This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Lyn-02-Q1b1x1_232445_TTUQ1b1x1_306739_sGz00Y8F
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 06 08.1803 2461199.6803 11.30 07:41:29.79 +54:55:00.1
162.81424 28.94590 galactic Lyn Second-epoch detections are separated by 2.3" and 5.4 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 985801028585303424 | 07:41:29.74 +54:54:60.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.457+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:29.79 +54:55:00.1: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:29.79 +54:55:00.1: 12.60 +/- 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 985801028585303424,2461199.6803,11.30,0.05,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 985801028585303424 20260608.1803 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 06 08.1803 2461199.6803 11.27 08:24:00.81 +54:08:22.1
164.08669 35.06247 galactic Lyn Second-epoch detections are separated by 0.8" and 4.6 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 1032104005851151360 | 08:24:00.76 +54:08:21.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.328+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:00.81 +54:08:22.1: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:00.81 +54:08:22.1: 12.44 +/- 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 1032104005851151360,2461199.6803,11.27,0.05,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 1032104005851151360 20260608.1803 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 06 08.1803 2461199.6803 11.33 08:23:32.17 +54:14:46.8
163.95790 34.99055 galactic Lyn Second-epoch detections are separated by 0.0" and 4.8 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 | ATO J125.8834+54.2504 | 08:23:32.15 +54:14:47.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.363+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:32.17 +54:14:46.8: 16.33 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:32.17 +54:14:46.8: 12.47 +/- 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
ATO J125.8834+54.2504,2461199.6803,11.33,0.05,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
ATO J125.8834+54.2504 20260608.1803 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 06 08.1803 2461199.6803 11.74 07:40:04.76 +55:03:36.6
162.62359 28.76146 galactic Lyn Second-epoch detections are separated by 0.9" and 5.3 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 | 07:40:04.76 +55:03:36.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.258+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:04.76 +55:03:36.6: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:04.76 +55:03:36.6: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 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,2461199.6803,11.74,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.62 08:25:03.71 +53:28:32.5
164.89496 35.22901 galactic Lyn Second-epoch detections are separated by 4.0" and 4.1 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 | 08:25:03.71 +53:28:32.5 (user input) | T | P | (position from user input) J-Ks=0.562+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:03.71 +53:28:32.5: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:03.71 +53:28:32.5: 12.91 +/- 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,2461199.6803,11.62,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.03 08:23:51.64 +53:44:49.9
164.56629 35.04678 galactic Lyn Second-epoch detections are separated by 0.8" and 4.8 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 | Gaia DR3 1031995600876344832 | 08:23:51.63 +53:44:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.689+/-0.032 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:51.64 +53:44:49.9: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:51.64 +53:44:49.9: 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 1031995600876344832,2461199.6803,11.03,0.05,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 1031995600876344832 20260608.1803 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 06 08.1803 2461199.6803 11.88 07:37:29.78 +55:13:06.1
162.39181 28.41528 galactic Lyn Second-epoch detections are separated by 4.1" and 4.6 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 | 07:37:29.78 +55:13:06.1 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.363+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:29.78 +55:13:06.1: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:29.78 +55:13:06.1: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 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,2461199.6803,11.88,0.05,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
target 20260608.1803 11.88CV 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 06 08.1803 2461199.6803 11.45 08:25:57.72 +54:29:22.2
163.64955 35.33755 galactic Lyn Second-epoch detections are separated by 1.0" and 4.6 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 1032135552386377984 | 08:25:57.68 +54:29:21.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.282+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:57.72 +54:29:22.2: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:57.72 +54:29:22.2: 12.47 +/- 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 1032135552386377984,2461199.6803,11.45,0.05,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
Gaia DR3 1032135552386377984 20260608.1803 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 06 08.1803 2461199.6803 11.56 07:40:03.23 +55:00:00.4
162.69106 28.75046 galactic Lyn Second-epoch detections are separated by 0.2" and 5.1 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 | 07:40:03.23 +55:00:00.4 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.467+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:03.23 +55:00:00.4: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:03.23 +55:00:00.4: 13.01 +/- 0.02 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,2461199.6803,11.56,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.48 08:30:35.78 +52:40:01.8
165.86898 36.07656 galactic Lyn Second-epoch detections are separated by 1.5" and 4.7 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 1028835574394609792 | 08:30:35.74 +52:40:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.628+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:30:35.78 +52:40:01.8: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:30:35.78 +52:40:01.8: 12.54 +/- 0.01 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 1028835574394609792,2461199.6803,11.48,0.05,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 1028835574394609792 20260608.1803 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 06 08.1803 2461199.6803 11.55 08:16:57.81 +54:01:28.8
164.23461 34.02937 galactic Lyn Second-epoch detections are separated by 1.6" and 4.7 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 1032240276573659520 | 08:16:57.75 +54:01:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.311+/-0.029 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:16:57.81 +54:01:28.8: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:16:57.81 +54:01:28.8: 12.52 +/- 0.01 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 1032240276573659520,2461199.6803,11.55,0.05,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
Gaia DR3 1032240276573659520 20260608.1803 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 06 08.1803 2461199.6803 11.71 07:39:09.96 +55:47:49.8
161.77134 28.72178 galactic Lyn Second-epoch detections are separated by 2.1" and 5.2 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 | 07:39:09.96 +55:47:49.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.674+/-0.032 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:09.96 +55:47:49.8: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:09.96 +55:47:49.8: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 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,2461199.6803,11.71,0.05,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
target 20260608.1803 11.71CV 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 06 08.1803 2461199.6803 11.52 07:51:21.45 +52:58:24.8
165.22065 30.16998 galactic Lyn Second-epoch detections are separated by 1.2" and 5.0 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 | ATO J117.8387+52.9695 | 07:51:21.45 +52:58:24.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F3 (LAMOST DR5) J-Ks=0.279+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:51:21.45 +52:58:24.8: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:51:21.45 +52:58:24.8: 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
ATO J117.8387+52.9695,2461199.6803,11.52,0.05,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
ATO J117.8387+52.9695 20260608.1803 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 06 08.1803 2461199.6803 10.38 08:20:41.34 +54:24:53.0
163.76077 34.57293 galactic Lyn Second-epoch detections are separated by 0.4" and 4.8 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 | Gaia DR3 1032230935020158976 | 08:20:41.36 +54:24:52.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.234+/-0.025 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:41.34 +54:24:53.0: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:41.34 +54:24:53.0: 11.27 +/- 0.00 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 1032230935020158976,2461199.6803,10.38,0.05,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 1032230935020158976 20260608.1803 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 06 08.1803 2461199.6803 11.47 08:21:40.12 +55:53:12.0
161.96864 34.68031 galactic Lyn Second-epoch detections are separated by 2.2" and 4.6 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 | 08:21:40.12 +55:53:12.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.334+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:40.12 +55:53:12.0: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:40.12 +55:53:12.0: 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,2461199.6803,11.47,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.72 07:36:41.06 +56:41:14.3
160.71798 28.48525 galactic Lyn Second-epoch detections are separated by 0.5" and 5.2 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 | 07:36:41.06 +56:41:14.3 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.311+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:41.06 +56:41:14.3: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:41.06 +56:41:14.3: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 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,2461199.6803,11.72,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.48 08:31:04.65 +52:33:39.0
165.99829 36.15225 galactic Lyn Second-epoch detections are separated by 1.6" and 4.5 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 J127.7692+52.5608 | 08:31:04.63 +52:33:39.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.269+/-0.029 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:31:04.65 +52:33:39.0: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:31:04.65 +52:33:39.0: 12.61 +/- 0.01 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
ATO J127.7692+52.5608,2461199.6803,11.48,0.05,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
ATO J127.7692+52.5608 20260608.1803 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 06 08.1803 2461199.6803 11.06 07:39:54.67 +54:51:50.3
162.84221 28.71322 galactic Lyn Second-epoch detections are separated by 2.0" and 5.0 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 985437090236302720 | 07:39:54.72 +54:51:50.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.624+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:54.67 +54:51:50.3: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:54.67 +54:51:50.3: 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 985437090236302720,2461199.6803,11.06,0.05,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 985437090236302720 20260608.1803 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 06 08.1803 2461199.6803 11.57 08:31:24.58 +53:21:19.4
165.01266 36.17765 galactic Lyn Second-epoch detections are separated by 1.4" and 4.8 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 | Gaia DR3 1028960983143844992 | 08:31:24.57 +53:21:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.724+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:31:24.58 +53:21:19.4: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:31:24.58 +53:21:19.4: 12.62 +/- 0.01 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 1028960983143844992,2461199.6803,11.57,0.05,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
Gaia DR3 1028960983143844992 20260608.1803 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 06 08.1803 2461199.6803 11.68 07:41:53.68 +54:15:59.6
163.55962 28.92411 galactic Lyn Second-epoch detections are separated by 1.6" and 5.4 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 | 07:41:53.68 +54:15:59.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.320+/-0.029 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:53.68 +54:15:59.6: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:53.68 +54:15:59.6: 13.00 +/- 0.02 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,2461199.6803,11.68,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.72 08:28:16.57 +51:54:40.2
166.80928 35.73401 galactic Lyn Second-epoch detections are separated by 2.2" and 4.6 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 | 08:28:16.57 +51:54:40.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:28:16.57 +51:54:40.2: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:28:16.57 +51:54:40.2: 13.07 +/- 0.02 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,2461199.6803,11.72,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.78 07:36:02.19 +55:16:12.9
162.30218 28.21590 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 | 07:36:02.19 +55:16:12.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.723+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:02.19 +55:16:12.9: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:02.19 +55:16:12.9: 13.32 +/- 0.03 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,2461199.6803,11.78,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.61 07:55:04.71 +52:15:16.7
166.11711 30.65800 galactic Lyn Second-epoch detections are separated by 0.2" and 5.1 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 | ATO J118.7696+52.2545 | 07:55:04.71 +52:15:16.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.246+/-0.034 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:55:04.71 +52:15:16.7: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:55:04.71 +52:15:16.7: 12.66 +/- 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
ATO J118.7696+52.2545,2461199.6803,11.61,0.05,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
ATO J118.7696+52.2545 20260608.1803 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 06 08.1803 2461199.6803 11.21 08:21:35.05 +55:03:26.9
162.97706 34.69122 galactic Lyn Second-epoch detections are separated by 1.1" and 4.7 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 1032344459595754752 | 08:21:35.04 +55:03:27.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.362+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:35.05 +55:03:26.9: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:35.05 +55:03:26.9: 12.58 +/- 0.01 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 1032344459595754752,2461199.6803,11.21,0.05,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 1032344459595754752 20260608.1803 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 06 08.1803 2461199.6803 11.37 07:38:13.63 +54:29:54.6
163.21894 28.42454 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 | ATO J114.5498+54.4986 | 07:38:13.56 +54:29:55.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.681+/-0.029 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:13.63 +54:29:54.6: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:13.63 +54:29:54.6: 12.75 +/- 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
ATO J114.5498+54.4986,2461199.6803,11.37,0.05,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
ATO J114.5498+54.4986 20260608.1803 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 06 08.1803 2461199.6803 11.16 07:46:09.06 +54:14:31.2
163.67090 29.53859 galactic Lyn Second-epoch detections are separated by 1.8" and 5.1 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 984969802090554752 | 07:46:09.02 +54:14:31.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.365+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:46:09.06 +54:14:31.2: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:46:09.06 +54:14:31.2: 12.21 +/- 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 984969802090554752,2461199.6803,11.16,0.05,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 984969802090554752 20260608.1803 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 06 08.1803 2461199.6803 11.44 08:17:35.39 +54:31:08.8
163.63793 34.12197 galactic Lyn Second-epoch detections are separated by 1.3" and 5.0 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 1032256670464168064 | 08:17:35.54 +54:31:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.419+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:17:35.39 +54:31:08.8: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:17:35.39 +54:31:08.8: 12.57 +/- 0.01 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 1032256670464168064,2461199.6803,11.44,0.05,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
Gaia DR3 1032256670464168064 20260608.1803 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 06 08.1803 2461199.6803 11.59 07:43:51.41 +53:32:09.1
164.42982 29.12012 galactic Lyn Second-epoch detections are separated by 2.3" and 4.8 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 | 07:43:51.41 +53:32:09.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.436+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:51.41 +53:32:09.1: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:51.41 +53:32:09.1: 12.63 +/- 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
target,2461199.6803,11.59,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.97 08:19:35.98 +54:30:32.0
163.64846 34.41369 galactic Lyn Second-epoch detections are separated by 0.7" and 4.7 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 | ATO J124.9001+54.5086 | 08:19:36.03 +54:30:31.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5) J-Ks=0.398+/-0.044 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:35.98 +54:30:32.0: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:35.98 +54:30:32.0: 12.15 +/- 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
ATO J124.9001+54.5086,2461199.6803,10.97,0.05,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
ATO J124.9001+54.5086 20260608.1803 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 06 08.1803 2461199.6803 11.10 07:39:48.96 +54:56:12.8
162.75778 28.70875 galactic Lyn Second-epoch detections are separated by 0.7" and 5.3 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 985440491850399744 | 07:39:48.95 +54:56:12.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.303+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:48.96 +54:56:12.8: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:48.96 +54:56:12.8: 12.23 +/- 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 985440491850399744,2461199.6803,11.10,0.05,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 985440491850399744 20260608.1803 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 06 08.1803 2461199.6803 11.72 08:21:50.21 +54:43:16.5
163.38507 34.73456 galactic Lyn Second-epoch detections are separated by 0.5" and 4.8 pix
The object was found in VSX 1" ASASSN-V J082150.18+544317.0
Type: ROT
# Max. Min./Amp. JD0 Period
14.070 g Y 0.120 g 2459332.77900 10.061000000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:50.21 +54:43:16.5: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:50.21 +54:43:16.5: 13.36 +/- 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
ASASSN-V J082150.18+544317.0,2461199.6803,11.72,0.05,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
ASASSN-V J082150.18+544317.0 20260608.1803 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 06 08.1803 2461199.6803 11.69 08:29:30.29 +52:42:36.3
165.82072 35.91020 galactic Lyn Second-epoch detections are separated by 1.5" and 4.8 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 | ATO J127.3763+52.7101 | 08:29:30.29 +52:42:36.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.345+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:29:30.29 +52:42:36.3: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:29:30.29 +52:42:36.3: 13.04 +/- 0.02 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
ATO J127.3763+52.7101,2461199.6803,11.69,0.05,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
ATO J127.3763+52.7101 20260608.1803 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 06 08.1803 2461199.6803 10.94 08:20:42.39 +55:07:06.1
162.90632 34.56438 galactic Lyn Second-epoch detections are separated by 1.4" and 4.6 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 1032395238993501696 | 08:20:42.38 +55:07:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 (LAMOST DR5) J-Ks=0.459+/-0.027 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:42.39 +55:07:06.1: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:42.39 +55:07:06.1: 12.15 +/- 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 1032395238993501696,2461199.6803,10.94,0.05,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 1032395238993501696 20260608.1803 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 06 08.1803 2461199.6803 11.41 07:37:35.52 +55:27:56.4
162.11489 28.46056 galactic Lyn Second-epoch detections are separated by 1.1" and 5.0 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 | 07:37:35.52 +55:27:56.4 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.376+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:35.52 +55:27:56.4: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:35.52 +55:27:56.4: 12.82 +/- 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
target,2461199.6803,11.41,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.55 08:29:35.69 +50:46:26.4
168.21141 35.94271 galactic Lyn Second-epoch detections are separated by 0.9" and 5.0 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 | 08:29:35.69 +50:46:26.4 (user input) | T | P | (position from user input) SpType: F3 (LAMOST DR5) J-Ks=0.278+/-0.031 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:29:35.69 +50:46:26.4: 13.37 +/- 0.03 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:29:35.69 +50:46:26.4: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.94 +/- 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
target,2461199.6803,11.55,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.31 07:45:41.00 +54:29:58.7
163.36804 29.49910 galactic Lyn Second-epoch detections are separated by 1.5" and 4.9 pix
The object was found in VSX 1" Gaia DR3 984977597455643904
Type: ROT
# Max. Min./Amp. JD0 Period
12.070 G 12.100 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:45:41.00 +54:29:58.7: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:45:41.00 +54:29:58.7: 12.28 +/- 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 984977597455643904,2461199.6803,11.31,0.05,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 984977597455643904 20260608.1803 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 06 08.1803 2461199.6803 10.71 08:18:11.02 +54:33:37.0
163.58786 34.20797 galactic Lyn Second-epoch detections are separated by 0.4" and 4.8 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 | Gaia DR3 1032279725848606592 | 08:18:11.06 +54:33:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.380+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:18:11.02 +54:33:37.0: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:18:11.02 +54:33:37.0: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.62 +/- 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 1032279725848606592,2461199.6803,10.71,0.05,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 1032279725848606592 20260608.1803 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 06 08.1803 2461199.6803 11.32 08:23:40.48 +55:06:30.6
162.90524 34.98890 galactic Lyn Second-epoch detections are separated by 0.8" and 4.8 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 | 08:23:40.48 +55:06:30.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.374+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:40.48 +55:06:30.6: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:40.48 +55:06:30.6: 12.63 +/- 0.01 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
target,2461199.6803,11.32,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.28 07:44:51.57 +53:39:04.0
164.31962 29.28187 galactic Lyn Second-epoch detections are separated by 1.1" and 5.0 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 984556175264057344 | 07:44:51.63 +53:39:03.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5) J-Ks=0.574+/-0.024 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:51.57 +53:39:04.0: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:51.57 +53:39:04.0: 12.31 +/- 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 984556175264057344,2461199.6803,11.28,0.05,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
Gaia DR3 984556175264057344 20260608.1803 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 06 08.1803 2461199.6803 11.54 07:48:00.97 +53:23:03.7
164.68660 29.71695 galactic Lyn Second-epoch detections are separated by 3.8" and 4.8 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 | 07:48:00.97 +53:23:03.7 (user input) | T | P | (position from user input) J-Ks=0.264+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:48:00.97 +53:23:03.7: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:48:00.97 +53:23:03.7: 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
target,2461199.6803,11.54,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.53 07:38:37.01 +54:28:01.6
163.26292 28.47643 galactic Lyn Second-epoch detections are separated by 0.5" and 5.2 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 | 07:38:37.01 +54:28:01.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.421+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:37.01 +54:28:01.6: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:37.01 +54:28:01.6: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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,2461199.6803,11.53,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.04 08:22:20.43 +55:13:53.6
162.76200 34.79492 galactic Lyn Second-epoch detections are separated by 1.0" and 4.6 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 1032370401198215168 | 08:22:20.47 +55:13:53.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.441+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:20.43 +55:13:53.6: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:20.43 +55:13:53.6: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 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 1032370401198215168,2461199.6803,11.04,0.05,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 1032370401198215168 20260608.1803 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 06 08.1803 2461199.6803 11.50 08:22:09.31 +54:05:44.2
164.14563 34.79092 galactic Lyn Second-epoch detections are separated by 1.7" and 4.9 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 | 08:22:09.31 +54:05:44.2 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.422+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:09.31 +54:05:44.2: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:09.31 +54:05:44.2: 13.05 +/- 0.02 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,2461199.6803,11.50,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.43 08:20:47.18 +53:50:31.3
164.45620 34.59189 galactic Lyn Second-epoch detections are separated by 0.5" and 4.9 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 | ATO J125.1962+53.8418 | 08:20:47.11 +53:50:30.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.865+/-0.032 (M)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:47.18 +53:50:31.3: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:47.18 +53:50:31.3: 12.71 +/- 0.01 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
ATO J125.1962+53.8418,2461199.6803,11.43,0.05,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
ATO J125.1962+53.8418 20260608.1803 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 06 08.1803 2461199.6803 11.53 08:24:43.36 +55:07:09.6
162.88604 35.13832 galactic Lyn Second-epoch detections are separated by 0.9" and 4.9 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 | 08:24:43.36 +55:07:09.6 (user input) | T | P | (position from user input) J-Ks=0.516+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:43.36 +55:07:09.6: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:43.36 +55:07:09.6: 12.73 +/- 0.01 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
target,2461199.6803,11.53,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.64 08:29:11.10 +52:20:44.7
166.27148 35.86842 galactic Lyn Second-epoch detections are separated by 1.1" and 4.7 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 | 08:29:11.10 +52:20:44.7 (user input) | T | P | (position from user input) J-Ks=0.261+/-0.032 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:29:11.10 +52:20:44.7: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:29:11.10 +52:20:44.7: 12.84 +/- 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,2461199.6803,11.64,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.38 08:21:05.41 +55:15:28.2
162.73551 34.61612 galactic Lyn Second-epoch detections are separated by 0.4" and 4.8 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 | 08:21:05.41 +55:15:28.2 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.330+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:05.41 +55:15:28.2: 16.31 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:05.41 +55:15:28.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 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,2461199.6803,11.38,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.80 07:35:06.39 +56:25:49.4
