.50 +70:45:22.3 -- not a known variable star
13:35:24.47 +71:05:40.9 -- not a known variable star
13:35:24.95 +72:17:30.1 -- not a known variable star
13:35:27.28 +70:59:16.7 -- not a known variable star
13:35:27.73 +71:16:15.3 -- not a known variable star
13:35:29.66 +71:23:40.1 -- not a known variable star
13:35:52.59 +71:40:36.9 -- not a known variable star
13:35:54.74 +71:15:19.2 -- not a known variable star
13:36:03.99 +70:46:41.7 -- not a known variable star
13:36:15.70 +71:16:33.1 -- not a known variable star
13:36:16.68 +71:41:24.7 -- not a known variable star
13:36:22.02 +70:31:25.0 -- not a known variable star
13:36:35.78 +71:56:58.8 -- not a known variable star
13:36:41.40 +71:23:59.0 -- not a known variable star
13:36:46.97 +70:23:25.7 -- not a known variable star
13:36:53.39 +72:04:01.7 -- not a known variable star
13:36:55.68 +71:52:42.9 -- not a known variable star
13:37:37.74 +71:39:49.9 -- not a known variable star
13:37:38.92 +71:42:32.2 -- not a known variable star
13:37:40.30 +71:23:59.4 -- not a known variable star
13:37:44.01 +71:56:18.1 -- not a known variable star
13:38:05.54 +71:09:31.5 -- not a known variable star
13:38:08.95 +71:03:09.2 -- not a known variable star
13:38:18.10 +71:59:08.1 -- not a known variable star
13:38:25.39 +71:21:43.9 -- not a known variable star
13:38:35.67 +71:01:20.0 -- not a known variable star
13:39:02.21 +71:46:34.8 -- not a known variable star
13:39:12.41 +71:14:33.8 -- not a known variable star
13:39:16.57 +70:16:48.5 -- not a known variable star
13:39:22.44 +71:07:42.1 -- not a known variable star
13:39:59.05 +71:25:10.6 -- not a known variable star
13:40:12.72 +71:01:57.3 -- not a known variable star
13:40:17.14 +71:20:14.4 -- not a known variable star
13:41:15.65 +71:45:19.4 -- not a known variable star
13:41:40.94 +71:00:43.9 -- not a known variable star
13:41:41.88 +71:05:34.0 -- not a known variable star
13:44:18.13 +71:01:29.2 -- not a known variable star
13:44:18.84 +70:54:55.5 -- not a known variable star
13:57:59.75 +65:11:33.9 -- not a known variable star
13:59:20.65 +65:04:45.3 -- not a known variable star
14:39:51.55 +74:45:02.0 -- a known variable star
15:24:45.65 +66:30:17.5 -- not a known variable star
15:25:13.93 +66:40:57.3 -- not a known variable star
15:26:36.25 +66:47:00.3 -- a known variable star
15:26:38.72 +66:13:52.6 -- not a known variable star
15:26:54.39 +66:13:17.5 -- not a known variable star
15:27:00.65 +66:36:15.0 -- not a known variable star
15:27:01.80 +66:33:21.5 -- not a known variable star
15:27:08.39 +66:24:52.0 -- not a known variable star
15:28:35.36 +66:28:09.1 -- not a known variable star
15:28:43.89 +66:32:41.9 -- not a known variable star
15:28:55.94 +66:26:17.9 -- not a known variable star
15:28:57.10 +66:27:31.1 -- a known variable star