160.97738 28.23795 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 989141280486471680 | 07:35:06.37 +56:25:49.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.330+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:06.39 +56:25:49.4: 14.73 +/- 0.13 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:06.39 +56:25:49.4: 11.97 +/- 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 989141280486471680,2461199.6803,10.80,0.05,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 989141280486471680 20260608.1803 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 06 08.1803 2461199.6803 11.71 07:47:19.19 +53:17:11.6
164.78481 29.60254 galactic Lyn Second-epoch detections are separated by 2.3" and 5.5 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 | 07:47:19.19 +53:17:11.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.326+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:47:19.19 +53:17:11.6: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:47:19.19 +53:17:11.6: 12.89 +/- 0.02 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,2461199.6803,11.71,0.05,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
target 20260608.1803 11.71CV 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 06 08.1803 2461199.6803 11.56 08:23:32.85 +54:43:15.6
163.37864 34.98150 galactic Lyn Second-epoch detections are separated by 1.3" and 4.9 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 | 08:23:32.85 +54:43:15.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.372+/-0.026 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:32.85 +54:43:15.6: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:32.85 +54:43:15.6: 13.07 +/- 0.02 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,2461199.6803,11.56,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.29 07:36:53.55 +56:28:46.4
160.95656 28.48886 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 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 986142736182919040 | 07:36:53.52 +56:28:47.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5) J-Ks=0.555+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:53.55 +56:28:46.4: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:53.55 +56:28:46.4: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 986142736182919040,2461199.6803,11.29,0.05,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 986142736182919040 20260608.1803 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 06 08.1803 2461199.6803 11.31 07:41:15.81 +55:31:02.6
162.12793 28.98300 galactic Lyn Second-epoch detections are separated by 1.5" and 5.1 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 985853946878201600 | 07:41:15.84 +55:31:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.557+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:15.81 +55:31:02.6: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:15.81 +55:31:02.6: 12.45 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.45 +/- 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 985853946878201600,2461199.6803,11.31,0.05,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 985853946878201600 20260608.1803 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 06 08.1803 2461199.6803 11.03 08:20:32.05 +54:36:18.0
163.53007 34.54811 galactic Lyn Second-epoch detections are separated by 0.8" and 4.7 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 1032237527794467712 | 08:20:32.00 +54:36:18.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.607+/-0.025 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:32.05 +54:36:18.0: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:32.05 +54:36:18.0: 12.31 +/- 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 1032237527794467712,2461199.6803,11.03,0.05,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 1032237527794467712 20260608.1803 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 06 08.1803 2461199.6803 11.13 08:22:11.83 +55:10:59.1
162.82167 34.77578 galactic Lyn Second-epoch detections are separated by 0.3" and 4.8 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 | Gaia DR3 1032368747635217792 | 08:22:11.80 +55:10:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.263+/-0.029 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:11.83 +55:10:59.1: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:11.83 +55:10:59.1: 12.35 +/- 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 1032368747635217792,2461199.6803,11.13,0.05,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 1032368747635217792 20260608.1803 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 06 08.1803 2461199.6803 11.22 07:38:52.63 +55:18:01.4
162.32768 28.62083 galactic Lyn Second-epoch detections are separated by 0.5" and 5.2 pix
The object was found in VSX 1" Gaia DR3 986012100458570112
Type: ROT
# Max. Min./Amp. JD0 Period
12.340 G 12.380 G G
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:52.63 +55:18:01.4: 15.11 +/- 0.17 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:52.63 +55:18:01.4: 12.50 +/- 0.01 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 986012100458570112,2461199.6803,11.22,0.05,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 986012100458570112 20260608.1803 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 06 08.1803 2461199.6803 11.32 07:43:11.97 +54:08:56.3
163.71976 29.09907 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 985343597387718784 | 07:43:11.96 +54:08:57.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.424+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:11.97 +54:08:56.3: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:11.97 +54:08:56.3: 12.50 +/- 0.01 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 985343597387718784,2461199.6803,11.32,0.05,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
Gaia DR3 985343597387718784 20260608.1803 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 06 08.1803 2461199.6803 11.44 07:53:59.56 +52:13:15.1
166.13641 30.48918 galactic Lyn Second-epoch detections are separated by 0.5" and 5.2 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 936147083474534272 | 07:53:59.63 +52:13:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.362+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:53:59.56 +52:13:15.1: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:53:59.56 +52:13:15.1: 12.42 +/- 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 936147083474534272,2461199.6803,11.44,0.05,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
Gaia DR3 936147083474534272 20260608.1803 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 06 08.1803 2461199.6803 11.67 08:23:25.31 +53:58:35.1
164.28766 34.97859 galactic Lyn Second-epoch detections are separated by 1.2" and 4.6 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 | 08:23:25.31 +53:58:35.1 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:25.31 +53:58:35.1: 16.32 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:25.31 +53:58:35.1: 13.30 +/- 0.02 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,2461199.6803,11.67,0.05,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
target 20260608.1803 11.67CV 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 06 08.1803 2461199.6803 11.92 07:38:33.04 +55:46:12.3
161.79016 28.63265 galactic Lyn Second-epoch detections are separated by 2.8" and 5.4 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 | ATO J114.6560+55.7685 | 07:38:33.04 +55:46:12.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.258+/-0.040 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:33.04 +55:46:12.3: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:33.04 +55:46:12.3: 13.37 +/- 0.03 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
ATO J114.6560+55.7685,2461199.6803,11.92,0.05,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
ATO J114.6560+55.7685 20260608.1803 11.92CV 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 06 08.1803 2461199.6803 11.21 07:38:43.19 +55:08:18.5
162.50744 28.57827 galactic Lyn Second-epoch detections are separated by 0.8" and 5.2 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 985632390989707264 | 07:38:43.15 +55:08:19.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.658+/-0.032 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:43.19 +55:08:18.5: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:43.19 +55:08:18.5: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 985632390989707264,2461199.6803,11.21,0.05,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 985632390989707264 20260608.1803 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 06 08.1803 2461199.6803 10.91 07:36:15.61 +56:11:10.5
161.27534 28.36592 galactic Lyn Second-epoch detections are separated by 0.3" and 5.2 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 986131023807983360 | 07:36:15.54 +56:11:06.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:15.61 +56:11:10.5: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:15.61 +56:11:10.5: 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 986131023807983360,2461199.6803,10.91,0.05,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 986131023807983360 20260608.1803 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 06 08.1803 2461199.6803 10.90 08:23:35.28 +54:26:58.8
163.70957 34.99384 galactic Lyn Second-epoch detections are separated by 0.8" and 4.8 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 | Gaia DR3 1032123526477964928 | 08:23:35.34 +54:26:59.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.321+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:35.28 +54:26:58.8: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:35.28 +54:26:58.8: 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 1032123526477964928,2461199.6803,10.90,0.05,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 1032123526477964928 20260608.1803 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 06 08.1803 2461199.6803 10.96 07:46:24.07 +53:53:07.4
164.08293 29.53537 galactic Lyn Second-epoch detections are separated by 0.8" and 5.2 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 984577516957381120 | 07:46:24.04 +53:53:07.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.414+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:46:24.07 +53:53:07.4: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:46:24.07 +53:53:07.4: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 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 984577516957381120,2461199.6803,10.96,0.05,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 984577516957381120 20260608.1803 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 06 08.1803 2461199.6803 10.95 07:44:50.85 +53:49:29.2
164.12167 29.30081 galactic Lyn Second-epoch detections are separated by 0.7" and 5.3 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 | ATO J116.2118+53.8247 | 07:44:50.84 +53:49:29.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.733+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:50.85 +53:49:29.2: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:50.85 +53:49:29.2: 11.90 +/- 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
ATO J116.2118+53.8247,2461199.6803,10.95,0.05,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
ATO J116.2118+53.8247 20260608.1803 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 06 08.1803 2461199.6803 10.90 07:35:55.33 +56:16:01.8
161.17744 28.32945 galactic Lyn Second-epoch detections are separated by 0.7" and 5.0 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 986136590085600896 | 07:35:55.31 +56:16:02.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.566+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:55.33 +56:16:01.8: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:55.33 +56:16:01.8: 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 986136590085600896,2461199.6803,10.90,0.05,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 986136590085600896 20260608.1803 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 06 08.1803 2461199.6803 10.98 07:37:56.12 +56:00:26.4
161.51002 28.57573 galactic Lyn Second-epoch detections are separated by 0.8" and 5.2 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 986114904794822528 | 07:37:56.04 +56:00:26.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.577+/-0.029 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:56.12 +56:00:26.4: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:56.12 +56:00:26.4: 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 986114904794822528,2461199.6803,10.98,0.05,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 986114904794822528 20260608.1803 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 06 08.1803 2461199.6803 10.73 08:21:56.67 +54:55:13.9
163.14223 34.74594 galactic Lyn Second-epoch detections are separated by 0.2" and 4.8 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 | ATO J125.4860+54.9205 | 08:21:56.66 +54:55:13.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5) J-Ks=0.215+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:56.67 +54:55:13.9: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:56.67 +54:55:13.9: 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
ATO J125.4860+54.9205,2461199.6803,10.73,0.05,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
ATO J125.4860+54.9205 20260608.1803 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 06 08.1803 2461199.6803 11.77 08:24:18.65 +55:32:22.0
162.37549 35.06450 galactic Lyn Second-epoch detections are separated by 3.8" and 4.2 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 | 08:24:18.65 +55:32:22.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.406+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:18.65 +55:32:22.0: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:18.65 +55:32:22.0: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 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,2461199.6803,11.77,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.04 08:20:25.65 +54:36:08.0
163.53369 34.53270 galactic Lyn Second-epoch detections are separated by 0.5" and 4.8 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 | Gaia DR3 1032237355995776000 | 08:20:25.73 +54:36:09.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 1986AJ.....91..144S StKM 1- 693
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:25.65 +54:36:08.0: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:25.65 +54:36:08.0: 12.36 +/- 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 1032237355995776000,2461199.6803,11.04,0.05,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 1032237355995776000 20260608.1803 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 06 08.1803 2461199.6803 11.38 07:40:37.52 +54:31:57.3
163.23194 28.77404 galactic Lyn Second-epoch detections are separated by 2.6" and 4.8 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 | Gaia DR3 985413863053178240 | 07:40:37.56 +54:31:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.344+/-0.035 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:37.52 +54:31:57.3: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:37.52 +54:31:57.3: 12.53 +/- 0.01 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 985413863053178240,2461199.6803,11.38,0.05,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 985413863053178240 20260608.1803 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 06 08.1803 2461199.6803 11.19 07:37:37.69 +55:30:54.0
162.05997 28.47190 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 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 986031105689254656 | 07:37:37.69 +55:30:54.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.352+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:37.69 +55:30:54.0: 14.09 +/- 0.07 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:37.69 +55:30:54.0: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 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 986031105689254656,2461199.6803,11.19,0.05,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
Gaia DR3 986031105689254656 20260608.1803 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 06 08.1803 2461199.6803 11.73 08:19:52.27 +54:23:11.1
163.79654 34.45420 galactic Lyn Second-epoch detections are separated by 0.1" and 4.8 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 | ATO J124.9654+54.3876 | 08:19:52.27 +54:23:11.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.478+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:52.27 +54:23:11.1: 15.98 +/- 0.29 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:52.27 +54:23:11.1: 13.29 +/- 0.02 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
ATO J124.9654+54.3876,2461199.6803,11.73,0.05,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
ATO J124.9654+54.3876 20260608.1803 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 06 08.1803 2461199.6803 11.22 07:36:16.56 +55:02:53.2
162.55721 28.21983 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 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 985642080435379072 | 07:36:16.54 +55:02:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.554+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:16.56 +55:02:53.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:16.56 +55:02:53.2: 12.60 +/- 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 985642080435379072,2461199.6803,11.22,0.05,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 985642080435379072 20260608.1803 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 06 08.1803 2461199.6803 10.88 07:38:49.79 +55:30:13.0
162.09698 28.63927 galactic Lyn Second-epoch detections are separated by 0.5" and 5.2 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 986021519321921536 | 07:38:49.83 +55:30:13.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.375+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:49.79 +55:30:13.0: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:49.79 +55:30:13.0: 11.93 +/- 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 986021519321921536,2461199.6803,10.88,0.05,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 986021519321921536 20260608.1803 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 06 08.1803 2461199.6803 10.81 07:36:19.16 +54:47:41.2
162.84295 28.19138 galactic Lyn Second-epoch detections are separated by 1.2" and 5.1 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 985612157399174016 | 07:36:19.16 +54:47:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:19.16 +54:47:41.2: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:19.16 +54:47:41.2: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 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 985612157399174016,2461199.6803,10.81,0.05,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 985612157399174016 20260608.1803 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 06 08.1803 2461199.6803 11.61 08:20:23.52 +54:43:10.0
163.39149 34.52599 galactic Lyn Second-epoch detections are separated by 2.4" and 4.4 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 | 08:20:23.52 +54:43:10.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.449+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:23.52 +54:43:10.0: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:23.52 +54:43:10.0: 13.36 +/- 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,2461199.6803,11.61,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.72 08:22:32.72 +55:14:19.4
162.75229 34.82391 galactic Lyn Second-epoch detections are separated by 0.6" and 4.7 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 | ATO J125.6429+55.2374 | 08:22:32.72 +55:14:19.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.580+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:32.72 +55:14:19.4: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:32.72 +55:14:19.4: 11.82 +/- 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
ATO J125.6429+55.2374,2461199.6803,10.72,0.05,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
ATO J125.6429+55.2374 20260608.1803 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 06 08.1803 2461199.6803 11.49 07:42:57.85 +55:23:49.5
162.29562 29.20910 galactic Lyn Second-epoch detections are separated by 3.8" and 5.6 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 985838377620323840 | 07:42:57.92 +55:23:49.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5) J-Ks=0.296+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:57.85 +55:23:49.5: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:57.85 +55:23:49.5: 12.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 985838377620323840,2461199.6803,11.49,0.05,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
Gaia DR3 985838377620323840 20260608.1803 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 06 08.1803 2461199.6803 11.78 08:25:21.22 +53:50:55.1
164.43740 35.26538 galactic Lyn Second-epoch detections are separated by 0.3" and 4.8 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 | ATO J126.3384+53.8484 | 08:25:21.22 +53:50:55.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.274+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:21.22 +53:50:55.1: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:21.22 +53:50:55.1: 13.14 +/- 0.02 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
ATO J126.3384+53.8484,2461199.6803,11.78,0.05,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
ATO J126.3384+53.8484 20260608.1803 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 06 08.1803 2461199.6803 11.40 07:41:55.54 +54:26:56.1
163.35346 28.95103 galactic Lyn Second-epoch detections are separated by 0.3" and 5.2 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 985364183167851776 | 07:41:55.60 +54:26:55.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.391+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:55.54 +54:26:56.1: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:55.54 +54:26:56.1: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 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 985364183167851776,2461199.6803,11.40,0.05,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 985364183167851776 20260608.1803 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 06 08.1803 2461199.6803 11.33 07:37:29.05 +56:35:29.5
160.84101 28.58313 galactic Lyn Second-epoch detections are separated by 1.2" and 5.3 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 986238118816407424 | 07:37:29.04 +56:35:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.298+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:29.05 +56:35:29.5: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:29.05 +56:35:29.5: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 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 986238118816407424,2461199.6803,11.33,0.05,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
Gaia DR3 986238118816407424 20260608.1803 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 06 08.1803 2461199.6803 11.18 08:23:00.37 +54:36:02.2
163.52774 34.90610 galactic Lyn Second-epoch detections are separated by 1.0" and 4.7 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 1032319411346522752 | 08:23:00.35 +54:36:01.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.303+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:00.37 +54:36:02.2: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:00.37 +54:36:02.2: 12.39 +/- 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 1032319411346522752,2461199.6803,11.18,0.05,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 1032319411346522752 20260608.1803 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 06 08.1803 2461199.6803 11.49 07:52:37.90 +51:53:24.3
166.49136 30.24546 galactic Lyn Second-epoch detections are separated by 1.7" and 5.0 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 936042668525057408 | 07:52:37.95 +51:53:23.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.318+/-0.029 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:52:37.90 +51:53:24.3: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:52:37.90 +51:53:24.3: 12.48 +/- 0.01 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 936042668525057408,2461199.6803,11.49,0.05,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
Gaia DR3 936042668525057408 20260608.1803 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 06 08.1803 2461199.6803 11.67 08:23:47.35 +55:37:40.6
162.27090 34.98750 galactic Lyn Second-epoch detections are separated by 2.0" and 5.1 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 | 08:23:47.35 +55:37:40.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.328+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:47.35 +55:37:40.6: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:47.35 +55:37:40.6: 13.12 +/- 0.02 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,2461199.6803,11.67,0.05,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
target 20260608.1803 11.67CV 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 06 08.1803 2461199.6803 11.47 07:41:11.23 +55:21:33.9
162.30587 28.95406 galactic Lyn Second-epoch detections are separated by 2.4" and 4.7 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 985829276586056704 | 07:41:11.35 +55:21:34.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.517+/-0.034 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:11.23 +55:21:33.9: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:11.23 +55:21:33.9: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 985829276586056704,2461199.6803,11.47,0.05,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
Gaia DR3 985829276586056704 20260608.1803 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 06 08.1803 2461199.6803 11.45 08:26:10.66 +52:46:37.9
165.74822 35.40563 galactic Lyn Second-epoch detections are separated by 1.8" and 4.6 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 J126.5440+52.7770 | 08:26:10.56 +52:46:37.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.635+/-0.038 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:26:10.66 +52:46:37.9: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:26:10.66 +52:46:37.9: 12.47 +/- 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
ATO J126.5440+52.7770,2461199.6803,11.45,0.05,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
ATO J126.5440+52.7770 20260608.1803 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 06 08.1803 2461199.6803 11.81 08:21:44.81 +54:19:59.5
163.85745 34.72801 galactic Lyn Second-epoch detections are separated by 2.3" and 4.4 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 | 08:21:44.81 +54:19:59.5 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.352+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:44.81 +54:19:59.5: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:44.81 +54:19:59.5: 13.34 +/- 0.02 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,2461199.6803,11.81,0.05,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
target 20260608.1803 11.81CV 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 06 08.1803 2461199.6803 11.35 08:28:27.72 +52:26:36.5
166.15307 35.75664 galactic Lyn Second-epoch detections are separated by 1.2" and 5.0 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 1028806020723830656 | 08:28:27.64 +52:26:36.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.573+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:28:27.72 +52:26:36.5: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:28:27.72 +52:26:36.5: 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 1028806020723830656,2461199.6803,11.35,0.05,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 1028806020723830656 20260608.1803 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 06 08.1803 2461199.6803 11.28 07:49:09.67 +53:17:30.8
164.81431 29.87658 galactic Lyn Second-epoch detections are separated by 1.4" and 5.0 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 | ATO J117.2915+53.2885 | 07:49:09.79 +53:17:31.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=0.829+/-0.036 (M)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:49:09.67 +53:17:30.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:49:09.67 +53:17:30.8: 12.42 +/- 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
ATO J117.2915+53.2885,2461199.6803,11.28,0.05,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
ATO J117.2915+53.2885 20260608.1803 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 06 08.1803 2461199.6803 11.11 08:22:09.54 +54:25:50.2
163.73776 34.78649 galactic Lyn Second-epoch detections are separated by 1.0" and 4.6 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 1032310679677178752 | 08:22:09.56 +54:25:50.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.620+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:09.54 +54:25:50.2: 16.33 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:09.54 +54:25:50.2: 12.42 +/- 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 1032310679677178752,2461199.6803,11.11,0.05,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 1032310679677178752 20260608.1803 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 06 08.1803 2461199.6803 11.24 07:39:58.65 +55:09:48.5
162.50460 28.75964 galactic Lyn Second-epoch detections are separated by 1.1" and 5.1 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 985819582844018304 | 07:39:58.64 +55:09:48.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.282+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:58.65 +55:09:48.5: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:58.65 +55:09:48.5: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 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 985819582844018304,2461199.6803,11.24,0.05,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
Gaia DR3 985819582844018304 20260608.1803 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 06 08.1803 2461199.6803 11.26 08:17:35.36 +54:32:08.6
163.61786 34.12186 galactic Lyn Second-epoch detections are separated by 0.2" and 4.9 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 | ATO J124.3898+54.5359 | 08:17:35.43 +54:32:08.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.318+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:17:35.36 +54:32:08.6: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:17:35.36 +54:32:08.6: 12.40 +/- 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
ATO J124.3898+54.5359,2461199.6803,11.26,0.05,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 J124.3898+54.5359 20260608.1803 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 06 08.1803 2461199.6803 11.16 07:38:05.50 +55:09:25.6
162.47338 28.49163 galactic Lyn Second-epoch detections are separated by 0.8" and 5.3 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 985634864890869248 | 07:38:05.52 +55:09:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.189+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:05.50 +55:09:25.6: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:05.50 +55:09:25.6: 12.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 985634864890869248,2461199.6803,11.16,0.05,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 985634864890869248 20260608.1803 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 06 08.1803 2461199.6803 11.28 07:39:06.38 +54:40:18.3
163.04262 28.57363 galactic Lyn Second-epoch detections are separated by 0.9" and 5.3 pix
The object was found in VSX 0" Gaia DR3 985430806700502784
Type: ROT
# Max. Min./Amp. JD0 Period
12.350 G 12.370 G G
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:06.38 +54:40:18.3: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:06.38 +54:40:18.3: 12.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 985430806700502784,2461199.6803,11.28,0.05,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
Gaia DR3 985430806700502784 20260608.1803 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 06 08.1803 2461199.6803 10.95 07:38:06.68 +55:57:53.4
161.56145 28.59503 galactic Lyn Second-epoch detections are separated by 0.1" and 5.1 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 986066186981744000 | 07:38:06.65 +55:57:54.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.592+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:06.68 +55:57:53.4: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:06.68 +55:57:53.4: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.95 +/- 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 986066186981744000,2461199.6803,10.95,0.05,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 986066186981744000 20260608.1803 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 06 08.1803 2461199.6803 10.71 08:21:46.32 +54:37:10.4
163.50900 34.72707 galactic Lyn Second-epoch detections are separated by 0.4" and 4.7 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 1032316044092172544 | 08:21:46.33 +54:37:10.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.259+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:46.32 +54:37:10.4: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:46.32 +54:37:10.4: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 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
Gaia DR3 1032316044092172544,2461199.6803,10.71,0.05,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 1032316044092172544 20260608.1803 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 06 08.1803 2461199.6803 11.16 08:22:25.51 +56:03:00.2
161.76543 34.78034 galactic Lyn Second-epoch detections are separated by 0.8" and 4.8 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 | Gaia DR3 1033959397363072896 | 08:22:25.41 +56:03:00.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.375+/-0.027 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:25.51 +56:03:00.2: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:25.51 +56:03:00.2: 12.35 +/- 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 1033959397363072896,2461199.6803,11.16,0.05,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 1033959397363072896 20260608.1803 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 06 08.1803 2461199.6803 11.68 07:36:55.95 +55:41:28.8
161.84688 28.39684 galactic Lyn Second-epoch detections are separated by 2.2" and 4.9 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 | 07:36:55.95 +55:41:28.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.304+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:55.95 +55:41:28.8: 15.64 +/- 0.29 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:55.95 +55:41:28.8: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 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,2461199.6803,11.68,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.75 08:19:57.25 +54:26:07.0
163.73716 34.46585 galactic Lyn Second-epoch detections are separated by 1.3" and 4.9 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 1032228839076123264 | 08:19:57.31 +54:26:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.420+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:57.25 +54:26:07.0: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:57.25 +54:26:07.0: 11.81 +/- 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 1032228839076123264,2461199.6803,10.75,0.05,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 1032228839076123264 20260608.1803 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 06 08.1803 2461199.6803 10.87 07:45:12.60 +53:51:05.8
164.09832 29.35707 galactic Lyn Second-epoch detections are separated by 0.3" and 5.3 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 984582705277890176 | 07:45:12.58 +53:51:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.575+/-0.027 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:45:12.60 +53:51:05.8: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:45:12.60 +53:51:05.8: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 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 984582705277890176,2461199.6803,10.87,0.05,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 984582705277890176 20260608.1803 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 06 08.1803 2461199.6803 11.19 07:36:02.24 +56:32:40.2
160.86697 28.37965 galactic Lyn Second-epoch detections are separated by 0.9" and 5.0 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 986146790631801344 | 07:35:57.45 +56:32:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.571+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:02.24 +56:32:40.2: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:02.24 +56:32:40.2: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 986146790631801344,2461199.6803,11.19,0.05,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
Gaia DR3 986146790631801344 20260608.1803 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 06 08.1803 2461199.6803 11.24 07:39:16.74 +55:55:09.1
161.63527 28.75192 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 986063678720831360 | 07:39:16.76 +55:55:09.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.605+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:16.74 +55:55:09.1: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:16.74 +55:55:09.1: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 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 986063678720831360,2461199.6803,11.24,0.05,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
Gaia DR3 986063678720831360 20260608.1803 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 06 08.1803 2461199.6803 11.48 07:48:52.53 +53:47:11.8
164.24177 29.88746 galactic Lyn Second-epoch detections are separated by 1.0" and 5.1 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 | ATO J117.2143+53.7930 | 07:48:52.59 +53:47:10.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.296+/-0.036 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:48:52.53 +53:47:11.8: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:48:52.53 +53:47:11.8: 12.44 +/- 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
ATO J117.2143+53.7930,2461199.6803,11.48,0.05,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
ATO J117.2143+53.7930 20260608.1803 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 06 08.1803 2461199.6803 11.30 07:39:17.77 +54:46:55.1
162.92215 28.61499 galactic Lyn Second-epoch detections are separated by 2.0" and 5.4 pix
The object was found in VSX 0" Gaia DR3 985433207585870336
Type: VAR
# Max. Min./Amp. JD0 Period
12.280 G 12.290 G 0.015789000000 G
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:17.77 +54:46:55.1: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:17.77 +54:46:55.1: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 985433207585870336,2461199.6803,11.30,0.05,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 985433207585870336 20260608.1803 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 06 08.1803 2461199.6803 11.81 08:23:28.28 +55:29:36.3
162.43693 34.94743 galactic Lyn Second-epoch detections are separated by 1.2" and 4.6 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 | 08:23:28.28 +55:29:36.3 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.421+/-0.026 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:28.28 +55:29:36.3: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:28.28 +55:29:36.3: 13.28 +/- 0.02 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,2461199.6803,11.81,0.05,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
target 20260608.1803 11.81CV 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 06 08.1803 2461199.6803 11.90 07:40:01.35 +55:37:17.0
161.98672 28.82081 galactic Lyn Second-epoch detections are separated by 1.0" and 5.1 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 | 07:40:01.35 +55:37:17.0 (user input) | T | P | (position from user input) J-Ks=0.313+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:01.35 +55:37:17.0: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:01.35 +55:37:17.0: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 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,2461199.6803,11.90,0.05,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
target 20260608.1803 11.90CV 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 06 08.1803 2461199.6803 10.71 08:22:07.97 +54:49:05.8
163.26594 34.77526 galactic Lyn Second-epoch detections are separated by 0.5" and 4.8 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 | ATO J125.5280+54.8225 | 08:22:07.96 +54:49:06.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.391+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:07.97 +54:49:05.8: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:07.97 +54:49:05.8: 11.78 +/- 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
ATO J125.5280+54.8225,2461199.6803,10.71,0.05,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
ATO J125.5280+54.8225 20260608.1803 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 06 08.1803 2461199.6803 10.77 08:22:53.87 +54:43:53.5
163.36859 34.88748 galactic Lyn Second-epoch detections are separated by 1.0" and 4.8 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 | Gaia DR3 1032323465795649024 | 08:22:53.90 +54:43:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.277+/-0.026 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:53.87 +54:43:53.5: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:53.87 +54:43:53.5: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 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 1032323465795649024,2461199.6803,10.77,0.05,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 1032323465795649024 20260608.1803 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 06 08.1803 2461199.6803 11.68 07:37:06.18 +54:48:15.3
162.84978 28.30455 galactic Lyn Second-epoch detections are separated by 2.3" and 4.9 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 | 07:37:06.18 +54:48:15.3 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.314+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:06.18 +54:48:15.3: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:06.18 +54:48:15.3: 13.30 +/- 0.03 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,2461199.6803,11.68,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.16 07:35:54.03 +55:37:17.7
161.90404 28.24349 galactic Lyn Second-epoch detections are separated by 0.9" and 5.3 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 | 07:35:54.03 +55:37:17.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.473+/-0.035 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:54.03 +55:37:17.7: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:54.03 +55:37:17.7: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 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,2461199.6803,11.16,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.48 07:52:50.93 +51:56:21.6
166.43900 30.28422 galactic Lyn Second-epoch detections are separated by 1.9" and 4.9 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 936044347857003392 | 07:52:50.91 +51:56:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.353+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:52:50.93 +51:56:21.6: 14.37 +/- 0.08 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:52:50.93 +51:56:21.6: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 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 936044347857003392,2461199.6803,11.48,0.05,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 936044347857003392 20260608.1803 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 06 08.1803 2461199.6803 11.35 07:36:14.89 +56:59:44.3
160.36166 28.46249 galactic Lyn Second-epoch detections are separated by 2.1" and 5.1 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 989256175155574656 | 07:36:14.98 +56:59:44.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.324+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:14.89 +56:59:44.3: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:14.89 +56:59:44.3: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 989256175155574656,2461199.6803,11.35,0.05,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 989256175155574656 20260608.1803 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 06 08.1803 2461199.6803 11.37 08:25:06.57 +52:50:43.1
165.66661 35.24358 galactic Lyn Second-epoch detections are separated by 1.1" and 4.9 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 | ATO J126.2775+52.8452 | 08:25:06.61 +52:50:42.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.380+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:06.57 +52:50:43.1: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:06.57 +52:50:43.1: 12.35 +/- 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
ATO J126.2775+52.8452,2461199.6803,11.37,0.05,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
ATO J126.2775+52.8452 20260608.1803 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 06 08.1803 2461199.6803 11.29 07:42:06.78 +54:10:48.9
163.66200 28.94507 galactic Lyn Second-epoch detections are separated by 0.9" and 5.3 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 | ATO J115.5268+54.1762 | 07:42:06.77 +54:10:48.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.286+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:06.78 +54:10:48.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:06.78 +54:10:48.9: 12.44 +/- 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
ATO J115.5268+54.1762,2461199.6803,11.29,0.05,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
ATO J115.5268+54.1762 20260608.1803 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 06 08.1803 2461199.6803 11.38 08:28:55.29 +52:46:49.2
165.73635 35.82046 galactic Lyn Second-epoch detections are separated by 2.9" and 4.8 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 | Gaia DR3 1028846496495750400 | 08:28:55.29 +52:46:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.541+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:28:55.29 +52:46:49.2: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:28:55.29 +52:46:49.2: 12.39 +/- 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 1028846496495750400,2461199.6803,11.38,0.05,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 1028846496495750400 20260608.1803 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 06 08.1803 2461199.6803 11.30 07:38:50.12 +54:28:35.1
163.25722 28.50913 galactic Lyn Second-epoch detections are separated by 0.5" and 5.3 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 985401532203422720 | 07:38:50.04 +54:28:35.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.443+/-0.035 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:50.12 +54:28:35.1: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:50.12 +54:28:35.1: 12.48 +/- 0.01 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 985401532203422720,2461199.6803,11.30,0.05,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 985401532203422720 20260608.1803 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 06 08.1803 2461199.6803 11.09 08:18:25.59 +54:52:09.2
163.21395 34.24101 galactic Lyn Second-epoch detections are separated by 0.1" and 4.8 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 | Gaia DR3 1032303223614223872 | 08:18:25.55 +54:52:09.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.469+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:18:25.59 +54:52:09.2: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:18:25.59 +54:52:09.2: 12.28 +/- 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 1032303223614223872,2461199.6803,11.09,0.05,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 1032303223614223872 20260608.1803 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 06 08.1803 2461199.6803 11.78 08:21:09.51 +54:52:49.0
163.19397 34.63380 galactic Lyn Second-epoch detections are separated by 1.4" and 4.6 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 | 08:21:09.51 +54:52:49.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.437+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:09.51 +54:52:49.0: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:09.51 +54:52:49.0: 13.71 +/- 0.04 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,2461199.6803,11.78,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.62 07:51:47.99 +52:02:46.5
166.29516 30.13571 galactic Lyn Second-epoch detections are separated by 0.9" and 5.3 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 | 07:51:47.99 +52:02:46.5 (user input) | T | P | (position from user input) J-Ks=0.317+/-0.032 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:51:47.99 +52:02:46.5: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:51:47.99 +52:02:46.5: 12.89 +/- 0.02 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,2461199.6803,11.62,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.81 08:20:13.16 +55:24:10.1
162.56289 34.48907 galactic Lyn Second-epoch detections are separated by 2.1" and 4.7 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 | 08:20:13.16 +55:24:10.1 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.589+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:13.16 +55:24:10.1: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:13.16 +55:24:10.1: 13.48 +/- 0.03 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,2461199.6803,11.81,0.05,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
target 20260608.1803 11.81CV 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 06 08.1803 2461199.6803 12.00 08:23:06.53 +55:21:06.2
162.61172 34.90071 galactic Lyn Second-epoch detections are separated by 1.5" and 4.8 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 | 08:23:06.53 +55:21:06.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.380+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:06.53 +55:21:06.2: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:06.53 +55:21:06.2: 13.64 +/- 0.03 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,2461199.6803,12.00,0.05,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
target 20260608.1803 12.00CV 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 06 08.1803 2461199.6803 11.81 08:21:34.56 +55:16:32.5
162.71178 34.68487 galactic Lyn Second-epoch detections are separated by 2.6" and 5.0 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 | 08:21:34.56 +55:16:32.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.515+/-0.029 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:34.56 +55:16:32.5: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:34.56 +55:16:32.5: 13.39 +/- 0.03 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,2461199.6803,11.81,0.05,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
target 20260608.1803 11.81CV 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 06 08.1803 2461199.6803 11.22 07:40:58.34 +54:34:29.0
163.19140 28.82922 galactic Lyn Second-epoch detections are separated by 0.7" and 5.3 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 985412523023379456 | 07:40:58.26 +54:34:28.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.463+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:58.34 +54:34:29.0: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:58.34 +54:34:29.0: 12.41 +/- 0.01 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 985412523023379456,2461199.6803,11.22,0.05,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 985412523023379456 20260608.1803 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 06 08.1803 2461199.6803 10.89 07:43:37.81 +54:20:34.7
163.50781 29.18463 galactic Lyn Second-epoch detections are separated by 0.5" and 5.2 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 | ATO J115.9065+54.3304 | 07:43:37.81 +54:20:34.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.872+/-0.032 (M)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:37.81 +54:20:34.7: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:37.81 +54:20:34.7: 11.90 +/- 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
ATO J115.9065+54.3304,2461199.6803,10.89,0.05,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
ATO J115.9065+54.3304 20260608.1803 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 06 08.1803 2461199.6803 11.55 08:20:31.20 +54:51:57.2
163.21340 34.54222 galactic Lyn Second-epoch detections are separated by 2.0" and 4.9 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 | 08:20:31.20 +54:51:57.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.378+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:31.20 +54:51:57.2: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:31.20 +54:51:57.2: 13.14 +/- 0.02 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,2461199.6803,11.55,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.67 07:39:35.36 +54:45:36.3
162.95303 28.65413 galactic Lyn Second-epoch detections are separated by 2.8" and 5.6 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 | 07:39:35.36 +54:45:36.3 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.199+/-0.031 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:35.36 +54:45:36.3: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:35.36 +54:45:36.3: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 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,2461199.6803,11.67,0.05,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
target 20260608.1803 11.67CV 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 06 08.1803 2461199.6803 11.52 07:37:07.12 +56:08:12.9
161.34783 28.47841 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 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 986120234850128512 | 07:37:05.02 +56:08:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.516+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:07.12 +56:08:12.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:07.12 +56:08:12.9: 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
Gaia DR3 986120234850128512,2461199.6803,11.52,0.05,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 986120234850128512 20260608.1803 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 06 08.1803 2461199.6803 11.57 08:21:52.15 +53:44:08.1
164.58442 34.75247 galactic Lyn Second-epoch detections are separated by 1.2" and 4.6 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 | 08:21:52.15 +53:44:08.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.400+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:52.15 +53:44:08.1: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:52.15 +53:44:08.1: 12.82 +/- 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
target,2461199.6803,11.57,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.62 07:34:47.64 +56:48:18.1
160.54936 28.24235 galactic Lyn Second-epoch detections are separated by 2.6" and 4.9 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 | 07:34:47.64 +56:48:18.1 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.369+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:34:47.64 +56:48:18.1: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:34:47.64 +56:48:18.1: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 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,2461199.6803,11.62,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.76 07:40:28.25 +54:50:55.9
162.87072 28.79126 galactic Lyn Second-epoch detections are separated by 2.6" and 4.8 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 | 07:40:28.25 +54:50:55.9 (user input) | T | P | (position from user input) J-Ks=0.303+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:28.25 +54:50:55.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:28.25 +54:50:55.9: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 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,2461199.6803,11.76,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.62 07:42:17.58 +54:16:12.4
163.56378 28.98226 galactic Lyn Second-epoch detections are separated by 3.8" and 4.6 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 | 07:42:17.58 +54:16:12.4 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.396+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:17.58 +54:16:12.4: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:17.58 +54:16:12.4: 12.95 +/- 0.02 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,2461199.6803,11.62,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.54 07:42:49.87 +53:55:21.5
163.96916 29.01768 galactic Lyn Second-epoch detections are separated by 2.1" and 4.9 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 | 07:42:49.87 +53:55:21.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.608+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:49.87 +53:55:21.5: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:49.87 +53:55:21.5: 12.78 +/- 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
target,2461199.6803,11.54,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.52 07:50:53.27 +52:02:00.8
166.29117 29.99493 galactic Lyn Second-epoch detections are separated by 2.3" and 5.2 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 984092357451144448 | 07:50:53.36 +52:02:01.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.636+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:50:53.27 +52:02:00.8: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:50:53.27 +52:02:00.8: 12.39 +/- 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 984092357451144448,2461199.6803,11.52,0.05,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 984092357451144448 20260608.1803 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 06 08.1803 2461199.6803 11.76 07:44:18.63 +54:02:10.9
163.87009 29.24734 galactic Lyn Second-epoch detections are separated by 2.2" and 5.5 pix
The object was found in VSX 0" Gaia DR3 984589852103425664
Type: ROT
# Max. Min./Amp. JD0 Period
13.000 G 13.040 G G
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:18.63 +54:02:10.9: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:18.63 +54:02:10.9: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 984589852103425664,2461199.6803,11.76,0.05,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
Gaia DR3 984589852103425664 20260608.1803 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 06 08.1803 2461199.6803 11.63 08:20:20.60 +54:25:09.5
163.75587 34.52260 galactic Lyn Second-epoch detections are separated by 1.1" and 4.9 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 | 08:20:20.60 +54:25:09.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.605+/-0.027 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:20.60 +54:25:09.5: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:20.60 +54:25:09.5: 13.37 +/- 0.03 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,2461199.6803,11.63,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.54 08:22:40.17 +55:45:09.4
162.12592 34.82532 galactic Lyn Second-epoch detections are separated by 1.6" and 4.7 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 | 08:22:40.17 +55:45:09.4 (user input) | T | P | (position from user input) J-Ks=0.386+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:40.17 +55:45:09.4: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:40.17 +55:45:09.4: 13.05 +/- 0.02 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,2461199.6803,11.54,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.32 08:18:00.44 +54:14:37.9
163.97048 34.18297 galactic Lyn Second-epoch detections are separated by 0.7" and 4.9 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 1032248802084135168 | 08:18:00.46 +54:14:38.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.370+/-0.027 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:18:00.44 +54:14:37.9: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:18:00.44 +54:14:37.9: 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 1032248802084135168,2461199.6803,11.32,0.05,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
Gaia DR3 1032248802084135168 20260608.1803 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 06 08.1803 2461199.6803 11.72 07:36:42.06 +55:25:31.8
162.14166 28.33009 galactic Lyn Second-epoch detections are separated by 0.7" and 5.1 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 | 07:36:42.06 +55:25:31.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.390+/-0.036 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:42.06 +55:25:31.8: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:42.06 +55:25:31.8: 13.24 +/- 0.03 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,2461199.6803,11.72,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.22 07:35:57.44 +56:32:21.2
160.87139 28.36806 galactic Lyn Second-epoch detections are separated by 2.4" and 5.4 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 986146790631801344 | 07:35:57.45 +56:32:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.565+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:57.44 +56:32:21.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:57.44 +56:32:21.2: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 986146790631801344,2461199.6803,11.22,0.05,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 986146790631801344 20260608.1803 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 06 08.1803 2461199.6803 11.32 07:51:42.67 +52:18:52.1