15:29:40.01 +66:22:09.7 -- not a known variable star
15:30:26.56 +65:59:47.7 -- not a known variable star
15:30:30.75 +65:56:33.3 -- not a known variable star
15:30:36.25 +66:16:20.0 -- not a known variable star
15:31:51.21 +65:47:40.0 -- a known variable star
15:32:04.15 +66:44:42.6 -- not a known variable star
15:33:00.32 +66:46:59.1 -- not a known variable star
15:33:02.87 +65:39:21.6 -- not a known variable star
15:33:52.91 +66:43:08.2 -- not a known variable star
15:34:06.07 +65:42:32.3 -- not a known variable star
15:34:39.02 +65:26:07.3 -- not a known variable star
15:34:41.44 +66:38:48.3 -- not a known variable star
15:34:42.38 +66:40:58.8 -- not a known variable star
15:34:52.40 +65:39:51.3 -- not a known variable star
15:35:55.99 +66:40:56.0 -- not a known variable star
15:36:12.29 +65:44:49.7 -- not a known variable star
15:36:58.16 +65:28:47.1 -- not a known variable star
15:37:01.65 +65:32:17.8 -- not a known variable star
15:38:50.47 +66:21:18.4 -- not a known variable star
15:38:54.93 +66:17:18.3 -- not a known variable star
Found 604 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
632 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 632 (excluding asteroids and hot pixels, 604 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461335.67896167 -observatory V36
15:07:55.19 -20:51:04.4 Mercury (0.3mag)
13:47:43.26 -18:24:45.1 Venus (-4.2mag)
09:04:09.09 +18:12:36.0 Mars (1.0mag)
09:40:52.22 +14:35:08.9 Jupiter (-2.0mag)
00:39:26.59 +01:18:23.8 Saturn (0.4mag)
04:10:48.37 +20:54:42.7 Uranus (5.6mag)
00:09:20.13 -00:32:02.6 Neptune (7.7mag)
20:24:11.14 -23:43:02.0 Pluto (14.5mag)
22:36:23.17 -08:21:44.2 Moon (-11.4mag)
-rw-r--r-- 1 apache apache 362 Oct 21 23:20 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461335.67896167:
09:40:46.38 +14:35:42.5 Io (6.1mag)
09:41:02.84 +14:34:09.6 Europa (6.2mag)
09:40:38.33 +14:36:28.3 Ganymede (5.5mag)
09:40:57.63 +14:34:41.0 Callisto (6.8mag)
09:41:25.54 +14:51:39.3 Himalia (15.6mag)
09:40:49.23 +14:35:25.5 Thebe (16.4mag)
09:39:58.27 +14:58:53.9 Elara (17.5mag)
09:42:34.75 +13:59:20.2 Pasiphae (17.8mag)
09:38:42.89 +15:04:45.5 Carme (18.8mag)
00:39:35.39 +01:18:25.6 Titan (8.2mag)
00:39:19.68 +01:18:22.1 Rhea (9.6mag)
00:39:25.33 +01:16:32.9 Iapetus (11.0mag)
00:39:42.30 +01:18:08.5 Hyperion (14.1mag)
00:37:41.71 +01:05:58.9 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Oct 21 23:20 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461335.67896167:
03:49:06.31 +20:04:18.0 JWST
17:27:20.04 +36:12:03.8 Chandra
05:54:29.89 +31:00:00.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Oct 21 23:20 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461335.67896167 -observatory V36
03:41:38.14 +20:09:36.4 17.1mag P/1996 R2 (Lagerkvist)