165.98518 30.15220 galactic Lyn Second-epoch detections are separated by 0.2" and 5.2 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 984195711544385920 | 07:51:42.64 +52:18:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5) J-Ks=0.340+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:51:42.67 +52:18:52.1: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:51:42.67 +52:18:52.1: 12.42 +/- 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 984195711544385920,2461199.6803,11.32,0.05,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
Gaia DR3 984195711544385920 20260608.1803 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 06 08.1803 2461199.6803 11.25 08:25:25.27 +54:28:25.1
163.67189 35.25952 galactic Lyn Second-epoch detections are separated by 1.1" and 4.8 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 | Gaia DR3 1032114829168488704 | 08:25:25.30 +54:28:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.357+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:25.27 +54:28:25.1: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:25.27 +54:28:25.1: 12.31 +/- 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 1032114829168488704,2461199.6803,11.25,0.05,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 1032114829168488704 20260608.1803 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 06 08.1803 2461199.6803 11.66 07:41:58.99 +54:53:17.2
162.85616 29.01198 galactic Lyn Second-epoch detections are separated by 3.2" and 4.7 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 | 07:41:58.99 +54:53:17.2 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.288+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:58.99 +54:53:17.2: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:58.99 +54:53:17.2: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 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,2461199.6803,11.66,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.12 08:21:31.30 +54:10:09.5
164.05733 34.69724 galactic Lyn Second-epoch detections are separated by 0.7" and 4.8 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 | Gaia DR3 1032207085066650496 | 08:21:31.31 +54:10:09.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.129+/-0.033 (A)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:31.30 +54:10:09.5: 16.31 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:31.30 +54:10:09.5: 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 1032207085066650496,2461199.6803,11.12,0.05,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 1032207085066650496 20260608.1803 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 06 08.1803 2461199.6803 11.12 08:23:14.65 +55:43:12.6
162.16193 34.90731 galactic Lyn Second-epoch detections are separated by 1.6" and 4.6 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 1033931772133430784 | 08:23:14.65 +55:43:12.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.320+/-0.025 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:14.65 +55:43:12.6: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:14.65 +55:43:12.6: 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 1033931772133430784,2461199.6803,11.12,0.05,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 1033931772133430784 20260608.1803 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 06 08.1803 2461199.6803 11.79 08:24:03.76 +55:39:09.9
162.23884 35.02512 galactic Lyn Second-epoch detections are separated by 2.3" and 4.7 pix
The object was found in VSX 1" Gaia DR3 1033883878953833600
Type: E
# Max. Min./Amp. JD0 Period
12.970 G 13.110 G 0.809240000000 F
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:03.76 +55:39:09.9: 16.32 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:03.76 +55:39:09.9: 13.18 +/- 0.02 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
Gaia DR3 1033883878953833600,2461199.6803,11.79,0.05,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
Gaia DR3 1033883878953833600 20260608.1803 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 06 08.1803 2461199.6803 11.66 07:46:32.64 +53:32:12.8
164.48360 29.51661 galactic Lyn Second-epoch detections are separated by 1.0" and 5.0 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 | 07:46:32.64 +53:32:12.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.414+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:46:32.64 +53:32:12.8: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:46:32.64 +53:32:12.8: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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,2461199.6803,11.66,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.54 08:23:03.29 +54:55:55.7
163.12339 34.90512 galactic Lyn Second-epoch detections are separated by 2.2" and 4.4 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 | 08:23:03.29 +54:55:55.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:03.29 +54:55:55.7: 14.16 +/- 0.05 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:03.29 +54:55:55.7: 12.98 +/- 0.02 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,2461199.6803,11.54,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.70 08:23:07.38 +54:01:29.0
164.22957 34.93392 galactic Lyn Second-epoch detections are separated by 2.0" and 4.9 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 | 08:23:07.38 +54:01:29.0 (user input) | T | P | (position from user input) J-Ks=0.629+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:07.38 +54:01:29.0: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:07.38 +54:01:29.0: 13.23 +/- 0.02 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,2461199.6803,11.70,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.23 07:37:24.57 +54:13:19.4
163.51160 28.26875 galactic Lyn Second-epoch detections are separated by 0.4" and 5.1 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 | ATO J114.3529+54.2281 | 07:37:24.50 +54:13:19.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.303+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:24.57 +54:13:19.4: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:24.57 +54:13:19.4: 12.44 +/- 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
ATO J114.3529+54.2281,2461199.6803,11.23,0.05,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
ATO J114.3529+54.2281 20260608.1803 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 06 08.1803 2461199.6803 11.26 07:39:38.17 +55:48:47.4
161.76209 28.78926 galactic Lyn Second-epoch detections are separated by 1.9" and 5.2 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 986050244063128960 | 07:39:38.19 +55:48:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.291+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:38.17 +55:48:47.4: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:38.17 +55:48:47.4: 12.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 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 986050244063128960,2461199.6803,11.26,0.05,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 986050244063128960 20260608.1803 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 06 08.1803 2461199.6803 11.71 08:22:02.47 +53:46:30.7
164.53596 34.77757 galactic Lyn Second-epoch detections are separated by 0.9" and 4.7 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 | 08:22:02.47 +53:46:30.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.409+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:02.47 +53:46:30.7: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:02.47 +53:46:30.7: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 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,2461199.6803,11.71,0.05,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
target 20260608.1803 11.71CV 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 06 08.1803 2461199.6803 11.76 07:47:19.74 +53:23:26.8
164.66591 29.61588 galactic Lyn Second-epoch detections are separated by 2.6" and 4.9 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 | 07:47:19.74 +53:23:26.8 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.577+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:47:19.74 +53:23:26.8: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:47:19.74 +53:23:26.8: 13.06 +/- 0.02 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,2461199.6803,11.76,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.83 07:46:14.97 +54:29:08.2
163.39428 29.57931 galactic Lyn Second-epoch detections are separated by 3.4" and 5.7 pix
The object was found in VSX 1" Gaia DR3 984982270379965696
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.940 G 12.980 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:46:14.97 +54:29:08.2: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:46:14.97 +54:29:08.2: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 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 984982270379965696,2461199.6803,11.83,0.05,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
Gaia DR3 984982270379965696 20260608.1803 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 06 08.1803 2461199.6803 11.54 07:35:36.22 +56:18:23.6
161.12673 28.29057 galactic Lyn Second-epoch detections are separated by 2.4" and 5.2 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 | 07:35:36.22 +56:18:23.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.401+/-0.035 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:36.22 +56:18:23.6: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:36.22 +56:18:23.6: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 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,2461199.6803,11.54,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.59 08:18:40.44 +54:53:54.8
163.17805 34.27633 galactic Lyn Second-epoch detections are separated by 1.1" and 4.9 pix
The object was found in VSX 3" Gaia DR3 1032303708945949568
Type: L
# Max. Min./Amp. JD0 Period
12.460 G 13.090 G M
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:18:40.44 +54:53:54.8: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:18:40.44 +54:53:54.8: 13.25 +/- 0.02 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
Gaia DR3 1032303708945949568,2461199.6803,11.59,0.05,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
Gaia DR3 1032303708945949568 20260608.1803 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 06 08.1803 2461199.6803 11.26 08:24:38.04 +53:27:22.1
164.92004 35.16564 galactic Lyn Second-epoch detections are separated by 1.3" and 4.6 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 1031940728374383616 | 08:24:38.05 +53:27:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5) J-Ks=0.561+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:38.04 +53:27:22.1: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:38.04 +53:27:22.1: 12.31 +/- 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 1031940728374383616,2461199.6803,11.26,0.05,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 1031940728374383616 20260608.1803 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 06 08.1803 2461199.6803 11.05 08:22:37.10 +54:57:33.1
163.09238 34.84177 galactic Lyn Second-epoch detections are separated by 1.0" and 4.6 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 1032362597242031616 | 08:22:37.14 +54:57:33.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.334+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:37.10 +54:57:33.1: 16.09 +/- 0.30 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:37.10 +54:57:33.1: 12.26 +/- 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 1032362597242031616,2461199.6803,11.05,0.05,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 1032362597242031616 20260608.1803 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 06 08.1803 2461199.6803 11.30 07:48:53.14 +52:51:05.1
165.31354 29.78616 galactic Lyn Second-epoch detections are separated by 1.3" and 5.3 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 984272058882698624 | 07:48:55.62 +52:51:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.415+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:48:53.14 +52:51:05.1: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:48:53.14 +52:51:05.1: 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 984272058882698624,2461199.6803,11.30,0.05,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 984272058882698624 20260608.1803 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 06 08.1803 2461199.6803 10.83 07:36:54.13 +55:53:12.8
161.62573 28.41735 galactic Lyn Second-epoch detections are separated by 0.9" and 5.2 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 986089684746866688 | 07:36:54.18 +55:53:12.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.460+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:54.13 +55:53:12.8: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:54.13 +55:53:12.8: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 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 986089684746866688,2461199.6803,10.83,0.05,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 986089684746866688 20260608.1803 10.83CV 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 06 08.1803 2461199.6803 10.89 07:34:37.63 +56:53:42.1
160.44478 28.23091 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 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 | ATO J113.6570+56.8951 | 07:34:37.68 +56:53:42.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.417+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:34:37.63 +56:53:42.1: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:34:37.63 +56:53:42.1: 11.96 +/- 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
ATO J113.6570+56.8951,2461199.6803,10.89,0.05,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
ATO J113.6570+56.8951 20260608.1803 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 06 08.1803 2461199.6803 10.69 08:22:26.98 +55:21:55.0
162.59868 34.80667 galactic Lyn Second-epoch detections are separated by 0.1" and 4.8 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 | Gaia DR3 1032424277267921792 | 08:22:26.99 +55:21:55.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5) J-Ks=0.550+/-0.027 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:26.98 +55:21:55.0: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:26.98 +55:21:55.0: 11.74 +/- 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 1032424277267921792,2461199.6803,10.69,0.05,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 1032424277267921792 20260608.1803 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 06 08.1803 2461199.6803 10.67 08:21:49.94 +55:34:36.4
162.34449 34.71300 galactic Lyn Second-epoch detections are separated by 0.7" and 4.8 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 | Gaia DR3 1032431797755034752 | 08:21:49.95 +55:34:37.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5) J-Ks=0.312+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:49.94 +55:34:36.4: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:49.94 +55:34:36.4: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 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 1032431797755034752,2461199.6803,10.67,0.05,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 1032431797755034752 20260608.1803 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 06 08.1803 2461199.6803 10.78 07:38:41.65 +54:45:44.0
162.93170 28.52636 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 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 985432318528956544 | 07:38:41.64 +54:45:43.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5) J-Ks=0.309+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:41.65 +54:45:44.0: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:41.65 +54:45:44.0: 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 985432318528956544,2461199.6803,10.78,0.05,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 985432318528956544 20260608.1803 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 06 08.1803 2461199.6803 11.38 07:38:42.35 +56:15:56.9
161.23206 28.71293 galactic Lyn Second-epoch detections are separated by 1.5" and 5.3 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 986124181924205568 | 07:38:42.40 +56:15:55.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5) J-Ks=0.152+/-0.031 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:42.35 +56:15:56.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:42.35 +56:15:56.9: 12.42 +/- 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 986124181924205568,2461199.6803,11.38,0.05,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 986124181924205568 20260608.1803 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 06 08.1803 2461199.6803 11.64 07:41:51.68 +54:14:53.6
163.57971 28.91700 galactic Lyn Second-epoch detections are separated by 1.1" and 5.0 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 | 07:41:51.68 +54:14:53.6 (user input) | T | P | (position from user input) J-Ks=0.232+/-0.031 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:51.68 +54:14:53.6: 15.46 +/- 0.24 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:51.68 +54:14:53.6: 12.89 +/- 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,2461199.6803,11.64,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.20 07:42:36.30 +54:37:51.7
163.16027 29.07073 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 | 07:42:36.30 +54:37:51.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.333+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:36.30 +54:37:51.7: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:36.30 +54:37:51.7: 12.34 +/- 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
target,2461199.6803,11.20,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.30 08:24:30.55 +54:40:25.7
163.43171 35.12166 galactic Lyn Second-epoch detections are separated by 1.6" and 4.6 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 1032155858991732224 | 08:24:30.52 +54:40:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.281+/-0.025 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:30.55 +54:40:25.7: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:30.55 +54:40:25.7: 12.28 +/- 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 1032155858991732224,2461199.6803,11.30,0.05,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 1032155858991732224 20260608.1803 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 06 08.1803 2461199.6803 11.05 07:35:07.53 +56:24:08.6
161.00929 28.23700 galactic Lyn Second-epoch detections are separated by 0.7" and 5.1 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 989140657715650432 | 07:35:07.44 +56:24:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.684+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:07.53 +56:24:08.6: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:07.53 +56:24:08.6: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 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 989140657715650432,2461199.6803,11.05,0.05,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 989140657715650432 20260608.1803 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 06 08.1803 2461199.6803 11.64 07:41:50.86 +54:06:49.1
163.73196 28.89820 galactic Lyn Second-epoch detections are separated by 3.1" and 5.6 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 | 07:41:50.86 +54:06:49.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.131+/-0.032 (A)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:50.86 +54:06:49.1: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:50.86 +54:06:49.1: 12.89 +/- 0.02 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,2461199.6803,11.64,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.52 07:39:48.71 +55:13:56.6
162.42329 28.74458 galactic Lyn Second-epoch detections are separated by 0.4" and 5.3 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 | 07:39:48.71 +55:13:56.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.382+/-0.035 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:48.71 +55:13:56.6: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:48.71 +55:13:56.6: 12.93 +/- 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
target,2461199.6803,11.52,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.87 07:38:05.39 +55:48:16.8
161.74208 28.57256 galactic Lyn Second-epoch detections are separated by 2.8" and 5.3 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 | 07:38:05.39 +55:48:16.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.418+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:05.39 +55:48:16.8: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:05.39 +55:48:16.8: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 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,2461199.6803,11.87,0.05,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
target 20260608.1803 11.87CV 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 06 08.1803 2461199.6803 11.71 07:45:45.34 +53:56:15.1
164.01103 29.44685 galactic Lyn Second-epoch detections are separated by 2.1" and 4.9 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 | 07:45:45.34 +53:56:15.1 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.281+/-0.032 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:45:45.34 +53:56:15.1: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:45:45.34 +53:56:15.1: 13.08 +/- 0.02 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,2461199.6803,11.71,0.05,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
target 20260608.1803 11.71CV 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 06 08.1803 2461199.6803 11.73 07:56:24.25 +51:18:20.8
167.23945 30.76428 galactic Lyn Second-epoch detections are separated by 1.7" and 5.1 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 | 07:56:24.25 +51:18:20.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.346+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:56:24.25 +51:18:20.8: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:56:24.25 +51:18:20.8: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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,2461199.6803,11.73,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.71 08:22:18.69 +55:14:58.2
162.74030 34.79030 galactic Lyn Second-epoch detections are separated by 2.3" and 4.4 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 | 08:22:18.69 +55:14:58.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.253+/-0.034 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:18.69 +55:14:58.2: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:18.69 +55:14:58.2: 13.70 +/- 0.04 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,2461199.6803,11.71,0.05,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
target 20260608.1803 11.71CV 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 06 08.1803 2461199.6803 11.37 08:22:19.19 +55:49:25.3
162.04148 34.77374 galactic Lyn Second-epoch detections are separated by 0.9" and 4.6 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 | 08:22:19.19 +55:49:25.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.307+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:19.19 +55:49:25.3: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:19.19 +55:49:25.3: 12.75 +/- 0.01 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,2461199.6803,11.37,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.45 08:22:57.08 +54:47:31.3
163.29463 34.89376 galactic Lyn Second-epoch detections are separated by 0.6" and 4.7 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 | 08:22:57.08 +54:47:31.3 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.396+/-0.027 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:57.08 +54:47:31.3: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:57.08 +54:47:31.3: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 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,2461199.6803,11.45,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.69 07:37:55.92 +55:58:52.9
161.53931 28.57212 galactic Lyn Second-epoch detections are separated by 0.7" and 5.3 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 | 07:37:55.92 +55:58:52.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.320+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:55.92 +55:58:52.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:55.92 +55:58:52.9: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 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,2461199.6803,11.69,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.75 07:36:26.43 +55:43:01.1
161.80789 28.33139 galactic Lyn Second-epoch detections are separated by 0.5" and 5.1 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 986081030388745344 | 07:36:26.44 +55:43:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.710+/-0.029 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:26.43 +55:43:01.1: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:26.43 +55:43:01.1: 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 986081030388745344,2461199.6803,10.75,0.05,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 986081030388745344 20260608.1803 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 06 08.1803 2461199.6803 10.78 07:38:27.15 +55:26:21.1
162.16226 28.57825 galactic Lyn Second-epoch detections are separated by 1.4" and 5.0 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 986026776361898496 | 07:38:27.05 +55:26:21.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.691+/-0.029 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:27.15 +55:26:21.1: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:27.15 +55:26:21.1: 11.82 +/- 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 986026776361898496,2461199.6803,10.78,0.05,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 986026776361898496 20260608.1803 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 06 08.1803 2461199.6803 11.63 07:40:06.52 +55:41:14.5
161.91356 28.84060 galactic Lyn Second-epoch detections are separated by 1.1" and 5.3 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 | 07:40:06.52 +55:41:14.5 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.421+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:06.52 +55:41:14.5: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:06.52 +55:41:14.5: 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,2461199.6803,11.63,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.52 08:24:04.86 +55:47:30.2
162.06915 35.02220 galactic Lyn Second-epoch detections are separated by 2.0" and 4.9 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 | ATO J126.0206+55.7918 | 08:24:04.96 +55:47:30.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.925+/-0.028 (M)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:04.86 +55:47:30.2: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:04.86 +55:47:30.2: 12.70 +/- 0.01 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
ATO J126.0206+55.7918,2461199.6803,11.52,0.05,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
ATO J126.0206+55.7918 20260608.1803 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 06 08.1803 2461199.6803 11.52 07:41:36.53 +53:47:29.7
164.09157 28.82228 galactic Lyn Second-epoch detections are separated by 1.8" and 4.9 pix
The object was found in VSX 1" ZTF J074136.45+534730.1
Type: EW
# Max. Min./Amp. JD0 Period
12.568 g Y 0.196 g 2458422.96280 0.595937200000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:36.53 +53:47:29.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:36.53 +53:47:29.7: 12.47 +/- 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
ZTF J074136.45+534730.1,2461199.6803,11.52,0.05,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
ZTF J074136.45+534730.1 20260608.1803 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 06 08.1803 2461199.6803 11.66 07:37:14.26 +55:41:09.7
161.85907 28.43882 galactic Lyn Second-epoch detections are separated by 1.4" and 5.4 pix
The object was found in VSX 1" Gaia DR3 986080137035539968
Type: ROT
# Max. Min./Amp. JD0 Period
12.850 G 12.870 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:14.26 +55:41:09.7: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:14.26 +55:41:09.7: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 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 986080137035539968,2461199.6803,11.66,0.05,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
Gaia DR3 986080137035539968 20260608.1803 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 06 08.1803 2461199.6803 11.58 07:39:43.97 +54:33:22.6
163.18639 28.64867 galactic Lyn Second-epoch detections are separated by 0.9" and 5.1 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 | 07:39:43.97 +54:33:22.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.344+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:43.97 +54:33:22.6: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:43.97 +54:33:22.6: 12.87 +/- 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,2461199.6803,11.58,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.60 07:54:46.95 +51:55:10.4
166.49902 30.57845 galactic Lyn Second-epoch detections are separated by 0.5" and 5.0 pix
The object was found in VSX 0" ASASSN-V J075446.93+515510.1
Type: EA
# Max. Min./Amp. JD0 Period
13.150 g Y 0.300 g 2458179.74500 2.936400000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:54:46.95 +51:55:10.4: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:54:46.95 +51:55:10.4: 12.97 +/- 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
ASASSN-V J075446.93+515510.1,2461199.6803,11.60,0.05,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
ASASSN-V J075446.93+515510.1 20260608.1803 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 06 08.1803 2461199.6803 11.74 07:34:56.89 +57:09:27.7
160.15486 28.30640 galactic Lyn Second-epoch detections are separated by 2.8" and 5.0 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 | 07:34:56.89 +57:09:27.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.324+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:34:56.89 +57:09:27.7: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:34:56.89 +57:09:27.7: 12.89 +/- 0.02 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,2461199.6803,11.74,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.60 08:23:49.90 +53:22:50.8
165.01389 35.04700 galactic Lyn Second-epoch detections are separated by 0.8" and 5.0 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 | 08:23:49.90 +53:22:50.8 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.335+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:49.90 +53:22:50.8: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:49.90 +53:22:50.8: 12.76 +/- 0.01 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,2461199.6803,11.60,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.53 07:41:45.73 +55:08:48.5
162.55814 29.01077 galactic Lyn Second-epoch detections are separated by 1.0" and 5.2 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 | 07:41:45.73 +55:08:48.5 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.552+/-0.032 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:45.73 +55:08:48.5: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:45.73 +55:08:48.5: 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,2461199.6803,11.53,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.62 07:46:56.91 +53:09:44.8
164.91908 29.53287 galactic Lyn Second-epoch detections are separated by 3.9" and 4.7 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 | 07:46:56.91 +53:09:44.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.486+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:46:56.91 +53:09:44.8: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:46:56.91 +53:09:44.8: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 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,2461199.6803,11.62,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.52 07:41:27.42 +54:17:45.6
163.51716 28.86439 galactic Lyn Second-epoch detections are separated by 1.8" and 5.5 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 | 07:41:27.42 +54:17:45.6 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.618+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:27.42 +54:17:45.6: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:27.42 +54:17:45.6: 12.84 +/- 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,2461199.6803,11.52,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.61 07:35:06.70 +56:38:01.5
160.74846 28.26424 galactic Lyn Second-epoch detections are separated by 1.8" and 4.9 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 | 07:35:06.70 +56:38:01.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.721+/-0.034 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:06.70 +56:38:01.5: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:06.70 +56:38:01.5: 13.18 +/- 0.03 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,2461199.6803,11.61,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.69 08:23:37.39 +53:38:58.1
164.68621 35.01296 galactic Lyn Second-epoch detections are separated by 1.7" and 4.6 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 | 08:23:37.39 +53:38:58.1 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:37.39 +53:38:58.1: 16.31 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:37.39 +53:38:58.1: 13.06 +/- 0.02 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,2461199.6803,11.69,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.10 08:22:59.77 +54:42:06.7
163.40435 34.90237 galactic Lyn Second-epoch detections are separated by 0.9" and 4.7 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 1032320407778933888 | 08:22:59.79 +54:42:06.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.258+/-0.026 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:59.77 +54:42:06.7: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:59.77 +54:42:06.7: 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 1032320407778933888,2461199.6803,11.10,0.05,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 1032320407778933888 20260608.1803 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 06 08.1803 2461199.6803 11.29 07:45:48.55 +54:15:16.3
163.65025 29.49034 galactic Lyn Second-epoch detections are separated by 2.6" and 4.8 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 | Gaia DR3 984970317486632320 | 07:45:48.57 +54:15:15.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5) J-Ks=0.284+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:45:48.55 +54:15:16.3: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:45:48.55 +54:15:16.3: 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 984970317486632320,2461199.6803,11.29,0.05,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 984970317486632320 20260608.1803 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 06 08.1803 2461199.6803 10.81 07:38:10.52 +55:46:39.3
161.77436 28.58118 galactic Lyn Second-epoch detections are separated by 0.9" and 5.2 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 986040692055881984 | 07:38:10.56 +55:46:38.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.592+/-0.032 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:10.52 +55:46:39.3: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:10.52 +55:46:39.3: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.88 +/- 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 986040692055881984,2461199.6803,10.81,0.05,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 986040692055881984 20260608.1803 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 06 08.1803 2461199.6803 10.71 07:36:35.60 +54:58:12.0
162.65205 28.25433 galactic Lyn Second-epoch detections are separated by 0.7" and 5.3 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 985615073681024768 | 07:36:35.61 +54:58:11.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.431+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:35.60 +54:58:12.0: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:35.60 +54:58:12.0: 11.89 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.89 +/- 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 985615073681024768,2461199.6803,10.71,0.05,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 985615073681024768 20260608.1803 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 06 08.1803 2461199.6803 11.32 07:46:43.83 +54:19:28.3
163.58712 29.63162 galactic Lyn Second-epoch detections are separated by 1.0" and 5.3 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 984971687580547968 | 07:46:43.84 +54:19:28.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.592+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:46:43.83 +54:19:28.3: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:46:43.83 +54:19:28.3: 12.29 +/- 0.01 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 984971687580547968,2461199.6803,11.32,0.05,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
Gaia DR3 984971687580547968 20260608.1803 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 06 08.1803 2461199.6803 11.30 08:25:06.82 +55:07:08.6
162.88397 35.19420 galactic Lyn Second-epoch detections are separated by 0.2" and 4.8 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 | Gaia DR3 1032356584287639424 | 08:25:06.80 +55:07:08.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.270+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:06.82 +55:07:08.6: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:06.82 +55:07:08.6: 12.21 +/- 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 1032356584287639424,2461199.6803,11.30,0.05,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 1032356584287639424 20260608.1803 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 06 08.1803 2461199.6803 11.16 07:37:02.14 +55:41:37.4
161.84629 28.41156 galactic Lyn Second-epoch detections are separated by 2.0" and 4.9 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 986080373257776000 | 07:37:02.25 +55:41:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.366+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:02.14 +55:41:37.4: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:02.14 +55:41:37.4: 12.38 +/- 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 986080373257776000,2461199.6803,11.16,0.05,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 986080373257776000 20260608.1803 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 06 08.1803 2461199.6803 10.97 08:20:29.59 +54:29:58.5
163.65813 34.54348 galactic Lyn Second-epoch detections are separated by 0.5" and 4.9 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 1032232373833713024 | 08:20:29.65 +54:29:59.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.418+/-0.027 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:29.59 +54:29:58.5: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:29.59 +54:29:58.5: 12.21 +/- 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 1032232373833713024,2461199.6803,10.97,0.05,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 1032232373833713024 20260608.1803 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 06 08.1803 2461199.6803 11.20 08:22:47.67 +53:36:29.4
164.73824 34.89057 galactic Lyn Second-epoch detections are separated by 1.0" and 4.7 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 1031970380828588544 | 08:22:47.70 +53:36:29.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.812+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:47.67 +53:36:29.4: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:47.67 +53:36:29.4: 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 1031970380828588544,2461199.6803,11.20,0.05,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 1031970380828588544 20260608.1803 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 06 08.1803 2461199.6803 11.25 07:44:28.28 +54:56:12.7
162.84710 29.37276 galactic Lyn Second-epoch detections are separated by 2.5" and 5.1 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 985754922112336384 | 07:44:28.20 +54:56:12.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.440+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:28.28 +54:56:12.7: 13.83 +/- 0.05 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:28.28 +54:56:12.7: 12.27 +/- 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 985754922112336384,2461199.6803,11.25,0.05,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 985754922112336384 20260608.1803 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 06 08.1803 2461199.6803 11.25 08:29:58.98 +52:39:36.2
165.88051 35.98376 galactic Lyn Second-epoch detections are separated by 0.4" and 4.8 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 | ATO J127.4956+52.6599 | 08:29:58.96 +52:39:35.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.329+/-0.027 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:29:58.98 +52:39:36.2: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:29:58.98 +52:39:36.2: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 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 J127.4956+52.6599,2461199.6803,11.25,0.05,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
ATO J127.4956+52.6599 20260608.1803 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 06 08.1803 2461199.6803 11.57 07:53:52.09 +52:21:54.6
165.96757 30.48520 galactic Lyn Second-epoch detections are separated by 2.7" and 5.3 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 | ATO J118.4683+52.3632 | 07:53:52.09 +52:21:54.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.331+/-0.037 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:53:52.09 +52:21:54.6: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:53:52.09 +52:21:54.6: 12.78 +/- 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
ATO J118.4683+52.3632,2461199.6803,11.57,0.05,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
ATO J118.4683+52.3632 20260608.1803 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 06 08.1803 2461199.6803 11.54 07:36:52.27 +56:32:22.5
160.88835 28.49314 galactic Lyn Second-epoch detections are separated by 1.8" and 5.2 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 | 07:36:52.27 +56:32:22.5 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:52.27 +56:32:22.5: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:52.27 +56:32:22.5: 12.93 +/- 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
target,2461199.6803,11.54,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.23 07:40:21.75 +55:07:44.6
162.55120 28.81006 galactic Lyn Second-epoch detections are separated by 1.0" and 5.0 pix
The object was found in VSX 1" Gaia DR3 985818521988026880
Type: VAR
# Max. Min./Amp. JD0 Period
12.220 G 12.240 G 0.084161300000 F
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:21.75 +55:07:44.6: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:21.75 +55:07:44.6: 12.35 +/- 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 985818521988026880,2461199.6803,11.23,0.05,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 985818521988026880 20260608.1803 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 06 08.1803 2461199.6803 11.25 07:43:47.07 +54:44:17.4
163.06097 29.25243 galactic Lyn Second-epoch detections are separated by 0.9" and 5.1 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 985746087363657472 | 07:43:47.00 +54:44:17.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.376+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:47.07 +54:44:17.4: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:47.07 +54:44:17.4: 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 985746087363657472,2461199.6803,11.25,0.05,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 985746087363657472 20260608.1803 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 06 08.1803 2461199.6803 11.31 07:43:25.33 +53:45:35.5
164.16629 29.08401 galactic Lyn Second-epoch detections are separated by 0.4" and 5.2 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 984561333520648576 | 07:43:25.37 +53:45:36.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.280+/-0.026 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:25.33 +53:45:35.5: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:25.33 +53:45:35.5: 12.29 +/- 0.01 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 984561333520648576,2461199.6803,11.31,0.05,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 984561333520648576 20260608.1803 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 06 08.1803 2461199.6803 11.34 08:30:26.59 +50:48:42.7
168.16474 36.07680 galactic Lyn Second-epoch detections are separated by 2.0" and 4.6 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 1028098454927026432 | 08:30:26.52 +50:48:43.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.665+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:30:26.59 +50:48:42.7: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:30:26.59 +50:48:42.7: 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 1028098454927026432,2461199.6803,11.34,0.05,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
Gaia DR3 1028098454927026432 20260608.1803 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 06 08.1803 2461199.6803 11.54 07:50:14.95 +52:35:55.8
165.62998 29.96260 galactic Lyn Second-epoch detections are separated by 2.5" and 5.5 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 | 07:50:14.95 +52:35:55.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.323+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:50:14.95 +52:35:55.8: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:50:14.95 +52:35:55.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 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,2461199.6803,11.54,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.41 08:21:17.65 +55:52:24.3
161.98678 34.62824 galactic Lyn Second-epoch detections are separated by 0.4" and 4.7 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 | 08:21:17.65 +55:52:24.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.425+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:17.65 +55:52:24.3: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:17.65 +55:52:24.3: 12.66 +/- 0.01 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,2461199.6803,11.41,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.62 07:57:21.96 +51:38:20.2
166.87125 30.94739 galactic Lyn Second-epoch detections are separated by 2.3" and 5.0 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 | ATO J119.3416+51.6391 | 07:57:21.96 +51:38:20.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.384+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:57:21.96 +51:38:20.2: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:57:21.96 +51:38:20.2: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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
ATO J119.3416+51.6391,2461199.6803,11.62,0.05,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
ATO J119.3416+51.6391 20260608.1803 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 06 08.1803 2461199.6803 11.55 07:48:20.02 +53:32:46.9
164.50719 29.78186 galactic Lyn Second-epoch detections are separated by 0.6" and 5.2 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 | 07:48:20.02 +53:32:46.9 (user input) | T | P | (position from user input) J-Ks=0.323+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:48:20.02 +53:32:46.9: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:48:20.02 +53:32:46.9: 12.73 +/- 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
target,2461199.6803,11.55,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.74 07:43:16.14 +54:57:39.5
162.79769 29.20387 galactic Lyn Second-epoch detections are separated by 2.5" and 5.4 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 | ATO J115.8087+54.9687 | 07:43:16.14 +54:57:39.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.716+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:16.14 +54:57:39.5: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:16.14 +54:57:39.5: 12.91 +/- 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
ATO J115.8087+54.9687,2461199.6803,11.74,0.05,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
ATO J115.8087+54.9687 20260608.1803 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 06 08.1803 2461199.6803 11.63 07:35:59.53 +56:25:04.9
161.00874 28.35789 galactic Lyn Second-epoch detections are separated by 0.7" and 5.0 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 | 07:35:59.53 +56:25:04.9 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.306+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:59.53 +56:25:04.9: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:59.53 +56:25:04.9: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 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,2461199.6803,11.63,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.39 07:36:46.02 +56:13:11.0
161.24752 28.44001 galactic Lyn Second-epoch detections are separated by 1.6" and 5.4 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 | 07:36:46.02 +56:13:11.0 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:46.02 +56:13:11.0: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:46.02 +56:13:11.0: 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,2461199.6803,11.39,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.63 07:42:20.10 +53:55:41.9
163.95230 28.94592 galactic Lyn Second-epoch detections are separated by 0.8" and 5.1 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 | ATO J115.5840+53.9280 | 07:42:20.10 +53:55:41.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.333+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:20.10 +53:55:41.9: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:20.10 +53:55:41.9: 12.82 +/- 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
ATO J115.5840+53.9280,2461199.6803,11.63,0.05,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
ATO J115.5840+53.9280 20260608.1803 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 06 08.1803 2461199.6803 11.60 07:46:00.03 +53:30:06.5
164.51280 29.43229 galactic Lyn Second-epoch detections are separated by 1.5" and 5.0 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 | 07:46:00.03 +53:30:06.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.352+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:46:00.03 +53:30:06.5: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:46:00.03 +53:30:06.5: 12.80 +/- 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,2461199.6803,11.60,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.07 08:21:29.96 +55:52:09.2
161.99077 34.65714 galactic Lyn Second-epoch detections are separated by 0.5" and 4.7 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 1033950777364407552 | 08:21:29.99 +55:52:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.270+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:29.96 +55:52:09.2: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:29.96 +55:52:09.2: 12.21 +/- 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 1033950777364407552,2461199.6803,11.07,0.05,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 1033950777364407552 20260608.1803 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 06 08.1803 2461199.6803 11.12 08:22:47.63 +53:55:31.4
164.35153 34.88694 galactic Lyn Second-epoch detections are separated by 0.7" and 4.9 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 1032001442032067840 | 08:22:47.65 +53:55:31.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.527+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:47.63 +53:55:31.4: 16.31 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:47.63 +53:55:31.4: 12.21 +/- 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 1032001442032067840,2461199.6803,11.12,0.05,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 1032001442032067840 20260608.1803 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 06 08.1803 2461199.6803 11.20 08:25:07.47 +54:53:40.7
163.15837 35.20352 galactic Lyn Second-epoch detections are separated by 1.2" and 4.6 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 1032165578502047360 | 08:25:07.58 +54:53:41.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.436+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:07.47 +54:53:40.7: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:07.47 +54:53:40.7: 12.17 +/- 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 1032165578502047360,2461199.6803,11.20,0.05,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 1032165578502047360 20260608.1803 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 06 08.1803 2461199.6803 11.25 07:45:23.81 +53:26:10.0
164.57539 29.33528 galactic Lyn Second-epoch detections are separated by 1.0" and 5.1 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 984533364693934592 | 07:45:23.80 +53:26:09.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.275+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:45:23.81 +53:26:10.0: 15.67 +/- 0.26 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:45:23.81 +53:26:10.0: 12.27 +/- 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 984533364693934592,2461199.6803,11.25,0.05,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 984533364693934592 20260608.1803 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 06 08.1803 2461199.6803 11.25 08:30:15.42 +51:18:45.9
167.54526 36.04569 galactic Lyn Second-epoch detections are separated by 1.8" and 5.1 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 1028144153379013760 | 08:30:15.44 +51:18:45.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.303+/-0.029 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:30:15.42 +51:18:45.9: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:30:15.42 +51:18:45.9: 12.32 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.32 +/- 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 1028144153379013760,2461199.6803,11.25,0.05,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 1028144153379013760 20260608.1803 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 06 08.1803 2461199.6803 11.74 07:36:46.57 +55:38:36.3
161.89769 28.36885 galactic Lyn Second-epoch detections are separated by 1.7" and 4.9 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 | 07:36:46.57 +55:38:36.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.445+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:46.57 +55:38:36.3: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:46.57 +55:38:36.3: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 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,2461199.6803,11.74,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.31 07:42:24.01 +53:56:43.2
163.93437 28.95757 galactic Lyn Second-epoch detections are separated by 1.0" and 5.0 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 985317591362702720 | 07:42:23.96 +53:56:43.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.264+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:24.01 +53:56:43.2: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:24.01 +53:56:43.2: 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 985317591362702720,2461199.6803,11.31,0.05,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 985317591362702720 20260608.1803 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 06 08.1803 2461199.6803 10.72 08:22:29.37 +56:15:05.1
161.52003 34.78147 galactic Lyn Second-epoch detections are separated by 0.1" and 4.7 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 1033986575916312832 | 08:22:29.35 +56:15:04.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.248+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:29.37 +56:15:05.1: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:29.37 +56:15:05.1: 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 1033986575916312832,2461199.6803,10.72,0.05,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 1033986575916312832 20260608.1803 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 06 08.1803 2461199.6803 10.62 08:19:32.42 +55:15:19.1
162.74400 34.39540 galactic Lyn Second-epoch detections are separated by 0.9" and 4.9 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 1032408196910391168 | 08:19:32.47 +55:15:19.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5) J-Ks=0.298+/-0.026 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:32.42 +55:15:19.1: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:32.42 +55:15:19.1: 11.68 +/- 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 1032408196910391168,2461199.6803,10.62,0.05,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 1032408196910391168 20260608.1803 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 06 08.1803 2461199.6803 10.70 08:18:10.08 +54:27:07.2
163.71880 34.20609 galactic Lyn Second-epoch detections are separated by 0.2" and 4.8 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 | Gaia DR3 1032278690760764288 | 08:18:10.12 +54:27:07.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.661+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:18:10.08 +54:27:07.2: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:18:10.08 +54:27:07.2: 11.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 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 1032278690760764288,2461199.6803,10.70,0.05,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 1032278690760764288 20260608.1803 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 06 08.1803 2461199.6803 11.48 07:44:18.47 +54:30:05.6
163.34033 29.30087 galactic Lyn Second-epoch detections are separated by 1.7" and 5.0 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 | 07:44:18.47 +54:30:05.6 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:18.47 +54:30:05.6: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:18.47 +54:30:05.6: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 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,2461199.6803,11.48,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.33 08:23:19.57 +55:02:07.5
162.99618 34.94120 galactic Lyn Second-epoch detections are separated by 1.1" and 4.6 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 J125.8373+55.0276 | 08:23:19.62 +55:02:08.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5) J-Ks=0.538+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:19.57 +55:02:07.5: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:19.57 +55:02:07.5: 12.67 +/- 0.01 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
ATO J125.8373+55.0276,2461199.6803,11.33,0.05,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
ATO J125.8373+55.0276 20260608.1803 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 06 08.1803 2461199.6803 11.59 07:53:35.42 +52:02:03.4
166.34406 30.40805 galactic Lyn Second-epoch detections are separated by 3.3" and 4.7 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 | ATO J118.3975+52.0347 | 07:53:35.41 +52:02:05.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.719+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:53:35.42 +52:02:03.4: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:53:35.42 +52:02:03.4: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 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
ATO J118.3975+52.0347,2461199.6803,11.59,0.05,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
ATO J118.3975+52.0347 20260608.1803 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 06 08.1803 2461199.6803 10.63 08:21:57.74 +55:47:38.9
162.07948 34.72454 galactic Lyn Second-epoch detections are separated by 0.8" and 4.9 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 1033947203951614592 | 08:21:57.74 +55:47:39.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.366+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:57.74 +55:47:38.9: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:57.74 +55:47:38.9: 11.58 +/- 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 1033947203951614592,2461199.6803,10.63,0.05,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 1033947203951614592 20260608.1803 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 06 08.1803 2461199.6803 11.46 07:44:13.32 +54:39:52.6
163.15293 29.30694 galactic Lyn Second-epoch detections are separated by 0.9" and 5.0 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 | 07:44:13.32 +54:39:52.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.420+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:13.32 +54:39:52.6: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:13.32 +54:39:52.6: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 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,2461199.6803,11.46,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.68 08:23:36.29 +55:44:19.2
162.13707 34.95736 galactic Lyn Second-epoch detections are separated by 0.4" and 4.7 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 | ATO J125.9153+55.7390 | 08:23:36.27 +55:44:19.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G9 (LAMOST DR5) J-Ks=0.652+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:36.29 +55:44:19.2: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:36.29 +55:44:19.2: 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
ATO J125.9153+55.7390,2461199.6803,10.68,0.05,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
ATO J125.9153+55.7390 20260608.1803 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 06 08.1803 2461199.6803 10.63 07:37:12.32 +55:23:32.6