07:41:38.21 +37:33:53.6 18.0mag P/2004 V5 (LINEAR-Hill)
07:41:43.23 +37:33:40.9 18.0mag P/2004 V5-A (LINEAR-Hill)
07:41:04.11 +37:33:53.3 18.0mag P/2004 V5-B (LINEAR-Hill)
05:02:27.21 +40:52:11.2 17.9mag P/2009 Y2 (Kowalski)
18:34:59.80 -33:13:33.8 14.9mag P/2010 H2 (Vales)
07:43:22.57 -73:06:48.4 17.2mag C/2014 UN271 (Bernardinelli-Bernstein)
06:14:15.41 +34:57:49.2 17.7mag C/2017 K2 (PANSTARRS)
04:40:53.77 +48:11:18.0 17.6mag P/2021 N1 (ZTF)
07:33:39.15 +25:22:24.9 16.9mag C/2022 N2 (PANSTARRS)
09:06:10.07 +36:54:02.0 16.3mag C/2024 E1 (Wierzchos)
18:30:16.03 +41:07:07.7 17.4mag C/2024 J3 (ATLAS)
05:45:50.65 -13:39:59.6 16.5mag C/2024 T5 (ATLAS)
12:37:41.17 +15:07:05.4 16.0mag C/2025 V2 (Rankin)
14:02:06.54 -03:36:45.3 16.4mag C/2025 Y1 (ATLAS)
19:26:51.36 +60:17:02.4 15.5mag C/2026 A2 (Bok)
02:23:53.01 +41:32:46.2 18.0mag C/2026 B2 (Sun-Gao)
12:56:00.34 +15:25:34.0 17.7mag A/2026 E1
16:23:57.81 -52:11:07.0 13.6mag P/2026 R2 (Leonard)
19:22:52.83 -05:06:11.9 16.6mag P/2026 T1 (ATLAS)
23:59:26.35 +17:02:02.6 17.2mag 2P/Encke
23:10:45.57 -29:06:07.5 14.9mag 10P/Tempel
02:25:09.34 +35:59:17.4 16.5mag 11P/Tempel-Swift-LINEAR
12:18:22.33 -09:02:37.8 16.3mag 29P/Schwassmann-Wachmann
00:16:05.08 -09:04:45.5 15.7mag 65P/Gunn
07:48:50.47 +14:51:18.6 13.9mag 78P/Gehrels
02:48:26.47 +13:45:48.9 17.8mag 88P/Howell
08:17:54.71 +43:07:36.5 17.0mag 112P/Urata-Niijima
09:26:42.90 +10:12:20.6 17.7mag 114P/Wiseman-Skiff
12:02:52.60 +10:47:49.7 14.8mag 123P/West-Hartley
14:34:23.93 -35:08:35.2 18.0mag 124P/Mrkos
20:29:44.24 +10:12:08.3 9.8mag 161P/Hartley-IRAS
10:44:54.65 -00:45:00.2 15.2mag 169P/NEAT
03:21:51.30 +03:18:40.3 15.0mag 220P/McNaught
06:16:38.56 +47:28:55.4 15.5mag 260P/McNaught
07:42:23.68 +25:20:34.1 17.7mag 266P/Christensen
-rw-r--r-- 1 apache apache 1.8K Oct 21 23:20 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
22:14:03.37 -45:07:18.60 ASASSN-26fm VIZIER
01:57:48.19 -33:14:42.30 SN 2026aedl -------
18:05:22.06 +17:52:41.00 ASASSN-26fn 2026-10-11.74 15.23
21:50:55.86 -02:51:49.30 SN2026acyb 2026-10-9.85 16.83
03:40:34.04 +02:31:56.70 SN2026acvp 2026-10-9.95 17.75
04:33:25.91 -13:41:04.20 SN2026adhl -------
09:20:05.05 +27:03:12.40 SN2026aeif -------
02:58:07.77 -65:18:52.90 ASASSN-26fl VIZIER
02:49:03.98 -49:55:57.00 SN 2026adfy 2026-10-4.88 16.61
22:03:46.31 -11:07:57.70 AT2026adgn 2026-10-4.28 -2.56
15:03:12.98 +49:51:05.40 ASASSN-26fj VIZIER
08:07:27.96 -65:51:03.90 ASASSN-26fi 2026-10-1.36 15.82
21:02:34.66 +23:57:26.20 ASASSN-26fh 2026-10-1.27 15.94
20:00:16.62 +03:26:29.90 AT2026adfv -------
00:08:42.74 -32:33:16.50 SN2026abhc -------
21:02:30.26 -19:27:41.80 SN2026acxa -------
04:39:17.45 -28:06:12.40 ASASSN-26fg VIZIER
05:25:07.80 +04:38:32.40 SN2026aajs -------
19:56:12.67 +08:25:27.70 AT2026acgs -------