162.18953 28.39676 galactic Lyn Second-epoch detections are separated by 0.7" and 5.1 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 985653663963012608 | 07:37:12.28 +55:23:33.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 (LAMOST DR5)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:12.32 +55:23:32.6: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:12.32 +55:23:32.6: 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 985653663963012608,2461199.6803,10.63,0.05,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 985653663963012608 20260608.1803 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 06 08.1803 2461199.6803 10.65 08:23:24.65 +54:58:57.1
163.06026 34.95483 galactic Lyn Second-epoch detections are separated by 0.5" and 4.8 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 | Gaia DR3 1032350953586293120 | 08:23:24.63 +54:58:57.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5) J-Ks=0.001+/-0.031 (A)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:24.65 +54:58:57.1: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:24.65 +54:58:57.1: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 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 1032350953586293120,2461199.6803,10.65,0.05,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 1032350953586293120 20260608.1803 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 06 08.1803 2461199.6803 10.64 08:20:39.80 +54:09:46.5
164.06661 34.57168 galactic Lyn Second-epoch detections are separated by 1.3" and 4.8 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 | ATO J125.1671+54.1744 | 08:20:39.82 +54:09:47.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.826+/-0.029 (M)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:39.80 +54:09:46.5: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:39.80 +54:09:46.5: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 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
ATO J125.1671+54.1744,2461199.6803,10.64,0.05,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
ATO J125.1671+54.1744 20260608.1803 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 06 08.1803 2461199.6803 11.22 08:21:26.25 +55:09:16.6
162.85955 34.66804 galactic Lyn Second-epoch detections are separated by 0.6" and 4.7 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 1032415373800184320 | 08:21:26.28 +55:09:17.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.939+/-0.028 (M)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:26.25 +55:09:16.6: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:26.25 +55:09:16.6: 12.62 +/- 0.01 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 1032415373800184320,2461199.6803,11.22,0.05,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 1032415373800184320 20260608.1803 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 06 08.1803 2461199.6803 11.38 07:36:03.84 +55:31:10.8
162.02219 28.25297 galactic Lyn Second-epoch detections are separated by 0.5" and 5.2 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 | 07:36:03.84 +55:31:10.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.707+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:03.84 +55:31:10.8: 15.13 +/- 0.19 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:03.84 +55:31:10.8: 12.82 +/- 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,2461199.6803,11.38,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.24 07:50:26.70 +53:06:24.0
165.05084 30.04770 galactic Lyn Second-epoch detections are separated by 0.8" and 5.2 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 984301397803554816 | 07:50:26.74 +53:06:23.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.869+/-0.033 (M)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:50:26.70 +53:06:24.0: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:50:26.70 +53:06:24.0: 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 984301397803554816,2461199.6803,11.24,0.05,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
Gaia DR3 984301397803554816 20260608.1803 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 06 08.1803 2461199.6803 11.31 07:39:04.20 +56:15:54.4
161.23950 28.76307 galactic Lyn Second-epoch detections are separated by 2.6" and 4.9 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 | ATO J114.7673+56.2653 | 07:39:04.16 +56:15:55.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.605+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:04.20 +56:15:54.4: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:04.20 +56:15:54.4: 12.36 +/- 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
ATO J114.7673+56.2653,2461199.6803,11.31,0.05,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
ATO J114.7673+56.2653 20260608.1803 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 06 08.1803 2461199.6803 11.70 07:41:29.74 +55:14:29.8
162.44544 28.98400 galactic Lyn Second-epoch detections are separated by 0.2" and 5.2 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 | 07:41:29.74 +55:14:29.8 (user input) | T | P | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=0.746+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:29.74 +55:14:29.8: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:29.74 +55:14:29.8: 13.06 +/- 0.02 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,2461199.6803,11.70,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.77 07:33:43.17 +57:39:46.0
159.56301 28.20298 galactic Lyn Second-epoch detections are separated by 0.2" and 5.1 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 | 07:33:43.17 +57:39:46.0 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:33:43.17 +57:39:46.0: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:33:43.17 +57:39:46.0: 12.90 +/- 0.02 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,2461199.6803,11.77,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.98 08:20:21.71 +55:04:59.9
162.95001 34.51576 galactic Lyn Second-epoch detections are separated by 1.0" and 4.7 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 1032393486646846208 | 08:20:21.63 +55:04:59.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 (LAMOST DR5) J-Ks=0.301+/-0.027 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:21.71 +55:04:59.9: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:21.71 +55:04:59.9: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 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 1032393486646846208,2461199.6803,10.98,0.05,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 1032393486646846208 20260608.1803 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 06 08.1803 2461199.6803 11.18 07:42:38.37 +54:49:25.3
162.94199 29.09825 galactic Lyn Second-epoch detections are separated by 0.9" and 5.1 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 985751000806241664 | 07:42:38.38 +54:49:25.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.365+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:38.37 +54:49:25.3: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:38.37 +54:49:25.3: 12.31 +/- 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 985751000806241664,2461199.6803,11.18,0.05,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 985751000806241664 20260608.1803 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 06 08.1803 2461199.6803 11.66 07:36:08.84 +54:55:50.8
162.68625 28.18555 galactic Lyn Second-epoch detections are separated by 4.1" and 5.7 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 | 07:36:08.84 +54:55:50.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.367+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:08.84 +54:55:50.8: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:08.84 +54:55:50.8: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461199.6803,11.66,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.73 08:21:03.10 +56:00:39.6
161.82100 34.58996 galactic Lyn Second-epoch detections are separated by 0.9" and 4.7 pix
The object was found in VSX 0" Gaia DR3 1034704561305317504
Type: RS
# Max. Min./Amp. JD0 Period
13.080 G 13.190 G G
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:03.10 +56:00:39.6: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:03.10 +56:00:39.6: 13.37 +/- 0.03 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
Gaia DR3 1034704561305317504,2461199.6803,11.73,0.05,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
Gaia DR3 1034704561305317504 20260608.1803 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 06 08.1803 2461199.6803 11.62 08:21:35.81 +54:46:36.6
163.31827 34.69887 galactic Lyn Second-epoch detections are separated by 0.8" and 4.7 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 | 08:21:35.81 +54:46:36.6 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.618+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:35.81 +54:46:36.6: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:35.81 +54:46:36.6: 13.26 +/- 0.02 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,2461199.6803,11.62,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.98 08:22:08.53 +54:17:21.7
163.90977 34.78631 galactic Lyn Second-epoch detections are separated by 0.8" and 4.8 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 | 08:22:08.53 +54:17:21.7 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.621+/-0.029 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:08.53 +54:17:21.7: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:08.53 +54:17:21.7: 12.19 +/- 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
target,2461199.6803,10.98,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.55 07:39:17.70 +55:23:16.0
162.23720 28.69056 galactic Lyn Second-epoch detections are separated by 2.6" and 4.8 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 | 07:39:17.70 +55:23:16.0 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.095+/-0.036 (A)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:17.70 +55:23:16.0: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:17.70 +55:23:16.0: 12.84 +/- 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,2461199.6803,11.55,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.51 07:48:08.25 +53:48:43.9
164.19908 29.78183 galactic Lyn Second-epoch detections are separated by 1.1" and 5.2 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 | 07:48:08.25 +53:48:43.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.388+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:48:08.25 +53:48:43.9: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:48:08.25 +53:48:43.9: 12.73 +/- 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
target,2461199.6803,11.51,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.12 07:39:21.84 +55:50:02.9
161.73322 28.75377 galactic Lyn Second-epoch detections are separated by 1.3" and 4.9 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 986062029453764608 | 07:39:24.59 +55:49:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.645+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:21.84 +55:50:02.9: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:21.84 +55:50:02.9: 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 986062029453764608,2461199.6803,11.12,0.05,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 986062029453764608 20260608.1803 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 06 08.1803 2461199.6803 11.21 07:41:03.34 +54:33:56.2
163.20344 28.84007 galactic Lyn Second-epoch detections are separated by 0.3" and 5.2 pix
The object was found in VSX 1" Gaia DR3 985412458600197632
Type: VAR
# Max. Min./Amp. JD0 Period
12.120 G 12.130 G 0.027932000000 G
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:03.34 +54:33:56.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:03.34 +54:33:56.2: 12.23 +/- 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 985412458600197632,2461199.6803,11.21,0.05,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 985412458600197632 20260608.1803 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 06 08.1803 2461199.6803 11.16 08:17:42.27 +54:23:25.7
163.79331 34.13878 galactic Lyn Second-epoch detections are separated by 1.4" and 5.0 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 1032254815038298240 | 08:17:42.31 +54:23:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.315+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:17:42.27 +54:23:25.7: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:17:42.27 +54:23:25.7: 12.15 +/- 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 1032254815038298240,2461199.6803,11.16,0.05,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 1032254815038298240 20260608.1803 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 06 08.1803 2461199.6803 11.18 07:43:27.24 +55:12:08.2
162.52627 29.25703 galactic Lyn Second-epoch detections are separated by 1.8" and 4.8 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 | Gaia DR3 985831578688565248 | 07:43:27.11 +55:12:03.5 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:27.24 +55:12:08.2: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:27.24 +55:12:08.2: 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 985831578688565248,2461199.6803,11.18,0.05,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 985831578688565248 20260608.1803 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 06 08.1803 2461199.6803 11.77 07:40:04.45 +54:40:36.9
163.05717 28.71305 galactic Lyn Second-epoch detections are separated by 0.9" and 5.3 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 | 07:40:04.45 +54:40:36.9 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.580+/-0.035 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:04.45 +54:40:36.9: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:04.45 +54:40:36.9: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.51 +/- 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,2461199.6803,11.77,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.81 07:35:50.66 +55:51:21.7
161.63899 28.26625 galactic Lyn Second-epoch detections are separated by 3.6" and 4.6 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 | 07:35:50.66 +55:51:21.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.614+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:50.66 +55:51:21.7: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:50.66 +55:51:21.7: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 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,2461199.6803,11.81,0.05,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
target 20260608.1803 11.81CV 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 06 08.1803 2461199.6803 11.53 08:24:24.22 +55:21:18.2
162.60004 35.08453 galactic Lyn Second-epoch detections are separated by 0.2" and 4.7 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 | 08:24:24.22 +55:21:18.2 (user input) | T | P | (position from user input) J-Ks=0.298+/-0.031 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:24.22 +55:21:18.2: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:24.22 +55:21:18.2: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.64 +/- 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
target,2461199.6803,11.53,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.70 07:35:13.81 +55:53:47.1
161.58079 28.18612 galactic Lyn Second-epoch detections are separated by 0.5" and 5.1 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 986098725653935744 | 07:35:13.81 +55:53:46.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.607+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:13.81 +55:53:47.1: 13.19 +/- 0.03 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:13.81 +55:53:47.1: 11.69 +/- 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 986098725653935744,2461199.6803,10.70,0.05,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 986098725653935744 20260608.1803 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 06 08.1803 2461199.6803 10.61 08:22:01.99 +56:08:09.4
161.66345 34.72251 galactic Lyn Second-epoch detections are separated by 0.8" and 4.8 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 | Gaia DR3 1033960879127437568 | 08:22:01.97 +56:08:09.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.467+/-0.027 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:01.99 +56:08:09.4: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:01.99 +56:08:09.4: 11.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.51 +/- 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 1033960879127437568,2461199.6803,10.61,0.05,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 1033960879127437568 20260608.1803 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 06 08.1803 2461199.6803 11.78 07:43:27.66 +54:04:31.3
163.80869 29.12822 galactic Lyn Second-epoch detections are separated by 2.8" and 4.9 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 | 07:43:27.66 +54:04:31.3 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:27.66 +54:04:31.3: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:27.66 +54:04:31.3: 13.18 +/- 0.03 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,2461199.6803,11.78,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.67 08:23:39.92 +54:46:40.2
163.30876 34.99702 galactic Lyn Second-epoch detections are separated by 0.8" and 4.7 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 | ATO J125.9187+54.7805 | 08:23:39.89 +54:46:40.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.601+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:39.92 +54:46:40.2: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:39.92 +54:46:40.2: 11.53 +/- 0.00 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
ATO J125.9187+54.7805,2461199.6803,10.67,0.05,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
ATO J125.9187+54.7805 20260608.1803 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 06 08.1803 2461199.6803 11.72 07:37:36.07 +56:03:44.1
161.44151 28.53607 galactic Lyn Second-epoch detections are separated by 0.7" and 5.1 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 | 07:37:36.07 +56:03:44.1 (user input) | T | P | (position from user input) J-Ks=0.604+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:36.07 +56:03:44.1: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:36.07 +56:03:44.1: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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,2461199.6803,11.72,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.68 07:43:24.84 +53:44:53.4
164.17940 29.08136 galactic Lyn Second-epoch detections are separated by 3.0" and 4.7 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 984561333520648576 | 07:43:25.37 +53:45:36.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.645+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:24.84 +53:44:53.4: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:24.84 +53:44:53.4: 13.02 +/- 0.02 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
Gaia DR3 984561333520648576,2461199.6803,11.68,0.05,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
Gaia DR3 984561333520648576 20260608.1803 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 06 08.1803 2461199.6803 11.86 07:34:16.59 +57:19:06.4
159.96119 28.23566 galactic Lyn Second-epoch detections are separated by 0.3" and 5.2 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 | 07:34:16.59 +57:19:06.4 (user input) | T | P | (position from user input) J-Ks=0.645+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:34:16.59 +57:19:06.4: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:34:16.59 +57:19:06.4: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 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,2461199.6803,11.86,0.05,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
target 20260608.1803 11.86CV 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 06 08.1803 2461199.6803 11.62 07:38:20.12 +54:33:14.5
163.15875 28.44751 galactic Lyn Second-epoch detections are separated by 3.9" and 5.6 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 | ASASSN-V J073818.59+543243.7 | 07:38:18.61 +54:32:43.3 (Gaia DR3) | ROT (local) | 1.202950000000 (local) | Gaia3var=NOT_AVAILABLE SpType: G9 (LAMOST DR5) J-Ks=0.423+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:20.12 +54:33:14.5: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:20.12 +54:33:14.5: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.11 +/- 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
ASASSN-V J073818.59+543243.7,2461199.6803,11.62,0.05,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
ASASSN-V J073818.59+543243.7 20260608.1803 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 06 08.1803 2461199.6803 11.78 07:55:01.80 +51:57:11.9
166.46464 30.61990 galactic Lyn Second-epoch detections are separated by 1.9" and 4.8 pix
The object was found in VSX 1" Gaia DR3 936123035953070976
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_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:55:01.80 +51:57:11.9: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:55:01.80 +51:57:11.9: 13.01 +/- 0.02 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
Gaia DR3 936123035953070976,2461199.6803,11.78,0.05,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
Gaia DR3 936123035953070976 20260608.1803 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 06 08.1803 2461199.6803 11.69 07:35:35.48 +56:49:28.6
160.54252 28.35304 galactic Lyn Second-epoch detections are separated by 2.4" and 4.7 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 | 07:35:35.48 +56:49:28.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.420+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:35.48 +56:49:28.6: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:35.48 +56:49:28.6: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 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,2461199.6803,11.69,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.81 07:48:18.46 +53:53:11.7
164.11694 29.81474 galactic Lyn Second-epoch detections are separated by 2.1" and 5.0 pix
The object was found in VSX 2" ASASSN-V J074818.39+535313.3
Type: ROT
# Max. Min./Amp. JD0 Period
14.040 g Y 0.120 g 2458578.66200 16.439000000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:48:18.46 +53:53:11.7: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:48:18.46 +53:53:11.7: 12.96 +/- 0.02 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
ASASSN-V J074818.39+535313.3,2461199.6803,11.81,0.05,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
ASASSN-V J074818.39+535313.3 20260608.1803 11.81CV 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 06 08.1803 2461199.6803 10.64 07:34:41.23 +56:39:58.6
160.70352 28.21044 galactic Lyn Second-epoch detections are separated by 0.4" and 5.3 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 989152511824785920 | 07:34:41.25 +56:39:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.647+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:34:41.23 +56:39:58.6: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:34:41.23 +56:39:58.6: 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 989152511824785920,2461199.6803,10.64,0.05,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 989152511824785920 20260608.1803 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 06 08.1803 2461199.6803 11.72 07:47:51.84 +53:06:16.7
165.00352 29.66250 galactic Lyn Second-epoch detections are separated by 2.1" and 4.8 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 | 07:47:51.84 +53:06:16.7 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.035 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:47:51.84 +53:06:16.7: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:47:51.84 +53:06:16.7: 13.00 +/- 0.02 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,2461199.6803,11.72,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.52 08:22:29.44 +54:29:24.4
163.66425 34.83362 galactic Lyn Second-epoch detections are separated by 1.0" and 4.7 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 | 08:22:29.44 +54:29:24.4 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.332+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:29.44 +54:29:24.4: 16.31 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:29.44 +54:29:24.4: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 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,2461199.6803,11.52,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.24 08:21:04.81 +54:37:13.0
163.51014 34.62693 galactic Lyn Second-epoch detections are separated by 1.1" and 4.8 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 | 08:21:04.81 +54:37:13.0 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.333+/-0.026 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:04.81 +54:37:13.0: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:04.81 +54:37:13.0: 12.59 +/- 0.01 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
target,2461199.6803,11.24,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.43 08:30:07.81 +51:31:28.6
167.28347 36.02428 galactic Lyn Second-epoch detections are separated by 1.5" and 4.6 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 1028156694683516928 | 08:30:07.84 +51:31:29.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.528+/-0.027 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:30:07.81 +51:31:28.6: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:30:07.81 +51:31:28.6: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 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 1028156694683516928,2461199.6803,11.43,0.05,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
Gaia DR3 1028156694683516928 20260608.1803 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 06 08.1803 2461199.6803 11.88 07:39:26.57 +54:51:37.2
162.83666 28.64591 galactic Lyn Second-epoch detections are separated by 1.3" and 5.1 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 | 07:39:26.57 +54:51:37.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.374+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:26.57 +54:51:37.2: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:26.57 +54:51:37.2: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 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,2461199.6803,11.88,0.05,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
target 20260608.1803 11.88CV 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 06 08.1803 2461199.6803 11.70 08:18:35.58 +54:19:26.4
163.87341 34.26833 galactic Lyn Second-epoch detections are separated by 1.1" and 5.0 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 | 08:18:35.58 +54:19:26.4 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.498+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:18:35.58 +54:19:26.4: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:18:35.58 +54:19:26.4: 13.25 +/- 0.02 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,2461199.6803,11.70,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.59 07:52:57.47 +52:27:42.3
165.83942 30.35718 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 | 07:52:57.47 +52:27:42.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.419+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:52:57.47 +52:27:42.3: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:52:57.47 +52:27:42.3: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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,2461199.6803,11.59,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.37 07:39:14.89 +55:16:20.8
162.36673 28.66978 galactic Lyn Second-epoch detections are separated by 0.6" and 5.2 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 | 07:39:14.89 +55:16:20.8 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=0.710+/-0.034 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:14.89 +55:16:20.8: 14.70 +/- 0.12 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:14.89 +55:16:20.8: 12.82 +/- 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,2461199.6803,11.37,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.60 07:37:46.20 +56:11:21.2
161.30125 28.57475 galactic Lyn Second-epoch detections are separated by 2.0" and 5.1 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 | 07:37:46.20 +56:11:21.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.752+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:46.20 +56:11:21.2: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:46.20 +56:11:21.2: 12.90 +/- 0.02 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,2461199.6803,11.60,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.51 07:50:20.44 +53:11:57.7
164.94244 30.04203 galactic Lyn Second-epoch detections are separated by 1.4" and 4.9 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 | 07:50:20.44 +53:11:57.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.387+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:50:20.44 +53:11:57.7: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:50:20.44 +53:11:57.7: 12.67 +/- 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
target,2461199.6803,11.51,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.57 08:27:13.12 +52:34:44.1
165.98949 35.56567 galactic Lyn Second-epoch detections are separated by 0.7" and 4.9 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 1028822208456419840 | 08:27:13.04 +52:34:44.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.572+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:27:13.12 +52:34:44.1: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:27:13.12 +52:34:44.1: 12.66 +/- 0.01 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 1028822208456419840,2461199.6803,11.57,0.05,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
Gaia DR3 1028822208456419840 20260608.1803 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 06 08.1803 2461199.6803 11.68 08:22:10.59 +55:34:38.0
162.34216 34.76160 galactic Lyn Second-epoch detections are separated by 2.1" and 4.4 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 | 08:22:10.59 +55:34:38.0 (user input) | T | P | (position from user input) J-Ks=0.355+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:10.59 +55:34:38.0: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:10.59 +55:34:38.0: 13.28 +/- 0.03 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,2461199.6803,11.68,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.37 08:22:52.05 +54:50:30.2
163.23442 34.88048 galactic Lyn Second-epoch detections are separated by 1.2" and 5.0 pix
The object was found in VSX17" Gaia DR3 1032326592531838464
Type: ROT
# Max. Min./Amp. JD0 Period
14.090 G 14.110 G G
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:52.05 +54:50:30.2: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:52.05 +54:50:30.2: 12.67 +/- 0.01 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 1032326592531838464,2461199.6803,11.37,0.05,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
Gaia DR3 1032326592531838464 20260608.1803 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 06 08.1803 2461199.6803 11.46 08:24:07.27 +55:38:10.7
162.25852 35.03400 galactic Lyn Second-epoch detections are separated by 1.7" and 4.6 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 1033883638435664640 | 08:24:07.27 +55:38:11.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.446+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:07.27 +55:38:10.7: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:07.27 +55:38:10.7: 12.61 +/- 0.01 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 1033883638435664640,2461199.6803,11.46,0.05,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 1033883638435664640 20260608.1803 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 06 08.1803 2461199.6803 11.64 08:30:03.09 +52:51:45.9
165.62978 35.98923 galactic Lyn Second-epoch detections are separated by 2.1" and 5.1 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 1028842716924528640 | 08:30:03.07 +52:51:46.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.373+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:30:03.09 +52:51:45.9: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:30:03.09 +52:51:45.9: 12.67 +/- 0.01 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 1028842716924528640,2461199.6803,11.64,0.05,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
Gaia DR3 1028842716924528640 20260608.1803 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 06 08.1803 2461199.6803 11.53 08:29:06.02 +50:27:08.2
168.60806 35.86254 galactic Lyn Second-epoch detections are separated by 0.8" and 5.0 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 | 08:29:06.02 +50:27:08.2 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.433+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:29:06.02 +50:27:08.2: 14.67 +/- 0.09 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:29:06.02 +50:27:08.2: 12.75 +/- 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
target,2461199.6803,11.53,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.25 08:19:46.18 +54:30:16.5
163.65341 34.43841 galactic Lyn Second-epoch detections are separated by 0.9" and 4.8 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 | Gaia DR3 1032235848462695552 | 08:19:46.21 +54:30:16.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.665+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:46.18 +54:30:16.5: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:46.18 +54:30:16.5: 12.61 +/- 0.01 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 1032235848462695552,2461199.6803,11.25,0.05,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 1032235848462695552 20260608.1803 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 06 08.1803 2461199.6803 11.68 08:19:50.90 +55:16:23.2
162.72145 34.43895 galactic Lyn Second-epoch detections are separated by 1.4" and 4.7 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 | 08:19:50.90 +55:16:23.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.442+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:50.90 +55:16:23.2: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:50.90 +55:16:23.2: 13.28 +/- 0.02 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,2461199.6803,11.68,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.83 07:39:03.82 +54:35:34.8
163.13061 28.55727 galactic Lyn Second-epoch detections are separated by 1.6" and 5.5 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 | 07:39:03.82 +54:35:34.8 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.494+/-0.034 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:03.82 +54:35:34.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:03.82 +54:35:34.8: 13.41 +/- 0.03 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,2461199.6803,11.83,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.89 08:23:40.68 +54:32:47.6
163.59095 35.00467 galactic Lyn Second-epoch detections are separated by 2.0" and 4.9 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 | 08:23:40.68 +54:32:47.6 (user input) | T | P | (position from user input) SpType: K3 (LAMOST DR5)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:40.68 +54:32:47.6: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:40.68 +54:32:47.6: 13.27 +/- 0.02 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,2461199.6803,11.89,0.05,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
target 20260608.1803 11.89CV 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 06 08.1803 2461199.6803 11.87 07:34:49.31 +56:46:00.1
160.59308 28.24136 galactic Lyn Second-epoch detections are separated by 1.5" and 5.2 pix
The object was found in VSX 1" Gaia DR3 989155436698584704
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.980 G 13.020 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:34:49.31 +56:46:00.1: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:34:49.31 +56:46:00.1: 13.18 +/- 0.03 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
Gaia DR3 989155436698584704,2461199.6803,11.87,0.05,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 989155436698584704 20260608.1803 11.87CV 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 06 08.1803 2461199.6803 11.12 07:38:27.23 +55:55:44.3
161.60858 28.63831 galactic Lyn Second-epoch detections are separated by 1.4" and 5.3 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 986067320853476224 | 07:38:27.31 +55:55:44.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.366+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:27.23 +55:55:44.3: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:27.23 +55:55:44.3: 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 986067320853476224,2461199.6803,11.12,0.05,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 986067320853476224 20260608.1803 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 06 08.1803 2461199.6803 11.73 08:21:28.35 +55:55:30.5
161.92298 34.65157 galactic Lyn Second-epoch detections are separated by 1.0" and 4.6 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 | 08:21:28.35 +55:55:30.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.359+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:28.35 +55:55:30.5: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:28.35 +55:55:30.5: 13.30 +/- 0.02 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,2461199.6803,11.73,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.46 07:41:40.62 +54:43:25.3
163.03677 28.94860 galactic Lyn Second-epoch detections are separated by 0.4" and 5.3 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 | ATO J115.4065+54.7336 | 07:41:40.62 +54:43:25.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.654+/-0.035 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:40.62 +54:43:25.3: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:40.62 +54:43:25.3: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 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
ATO J115.4065+54.7336,2461199.6803,11.46,0.05,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
ATO J115.4065+54.7336 20260608.1803 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 06 08.1803 2461199.6803 11.88 08:23:01.42 +53:58:13.5
164.29606 34.92014 galactic Lyn Second-epoch detections are separated by 2.6" and 4.4 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 | 08:23:01.42 +53:58:13.5 (user input) | T | P | (position from user input) J-Ks=0.705+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:01.42 +53:58:13.5: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:01.42 +53:58:13.5: 13.38 +/- 0.03 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,2461199.6803,11.88,0.05,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
target 20260608.1803 11.88CV 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 06 08.1803 2461199.6803 11.56 07:43:55.30 +55:02:42.7
162.71369 29.30624 galactic Lyn Second-epoch detections are separated by 2.3" and 5.4 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 | ATO J115.9814+55.0421 | 07:43:55.30 +55:02:42.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.430+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:55.30 +55:02:42.7: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:55.30 +55:02:42.7: 12.75 +/- 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
ATO J115.9814+55.0421,2461199.6803,11.56,0.05,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
ATO J115.9814+55.0421 20260608.1803 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 06 08.1803 2461199.6803 11.54 08:25:10.76 +53:58:41.6
164.27944 35.23690 galactic Lyn Second-epoch detections are separated by 0.9" and 4.6 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 1032051641609883648 | 08:25:10.81 +53:58:42.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.817+/-0.034 (M)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:10.76 +53:58:41.6: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:10.76 +53:58:41.6: 12.57 +/- 0.01 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 1032051641609883648,2461199.6803,11.54,0.05,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
Gaia DR3 1032051641609883648 20260608.1803 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 06 08.1803 2461199.6803 11.55 07:55:24.96 +51:59:57.6
166.41851 30.68375 galactic Lyn Second-epoch detections are separated by 1.5" and 4.9 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 | 07:55:24.96 +51:59:57.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.418+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:55:24.96 +51:59:57.6: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:55:24.96 +51:59:57.6: 12.67 +/- 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
target,2461199.6803,11.55,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.52 07:46:26.89 +53:12:40.4
164.85323 29.46422 galactic Lyn Second-epoch detections are separated by 2.5" and 4.8 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 | 07:46:26.89 +53:12:40.4 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.413+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:46:26.89 +53:12:40.4: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:46:26.89 +53:12:40.4: 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
target,2461199.6803,11.52,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.27 08:21:15.19 +54:33:43.7
163.58033 34.65288 galactic Lyn Second-epoch detections are separated by 1.7" and 4.6 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 1032327142287671168 | 08:21:15.15 +54:33:44.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.379+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:15.19 +54:33:43.7: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:15.19 +54:33:43.7: 12.54 +/- 0.01 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 1032327142287671168,2461199.6803,11.27,0.05,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 1032327142287671168 20260608.1803 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 06 08.1803 2461199.6803 11.51 08:22:36.28 +54:19:34.6
163.86348 34.85316 galactic Lyn Second-epoch detections are separated by 0.4" and 4.8 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 | 08:22:36.28 +54:19:34.6 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.700+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:36.28 +54:19:34.6: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:36.28 +54:19:34.6: 12.93 +/- 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
target,2461199.6803,11.51,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.63 07:39:26.44 +54:52:11.4
162.82588 28.64681 galactic Lyn Second-epoch detections are separated by 1.9" and 4.9 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 | 07:39:26.44 +54:52:11.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.635+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:26.44 +54:52:11.4: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:26.44 +54:52:11.4: 13.05 +/- 0.02 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,2461199.6803,11.63,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.60 08:20:44.12 +54:50:49.5
163.23561 34.57351 galactic Lyn Second-epoch detections are separated by 0.9" and 4.6 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 | 08:20:44.12 +54:50:49.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.303+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:44.12 +54:50:49.5: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:44.12 +54:50:49.5: 13.43 +/- 0.03 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,2461199.6803,11.60,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.85 07:38:11.55 +54:56:55.7
162.71051 28.47903 galactic Lyn Second-epoch detections are separated by 1.8" and 5.5 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 | 07:38:11.55 +54:56:55.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.385+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:11.55 +54:56:55.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:11.55 +54:56:55.7: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 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,2461199.6803,11.85,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.83 08:19:18.59 +54:26:52.2
163.72285 34.37208 galactic Lyn Second-epoch detections are separated by 0.8" and 4.7 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 | 08:19:18.59 +54:26:52.2 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.371+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:18.59 +54:26:52.2: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:18.59 +54:26:52.2: 13.38 +/- 0.03 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,2461199.6803,11.83,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.83 07:43:21.52 +54:02:15.9
163.84935 29.10877 galactic Lyn Second-epoch detections are separated by 3.0" and 4.8 pix
The object was found in VSX 0" Gaia DR3 985316251332889984
Type: VAR
# Max. Min./Amp. JD0 Period
12.960 G 13.090 G 0.124454600000 F
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:21.52 +54:02:15.9: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:21.52 +54:02:15.9: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 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 985316251332889984,2461199.6803,11.83,0.05,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
Gaia DR3 985316251332889984 20260608.1803 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 06 08.1803 2461199.6803 11.74 08:25:15.13 +54:20:44.1
163.82948 35.23853 galactic Lyn Second-epoch detections are separated by 1.7" and 4.8 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 | 08:25:15.13 +54:20:44.1 (user input) | T | P | (position from user input) J-Ks=0.448+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:15.13 +54:20:44.1: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:15.13 +54:20:44.1: 12.95 +/- 0.02 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,2461199.6803,11.74,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.46 08:22:50.92 +54:25:04.6
163.75098 34.88702 galactic Lyn Second-epoch detections are separated by 1.0" and 4.9 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 | 08:22:50.92 +54:25:04.6 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.331+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:50.92 +54:25:04.6: 15.31 +/- 0.16 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:50.92 +54:25:04.6: 12.94 +/- 0.02 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,2461199.6803,11.46,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.71 07:51:07.20 +52:19:45.7
165.95643 30.06409 galactic Lyn Second-epoch detections are separated by 1.3" and 5.4 pix
The object was found in VSX 1" ASASSN-V J075107.18+521945.4
Type: ROT
# Max. Min./Amp. JD0 Period
13.580 g Y 0.200 g 2459520.94300 0.996555000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:51:07.20 +52:19:45.7: 15.57 +/- 0.23 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:51:07.20 +52:19:45.7: 12.89 +/- 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
ASASSN-V J075107.18+521945.4,2461199.6803,11.71,0.05,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
ASASSN-V J075107.18+521945.4 20260608.1803 11.71CV 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 06 08.1803 2461199.6803 11.78 08:22:40.52 +56:06:17.7
161.69704 34.81312 galactic Lyn Second-epoch detections are separated by 1.6" and 4.5 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 | 08:22:40.52 +56:06:17.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.367+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:40.52 +56:06:17.7: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:40.52 +56:06:17.7: 13.38 +/- 0.03 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,2461199.6803,11.78,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.38 07:37:30.68 +56:12:49.8
161.26851 28.54200 galactic Lyn Second-epoch detections are separated by 2.7" and 4.7 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 | 07:37:30.68 +56:12:49.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.427+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:30.68 +56:12:49.8: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:30.68 +56:12:49.8: 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
target,2461199.6803,11.38,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.73 08:24:57.97 +55:14:32.0
162.73432 35.16866 galactic Lyn Second-epoch detections are separated by 0.2" and 4.8 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 1033862094879245696 | 08:24:57.97 +55:14:32.0 (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) SpType: F9 (LAMOST DR5) J-Ks=0.401+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:57.97 +55:14:32.0: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:57.97 +55:14:32.0: 12.94 +/- 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
Large-amplitude variable Gaia DR2 1033862094879245696,2461199.6803,11.73,0.05,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
Large-amplitude variable Gaia DR2 1033862094879245696 20260608.1803 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 06 08.1803 2461199.6803 11.45 08:22:34.71 +54:35:25.5
163.54176 34.84439 galactic Lyn Second-epoch detections are separated by 1.3" and 4.7 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 | 08:22:34.71 +54:35:25.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.370+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:34.71 +54:35:25.5: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:34.71 +54:35:25.5: 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,2461199.6803,11.45,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.61 07:45:33.34 +54:01:06.8
163.91474 29.42689 galactic Lyn Second-epoch detections are separated by 3.4" and 4.9 pix
The object was found in VSX 1" Gaia DR3 984591054694260096
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.940 G 12.980 G A
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:45:33.34 +54:01:06.8: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:45:33.34 +54:01:06.8: 13.00 +/- 0.02 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
Gaia DR3 984591054694260096,2461199.6803,11.61,0.05,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
Gaia DR3 984591054694260096 20260608.1803 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 06 08.1803 2461199.6803 11.39 08:23:32.26 +55:55:42.3
161.90620 34.94052 galactic Lyn Second-epoch detections are separated by 1.2" and 4.8 pix
The object was found in VSX 0" Gaia DR3 1033944455172533376
Type: ROT
# Max. Min./Amp. JD0 Period
12.400 G 12.430 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:32.26 +55:55:42.3: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:32.26 +55:55:42.3: 12.60 +/- 0.01 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 1033944455172533376,2461199.6803,11.39,0.05,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
Gaia DR3 1033944455172533376 20260608.1803 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 06 08.1803 2461199.6803 11.39 07:42:09.60 +54:13:47.9
163.60658 28.95804 galactic Lyn Second-epoch detections are separated by 2.7" and 4.7 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 985357135124631936 | 07:42:09.56 +54:13:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.555+/-0.029 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:09.60 +54:13:47.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:09.60 +54:13:47.9: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 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 985357135124631936,2461199.6803,11.39,0.05,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
Gaia DR3 985357135124631936 20260608.1803 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 06 08.1803 2461199.6803 11.59 07:44:38.90 +53:34:46.4
164.39670 29.24214 galactic Lyn Second-epoch detections are separated by 1.3" and 5.1 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 984555492365118208 | 07:44:38.90 +53:34:46.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.767+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:38.90 +53:34:46.4: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:38.90 +53:34:46.4: 12.66 +/- 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 984555492365118208,2461199.6803,11.59,0.05,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
Gaia DR3 984555492365118208 20260608.1803 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 06 08.1803 2461199.6803 11.29 08:20:22.08 +54:27:04.1
163.71719 34.52585 galactic Lyn Second-epoch detections are separated by 0.2" and 4.8 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 | Gaia DR3 1032231656574665600 | 08:20:22.12 +54:27:04.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.570+/-0.025 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:22.08 +54:27:04.1: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:22.08 +54:27:04.1: 12.56 +/- 0.01 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 1032231656574665600,2461199.6803,11.29,0.05,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 1032231656574665600 20260608.1803 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 06 08.1803 2461199.6803 11.39 07:36:14.73 +56:02:36.2
161.43610 28.34593 galactic Lyn Second-epoch detections are separated by 0.8" and 5.2 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 | 07:36:14.73 +56:02:36.2 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.325+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:14.73 +56:02:36.2: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:14.73 +56:02:36.2: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 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,2461199.6803,11.39,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.32 08:22:49.24 +54:34:15.5
163.56457 34.87987 galactic Lyn Second-epoch detections are separated by 0.6" and 4.7 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 1032313467111788288 | 08:22:49.29 +54:34:15.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.242+/-0.029 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:49.24 +54:34:15.5: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:49.24 +54:34:15.5: 12.58 +/- 0.01 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 1032313467111788288,2461199.6803,11.32,0.05,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
Gaia DR3 1032313467111788288 20260608.1803 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 06 08.1803 2461199.6803 11.90 07:37:35.89 +54:14:28.7
163.49430 28.29873 galactic Lyn Second-epoch detections are separated by 2.7" and 5.2 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 | 07:37:35.89 +54:14:28.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.332+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:35.89 +54:14:28.7: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:35.89 +54:14:28.7: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 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,2461199.6803,11.90,0.05,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
target 20260608.1803 11.90CV 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 06 08.1803 2461199.6803 11.48 08:26:08.55 +52:18:31.3
166.32305 35.40398 galactic Lyn Second-epoch detections are separated by 0.9" and 4.8 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 | ATO J126.5270+52.3097 | 08:26:08.55 +52:18:31.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.656+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:26:08.55 +52:18:31.3: 13.38 +/- 0.03 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:26:08.55 +52:18:31.3: 12.61 +/- 0.01 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
ATO J126.5270+52.3097,2461199.6803,11.48,0.05,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
ATO J126.5270+52.3097 20260608.1803 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 06 08.1803 2461199.6803 11.81 08:18:53.48 +55:00:48.8
163.03845 34.30624 galactic Lyn Second-epoch detections are separated by 0.3" and 4.9 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 | 08:18:53.48 +55:00:48.8 (user input) | T | P | (position from user input) J-Ks=0.625+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:18:53.48 +55:00:48.8: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:18:53.48 +55:00:48.8: 13.47 +/- 0.03 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,2461199.6803,11.81,0.05,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
target 20260608.1803 11.81CV 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 06 08.1803 2461199.6803 10.52 07:36:10.39 +55:55:50.5
161.56163 28.32157 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 986092369102328448 | 07:36:10.39 +55:55:49.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.664+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:10.39 +55:55:50.5: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:10.39 +55:55:50.5: 11.54 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.54 +/- 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 986092369102328448,2461199.6803,10.52,0.05,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
Gaia DR3 986092369102328448 20260608.1803 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 06 08.1803 2461199.6803 11.63 07:50:12.59 +52:50:49.4
165.34445 29.98433 galactic Lyn Second-epoch detections are separated by 1.4" and 5.1 pix
The object was found in VSX 0" ASASSN-V J075012.56+525049.6
Type: ROT
# Max. Min./Amp. JD0 Period
13.480 g Y 0.080 g 2458619.65900 8.106600000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:50:12.59 +52:50:49.4: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:50:12.59 +52:50:49.4: 13.00 +/- 0.02 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
ASASSN-V J075012.56+525049.6,2461199.6803,11.63,0.05,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
ASASSN-V J075012.56+525049.6 20260608.1803 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 06 08.1803 2461199.6803 11.48 07:37:04.40 +54:52:40.1
162.76634 28.31023 galactic Lyn Second-epoch detections are separated by 1.0" and 5.3 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 | 07:37:04.40 +54:52:40.1 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.322+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:04.40 +54:52:40.1: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:04.40 +54:52:40.1: 13.01 +/- 0.02 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,2461199.6803,11.48,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.64 07:48:12.81 +53:28:36.0
164.58473 29.75644 galactic Lyn Second-epoch detections are separated by 1.6" and 4.9 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 | 07:48:12.81 +53:28:36.0 (user input) | T | P | (position from user input) J-Ks=0.269+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:48:12.81 +53:28:36.0: 12.37 +/- 0.01 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:48:12.81 +53:28:36.0: 13.01 +/- 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
target,2461199.6803,11.64,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.55 07:37:58.07 +55:54:11.3
161.62841 28.56760 galactic Lyn Second-epoch detections are separated by 0.2" and 5.1 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 | ATO J114.4920+55.9027 | 07:37:58.07 +55:54:11.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.414+/-0.043 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:58.07 +55:54:11.3: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:58.07 +55:54:11.3: 13.36 +/- 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
ATO J114.4920+55.9027,2461199.6803,11.55,0.05,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
ATO J114.4920+55.9027 20260608.1803 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 06 08.1803 2461199.6803 11.71 07:37:01.75 +54:44:06.1
162.92603 28.28463 galactic Lyn Second-epoch detections are separated by 2.8" and 5.3 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 | 07:37:01.75 +54:44:06.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.625+/-0.032 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:01.75 +54:44:06.1: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:01.75 +54:44:06.1: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 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,2461199.6803,11.71,0.05,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
target 20260608.1803 11.71CV 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 06 08.1803 2461199.6803 11.21 07:48:07.62 +52:54:29.8
165.23327 29.67904 galactic Lyn Second-epoch detections are separated by 1.2" and 5.3 pix
The object was found in ASASSN-V 2" ASASSN-V J074807.68+525428.2
Type: RRAB
MeanMag 12.28 m Amp. 0.15 m Period 0.6172462 d
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:48:07.62 +52:54:29.8: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:48:07.62 +52:54:29.8: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 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
VARIABLE_NAME,2461199.6803,11.21,0.05,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
VARIABLE_NAME 20260608.1803 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 06 08.1803 2461199.6803 11.72 08:23:38.69 +54:02:34.5