00:02:34.06 +52:55:18.90 ASASSN-26ff 2026-09-16.38 15.41
23:44:33.18 +17:46:12.20 SN2026yjv -------
16:21:12.24 +57:37:51.30 SN 2026aafh -------
23:36:00.27 -19:28:18.00 SN 2026aaks 2026-09-14.44 16.89
16:35:24.86 -05:32:38.20 SN2026aasi -------
16:46:08.71 +37:25:21.80 SN2026aafk 2026-09-13.25 17.4
23:48:37.86 +50:25:24.60 SN2026aafs -------
21:20:27.02 +02:10:42.50 SN2026aagh -------
08:02:26.85 -24:37:44.10 ASASSN-26fe 2026-09-13.34 13.67
02:29:34.91 +23:06:56.30 SN2026aars -------
02:47:25.52 -32:58:34.50 SN 2026znh -------
04:59:14.53 -83:27:58.80 ASASSN-26fd 2026-09-9.11 17.27
17:52:06.79 -23:43:20.70 ASASSN-26fc VIZIER
03:52:53.26 -14:19:28.70 SN 2026zfw -------
01:53:26.46 +10:07:25.10 SN2026aacj -------
20:04:34.47 +62:38:38.10 SN2026zji 2026-09-7.14 15.87
22:37:05.64 +34:24:35.00 SN2026aaiv -------
22:24:21.29 -10:25:31.60 ASASSN-26fb 2026-09-5.3 13.93
00:44:54.28 +41:33:10.50 AT2026aabo 2026-09-3.29 15.02
00:52:12.40 -58:22:08.60 SN 2026zhl 2026-08-31.92 16.51
19:53:57.87 +61:00:19.70 ASASSN-26fa VIZIER
00:21:50.96 -09:29:16.30 AT2026zwp 2026-08-31.41 15.59
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 -------
17:17:45.96 +64:31:40.10 ASASSN-26ez VIZIER
19:02:47.09 +58:08:21.00 AT2026zwo -------
04:20:07.58 -42:26:59.90 AT2026zjy -------
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid -------
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn -------
23:01:28.67 -61:00:39.00 SN 2026yib -------
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew VIZIER
13:53:14.21 +00:26:52.00 SN 2026wkv -------
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau -------
01:10:22.05 -09:34:08.50 SN2026weo -------
00:56:54.35 -35:55:29.40 AT2026wdy -------
22:08:07.63 -53:03:58.90 AT2026wek -------
14:51:51.34 +66:13:24.60 ASASSN-26ev VIZIER
12:06:50.79 -36:16:06.20 SN2026wgm -------
16:56:36.90 -59:29:26.00 ASASSN-26er VIZIER
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep VIZIER
12:18:47.98 -30:48:47.50 ASASSN-26et VIZIER
13:00:47.82 +15:42:17.60 SN2026uwk -------
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu VIZIER
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo VIZIER
04:50:01.03 -02:22:33.80 ASASSN-26ej VIZIER
18:34:55.28 -31:41:00.90 ASASSN-26ek VIZIER
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei VIZIER
10:00:46.44 -32:36:31.10 AT 2023mhb -------
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh VIZIER
19:33:53.06 -07:15:00.80 ASASSN-22le -------
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb -------
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil -------
20:21:30.50 -32:03:40.10 ASASSN-26ee VIZIER
19:37:44.09 -05:35:42.80 AT2026ryu -------
11:06:55.46 -04:07:04.50 AT2026qqg -------
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea VIZIER
19:59:01.43 -32:07:34.30 ASASSN-26eb VIZIER
18:46:50.35 -57:44:13.20 SN 2026qqp -------
19:17:31.69 -39:55:29.90 ASASSN-26dz VIZIER
-rw-r--r-- 1 apache apache 9.3K Oct 21 23:20 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
00:42:12.76 +41:16:28.4 PNV J00421276+4116284 2026-09-10.9176 18.67Cmag
17:52:06.80 -23:43:20.7 TCP J17520680-2343207 2026-09-08.7896 12.6mag
00:42:40.94 +41:15:37.1 PNV J00424094+4115371 2026-09-17.8925 18.3mag
08:49:20.13 -09:19:15.8 TCP J08492013-0919158 2026-09-18.4698 13.3mag
00:42:13.93 +41:16:35.6 PNV J00421393+4116356 2026-09-22.6597 19.66Cmag
18:14:01.58 +15:13:55.5 TCP J18140158+1513555 2026-09-24.4645 14.1mag
00:42:36.61 +41:13:50.5 TCP J00423661+4113505 2026-09-29.7462 17.4mag
22:03:46.29 -11:07:57.8 TCP J22034629-1107578 2026-09-29.7438 14.51Cmag
22:05:02.06 +20:49:01.2 TCP J22050206+2049012 2026-10-03.5715 17.13Cmag
00:38:15.01 +41:14:47.2 TCP J00381501+4114472 2026-10-08.5978 17.72Cmag
01:06:05.83 +09:51:20.4 TCP J01060583+0951204 2026-10-10.8543 14.54Cmag
17:54:18.76 -27:36:36.2 TCP J17541876-2736362 2026-10-12.3993 10.8mag
09:56:00.79 +69:06:15.2 PNV J09560079+6906152 2026-10-14.9274 19.38Cmag
00:43:30.83 +41:26:55.3 PNV J00433083+4126553 2026-10-17.5651 18.61Cmag
04:57:32.08 +30:15:41.6 TCP J04573208+3015416 2026-10-17.7818 18.21Cmag
05:21:07.64 +23:38:21.3 TCP J05210764+2338213 2026-10-18.4020 10.3mag
05:34:11.01 +28:45:30.5 TCP J05341101+2845305 2026-10-18.3604 16.6mag
-rw-r--r-- 1 apache apache 191K Oct 21 23:20 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
01:10:49.770 +02:38:30.67 AT 2026aebt 2026-09-30.66 21.23
01:05:19.330 -00:11:32.74 AT 2026aebs 2026-09-30.65 21.65
01:35:09.144 -01:03:49.94 AT 2026aebr 2026-09-20.83 23.01
01:02:37.840 +04:28:02.19 AT 2026aebq 2026-09-20.82 22.78
01:28:12.190 +05:17:51.61 AT 2026aebp 2026-09-13.85 22.41
22:47:15.050 +03:42:02.27 AT 2026aebo 2026-09-21.73 22.04
23:45:08.040 +01:05:55.47 AT 2026aebn 2026-09-30.76 21.95
23:25:27.380 -00:44:47.15 AT 2026aebm 2026-09-15.74 22.29
00:43:52.136 -04:09:35.26 SN 2026aebl 2026-09-20.33 20.4818
23:57:05.580 +47:22:43.66 AT 2026aebk 2026-10-02.25 20.1485
21:45:41.050 -07:03:45.02 SN 2026aebj 2026-10-02.17 19.9213
01:27:33.024 +84:50:25.70 AT 2026aebi 2026-10-03.20 19.7953
00:26:39.140 -03:17:00.58 AT 2026aebh 2026-10-02.27 20.1095
21:28:41.378 +03:57:48.01 SN 2026aebg 2026-10-01.26 20.3099
00:57:54.471 -27:53:53.62 AT 2026aebf 2026-09-30.33 19.3916
22:47:58.650 +03:51:05.09 AT 2026aebe 2026-09-30.23 20.1921
23:27:00.498 -10:43:55.07 AT 2026aebd 2026-10-01.39 20.03
23:40:24.092 -09:27:20.60 AT 2026aebc 2026-10-01.39 20.07
00:56:09.593 -01:35:47.87 AT 2026aebb 2026-10-01.40 20.95
01:31:39.979 -01:39:43.87 AT 2026aeba 2026-10-01.46 21.45
-rw-r--r-- 1 apache apache 89K Oct 21 23:20 tns_transients_list.txt