164.20583 35.01023 galactic Lyn Second-epoch detections are separated by 1.3" and 4.7 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 | 08:23:38.69 +54:02:34.5 (user input) | T | P | (position from user input) J-Ks=0.364+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:38.69 +54:02:34.5: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:38.69 +54:02:34.5: 12.86 +/- 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,2461199.6803,11.72,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.87 07:43:48.01 +54:47:39.5
162.99733 29.26101 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 | 07:43:48.01 +54:47:39.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.697+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:48.01 +54:47:39.5: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:48.01 +54:47:39.5: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 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,2461199.6803,11.87,0.05,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
target 20260608.1803 11.87CV 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 06 08.1803 2461199.6803 11.50 07:46:19.67 +53:56:13.3
164.02256 29.53045 galactic Lyn Second-epoch detections are separated by 1.5" and 5.4 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 | ATO J116.5767+53.9452 | 07:46:19.67 +53:56:13.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.731+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:46:19.67 +53:56:13.3: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:46:19.67 +53:56:13.3: 12.66 +/- 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
ATO J116.5767+53.9452,2461199.6803,11.50,0.05,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
ATO J116.5767+53.9452 20260608.1803 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 06 08.1803 2461199.6803 11.24 08:19:29.06 +54:23:31.3
163.79025 34.39784 galactic Lyn Second-epoch detections are separated by 0.9" and 4.8 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 | ATO J124.8710+54.3922 | 08:19:25.81 +54:23:57.2 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.455+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:29.06 +54:23:31.3: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:29.06 +54:23:31.3: 12.55 +/- 0.01 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
ATO J124.8710+54.3922,2461199.6803,11.24,0.05,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
ATO J124.8710+54.3922 20260608.1803 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 06 08.1803 2461199.6803 11.42 07:40:58.31 +54:23:59.2
163.38950 28.80728 galactic Lyn Second-epoch detections are separated by 1.9" and 5.5 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 | 07:40:58.31 +54:23:59.2 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.396+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:58.31 +54:23:59.2: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:58.31 +54:23:59.2: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 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,2461199.6803,11.42,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.31 08:19:02.89 +55:03:45.0
162.97884 34.32809 galactic Lyn Second-epoch detections are separated by 0.5" and 4.8 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 | Gaia DR3 1032399259082892544 | 08:19:02.83 +55:03:45.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.557+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:02.89 +55:03:45.0: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:02.89 +55:03:45.0: 11.22 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.22 +/- 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 1032399259082892544,2461199.6803,10.31,0.05,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 1032399259082892544 20260608.1803 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 06 08.1803 2461199.6803 11.39 08:22:47.07 +53:46:45.6
164.52959 34.88734 galactic Lyn Second-epoch detections are separated by 0.2" and 4.8 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 | Gaia DR3 1031998246576401152 | 08:22:47.12 +53:46:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.403+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:47.07 +53:46:45.6: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:47.07 +53:46:45.6: 12.57 +/- 0.01 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 1031998246576401152,2461199.6803,11.39,0.05,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
Gaia DR3 1031998246576401152 20260608.1803 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 06 08.1803 2461199.6803 11.29 07:38:01.34 +55:17:50.6
162.31363 28.49976 galactic Lyn Second-epoch detections are separated by 1.0" and 5.0 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 | 07:38:01.34 +55:17:50.6 (user input) | T | P | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=0.352+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:01.34 +55:17:50.6: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:01.34 +55:17:50.6: 12.67 +/- 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
target,2461199.6803,11.29,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.64 08:23:26.79 +53:48:34.0
164.49136 34.98471 galactic Lyn Second-epoch detections are separated by 1.9" and 5.1 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 | 08:23:26.79 +53:48:34.0 (user input) | T | P | (position from user input) J-Ks=0.342+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:26.79 +53:48:34.0: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:26.79 +53:48:34.0: 12.91 +/- 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,2461199.6803,11.64,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.69 07:41:25.85 +54:13:11.0
163.60302 28.85102 galactic Lyn Second-epoch detections are separated by 1.5" and 5.4 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 | 07:41:25.85 +54:13:11.0 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.225+/-0.032 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:25.85 +54:13:11.0: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:25.85 +54:13:11.0: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 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,2461199.6803,11.69,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.20 07:37:32.36 +54:09:45.7
163.58135 28.27928 galactic Lyn Second-epoch detections are separated by 1.5" and 5.4 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 985299689938839552 | 07:37:32.39 +54:09:46.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.668+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:32.36 +54:09:45.7: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:32.36 +54:09:45.7: 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 985299689938839552,2461199.6803,11.20,0.05,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 985299689938839552 20260608.1803 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 06 08.1803 2461199.6803 11.13 07:40:36.19 +55:18:33.5
162.35160 28.86571 galactic Lyn Second-epoch detections are separated by 0.8" and 5.0 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 | ATO J115.1508+55.3092 | 07:40:36.19 +55:18:33.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.302+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:36.19 +55:18:33.5: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:36.19 +55:18:33.5: 12.23 +/- 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
ATO J115.1508+55.3092,2461199.6803,11.13,0.05,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
ATO J115.1508+55.3092 20260608.1803 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 06 08.1803 2461199.6803 11.09 07:38:02.61 +55:53:42.3
161.63899 28.57714 galactic Lyn Second-epoch detections are separated by 0.6" and 5.0 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 986065568506456832 | 07:38:02.63 +55:53:42.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.274+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:02.61 +55:53:42.3: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:02.61 +55:53:42.3: 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 986065568506456832,2461199.6803,11.09,0.05,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 986065568506456832 20260608.1803 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 06 08.1803 2461199.6803 10.86 08:19:33.42 +54:53:34.6
163.18306 34.40333 galactic Lyn Second-epoch detections are separated by 1.3" and 4.9 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 1032384690553804416 | 08:19:33.41 +54:53:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.356+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:33.42 +54:53:34.6: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:33.42 +54:53:34.6: 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 1032384690553804416,2461199.6803,10.86,0.05,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 1032384690553804416 20260608.1803 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 06 08.1803 2461199.6803 10.95 08:19:25.81 +54:23:56.9
163.78170 34.38991 galactic Lyn Second-epoch detections are separated by 0.3" and 4.8 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 | ATO J124.8710+54.3922 | 08:19:25.81 +54:23:57.2 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.647+/-0.025 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:19:25.81 +54:23:56.9: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:19:25.81 +54:23:56.9: 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
ATO J124.8710+54.3922,2461199.6803,10.95,0.05,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
ATO J124.8710+54.3922 20260608.1803 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 06 08.1803 2461199.6803 11.13 08:24:38.92 +54:18:14.7
163.88301 35.15164 galactic Lyn Second-epoch detections are separated by 0.8" and 4.6 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 1032112668800636288 | 08:24:38.92 +54:18:15.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.550+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:38.92 +54:18:14.7: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:38.92 +54:18:14.7: 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 1032112668800636288,2461199.6803,11.13,0.05,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 1032112668800636288 20260608.1803 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 06 08.1803 2461199.6803 11.04 08:23:53.47 +54:35:02.7
163.54422 35.03465 galactic Lyn Second-epoch detections are separated by 0.9" and 4.9 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 1032132455714267648 | 08:23:53.46 +54:35:02.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5) J-Ks=0.228+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:53.47 +54:35:02.7: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:53.47 +54:35:02.7: 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 1032132455714267648,2461199.6803,11.04,0.05,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 1032132455714267648 20260608.1803 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 06 08.1803 2461199.6803 11.20 07:38:29.72 +54:15:26.6
163.49660 28.43074 galactic Lyn Second-epoch detections are separated by 1.4" and 5.4 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 985392461232577152 | 07:38:29.73 +54:15:24.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.320+/-0.049 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:29.72 +54:15:26.6: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:29.72 +54:15:26.6: 12.20 +/- 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 985392461232577152,2461199.6803,11.20,0.05,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 985392461232577152 20260608.1803 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 06 08.1803 2461199.6803 10.97 07:36:43.96 +55:13:09.0
162.37468 28.30742 galactic Lyn Second-epoch detections are separated by 1.2" and 5.1 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 | ATO J114.1828+55.2193 | 07:36:43.89 +55:13:09.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.541+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:43.96 +55:13:09.0: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:43.96 +55:13:09.0: 12.20 +/- 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
ATO J114.1828+55.2193,2461199.6803,10.97,0.05,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
ATO J114.1828+55.2193 20260608.1803 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 06 08.1803 2461199.6803 11.03 07:39:51.24 +54:38:15.0
163.09714 28.67647 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 985427164568228608 | 07:39:51.19 +54:38:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.394+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:51.24 +54:38:15.0: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:51.24 +54:38:15.0: 12.15 +/- 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 985427164568228608,2461199.6803,11.03,0.05,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 985427164568228608 20260608.1803 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 06 08.1803 2461199.6803 11.11 07:50:10.27 +52:52:47.8
165.30597 29.98215 galactic Lyn Second-epoch detections are separated by 0.6" and 5.2 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 984262919192277760 | 07:50:10.34 +52:52:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.354+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:50:10.27 +52:52:47.8: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:50:10.27 +52:52:47.8: 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 984262919192277760,2461199.6803,11.11,0.05,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 984262919192277760 20260608.1803 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 06 08.1803 2461199.6803 10.92 08:22:31.19 +55:03:51.3
162.96487 34.82498 galactic Lyn Second-epoch detections are separated by 0.4" and 4.7 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 1032364250805047808 | 08:22:31.21 +55:03:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.599+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:31.19 +55:03:51.3: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:31.19 +55:03:51.3: 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 1032364250805047808,2461199.6803,10.92,0.05,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 1032364250805047808 20260608.1803 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 06 08.1803 2461199.6803 11.09 07:44:22.96 +54:01:23.9
163.88639 29.25632 galactic Lyn Second-epoch detections are separated by 0.8" and 5.3 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 984588164180471936 | 07:44:22.94 +54:01:23.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.580+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:22.96 +54:01:23.9: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:22.96 +54:01:23.9: 12.12 +/- 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 984588164180471936,2461199.6803,11.09,0.05,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 984588164180471936 20260608.1803 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 06 08.1803 2461199.6803 11.14 07:49:35.56 +52:46:57.8
165.40622 29.88448 galactic Lyn Second-epoch detections are separated by 1.1" and 5.3 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 | ATO J117.3893+52.7845 | 07:49:35.56 +52:46:57.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.471+/-0.035 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:49:35.56 +52:46:57.8: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:49:35.56 +52:46:57.8: 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
ATO J117.3893+52.7845,2461199.6803,11.14,0.05,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
ATO J117.3893+52.7845 20260608.1803 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 06 08.1803 2461199.6803 11.50 08:21:06.79 +54:02:48.9
164.20686 34.63859 galactic Lyn Second-epoch detections are separated by 2.1" and 4.9 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 | 08:21:06.79 +54:02:48.9 (user input) | T | P | (position from user input) SpType: K0 (LAMOST DR5) J-Ks=0.540+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:06.79 +54:02:48.9: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:06.79 +54:02:48.9: 12.84 +/- 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,2461199.6803,11.50,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.55 07:37:26.97 +56:09:51.9
161.32316 28.52749 galactic Lyn Second-epoch detections are separated by 1.8" and 5.2 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 | 07:37:26.97 +56:09:51.9 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.409+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:26.97 +56:09:51.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:26.97 +56:09:51.9: 12.98 +/- 0.02 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,2461199.6803,11.55,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.65 07:38:53.07 +55:42:39.7
161.86343 28.67215 galactic Lyn Second-epoch detections are separated by 2.8" and 4.7 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 | 07:38:53.07 +55:42:39.7 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.260+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:53.07 +55:42:39.7: 15.25 +/- 0.24 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:53.07 +55:42:39.7: 13.16 +/- 0.03 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,2461199.6803,11.65,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.57 07:39:10.36 +54:45:52.7
162.93913 28.59511 galactic Lyn Second-epoch detections are separated by 0.5" and 5.2 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 | 07:39:10.36 +54:45:52.7 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.409+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:10.36 +54:45:52.7: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:10.36 +54:45:52.7: 13.01 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 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,2461199.6803,11.57,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.06 08:24:26.80 +54:03:54.0
164.17611 35.12746 galactic Lyn Second-epoch detections are separated by 0.8" and 4.6 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 J126.1119+54.0652 | 08:24:26.80 +54:03:54.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.295+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:26.80 +54:03:54.0: 12.04 +/- 0.01 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:26.80 +54:03:54.0: 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
ATO J126.1119+54.0652,2461199.6803,11.06,0.05,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
ATO J126.1119+54.0652 20260608.1803 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 06 08.1803 2461199.6803 11.56 07:38:04.77 +55:03:01.7
162.59343 28.47616 galactic Lyn Second-epoch detections are separated by 0.5" and 5.2 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 | 07:38:04.77 +55:03:01.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.364+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:04.77 +55:03:01.7: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:04.77 +55:03:01.7: 13.01 +/- 0.02 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,2461199.6803,11.56,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.29 08:23:42.64 +54:28:03.8
163.68704 35.01125 galactic Lyn Second-epoch detections are separated by 0.8" and 4.7 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 1032129225898865024 | 08:23:42.64 +54:28:04.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.787+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:42.64 +54:28:03.8: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:42.64 +54:28:03.8: 12.53 +/- 0.01 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 1032129225898865024,2461199.6803,11.29,0.05,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 1032129225898865024 20260608.1803 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 06 08.1803 2461199.6803 11.35 07:35:28.16 +56:19:03.1
161.11170 28.27348 galactic Lyn Second-epoch detections are separated by 0.5" and 5.1 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 986137758316671872 | 07:35:28.14 +56:19:02.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.511+/-0.035 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:28.16 +56:19:03.1: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:28.16 +56:19:03.1: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 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 986137758316671872,2461199.6803,11.35,0.05,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 986137758316671872 20260608.1803 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 06 08.1803 2461199.6803 11.30 07:38:46.84 +55:09:13.2
162.49152 28.58881 galactic Lyn Second-epoch detections are separated by 1.3" and 5.0 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 985632807601891840 | 07:38:46.88 +55:09:13.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.619+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:46.84 +55:09:13.2: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:46.84 +55:09:13.2: 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 985632807601891840,2461199.6803,11.30,0.05,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 985632807601891840 20260608.1803 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 06 08.1803 2461199.6803 11.43 08:29:00.74 +51:59:48.2
166.70253 35.84665 galactic Lyn Second-epoch detections are separated by 2.2" and 4.7 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 | ATO J127.2533+51.9967 | 08:29:00.79 +51:59:48.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.341+/-0.027 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:29:00.74 +51:59:48.2: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:29:00.74 +51:59:48.2: 12.63 +/- 0.01 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
ATO J127.2533+51.9967,2461199.6803,11.43,0.05,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
ATO J127.2533+51.9967 20260608.1803 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 06 08.1803 2461199.6803 11.70 07:35:37.12 +56:50:12.9
160.52916 28.35824 galactic Lyn Second-epoch detections are separated by 1.9" and 5.0 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 | 07:35:37.12 +56:50:12.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:37.12 +56:50:12.9: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:37.12 +56:50:12.9: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 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,2461199.6803,11.70,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.81 07:44:39.02 +54:49:01.2
162.98705 29.38527 galactic Lyn Second-epoch detections are separated by 2.0" and 4.9 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 | 07:44:39.02 +54:49:01.2 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.579+/-0.032 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:39.02 +54:49:01.2: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:39.02 +54:49:01.2: 12.99 +/- 0.02 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,2461199.6803,11.81,0.05,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
target 20260608.1803 11.81CV 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 06 08.1803 2461199.6803 11.57 07:39:33.19 +54:46:50.8
162.92888 28.65159 galactic Lyn Second-epoch detections are separated by 3.4" and 5.6 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 | 07:39:33.19 +54:46:50.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.390+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:33.19 +54:46:50.8: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:33.19 +54:46:50.8: 13.01 +/- 0.02 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,2461199.6803,11.57,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.80 07:39:44.46 +54:59:44.5
162.68972 28.70539 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 | 07:39:44.46 +54:59:44.5 (user input) | T | P | (position from user input) J-Ks=0.310+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:44.46 +54:59:44.5: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:44.46 +54:59:44.5: 13.36 +/- 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,2461199.6803,11.80,0.05,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
target 20260608.1803 11.80CV 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 06 08.1803 2461199.6803 11.54 07:35:32.80 +56:35:01.5
160.81325 28.31741 galactic Lyn Second-epoch detections are separated by 2.2" and 4.9 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 | 07:35:32.80 +56:35:01.5 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.482+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:32.80 +56:35:01.5: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:32.80 +56:35:01.5: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 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,2461199.6803,11.54,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.97 07:35:50.19 +55:18:14.2
162.25995 28.19222 galactic Lyn Second-epoch detections are separated by 0.1" and 5.2 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 985693276445096448 | 07:35:50.23 +55:18:13.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.250+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:50.19 +55:18:14.2: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:50.19 +55:18:14.2: 12.17 +/- 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 985693276445096448,2461199.6803,10.97,0.05,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 985693276445096448 20260608.1803 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 06 08.1803 2461199.6803 11.48 07:38:39.15 +55:04:11.9
162.58341 28.56002 galactic Lyn Second-epoch detections are separated by 3.1" and 4.8 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 | ATO J114.6614+55.0769 | 07:38:39.15 +55:04:11.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.354+/-0.035 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:39.15 +55:04:11.9: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:39.15 +55:04:11.9: 12.96 +/- 0.02 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
ATO J114.6614+55.0769,2461199.6803,11.48,0.05,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
ATO J114.6614+55.0769 20260608.1803 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 06 08.1803 2461199.6803 11.57 07:40:55.12 +55:03:00.8
162.65148 28.87956 galactic Lyn Second-epoch detections are separated by 2.6" and 5.1 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 | 07:40:55.12 +55:03:00.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.345+/-0.035 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:55.12 +55:03:00.8: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:55.12 +55:03:00.8: 13.06 +/- 0.02 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,2461199.6803,11.57,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.71 08:22:37.49 +54:18:22.1
163.88795 34.85645 galactic Lyn Second-epoch detections are separated by 1.0" and 4.8 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 | ATO J125.6535+54.3101 | 08:22:37.49 +54:18:22.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.341+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:37.49 +54:18:22.1: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:37.49 +54:18:22.1: 13.16 +/- 0.02 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
ATO J125.6535+54.3101,2461199.6803,11.71,0.05,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
ATO J125.6535+54.3101 20260608.1803 11.71CV 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 06 08.1803 2461199.6803 11.07 07:45:26.17 +53:55:16.8
164.02329 29.39827 galactic Lyn Second-epoch detections are separated by 1.4" and 5.0 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 | ATO J116.3590+53.9214 | 07:45:26.18 +53:55:17.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.454+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:45:26.17 +53:55:16.8: 14.49 +/- 0.09 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:45:26.17 +53:55:16.8: 12.11 +/- 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
ATO J116.3590+53.9214,2461199.6803,11.07,0.05,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
ATO J116.3590+53.9214 20260608.1803 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 06 08.1803 2461199.6803 11.52 07:40:35.14 +54:52:08.2
162.85029 28.81013 galactic Lyn Second-epoch detections are separated by 2.4" and 4.8 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 | 07:40:35.14 +54:52:08.2 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.757+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:35.14 +54:52:08.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:35.14 +54:52:08.2: 12.99 +/- 0.02 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,2461199.6803,11.52,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.61 07:44:21.86 +54:27:42.3
163.38675 29.30449 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 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 | 07:44:21.86 +54:27:42.3 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.531+/-0.027 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:21.86 +54:27:42.3: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:21.86 +54:27:42.3: 12.99 +/- 0.02 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,2461199.6803,11.61,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.52 08:18:43.13 +54:11:04.4
164.04211 34.28703 galactic Lyn Second-epoch detections are separated by 0.5" and 4.9 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 | 08:18:43.13 +54:11:04.4 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.465+/-0.025 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:18:43.13 +54:11:04.4: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:18:43.13 +54:11:04.4: 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,2461199.6803,11.52,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.40 07:47:48.82 +53:39:22.0
164.37179 29.71724 galactic Lyn Second-epoch detections are separated by 0.6" and 5.1 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 984521678086223872 | 07:47:48.80 +53:39:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.350+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:47:48.82 +53:39:22.0: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:47:48.82 +53:39:22.0: 12.56 +/- 0.01 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 984521678086223872,2461199.6803,11.40,0.05,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 984521678086223872 20260608.1803 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 06 08.1803 2461199.6803 11.51 07:41:00.69 +54:10:29.6
163.64489 28.78450 galactic Lyn Second-epoch detections are separated by 1.0" and 5.3 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 | ATO J115.2469+54.1755 | 07:41:00.73 +54:10:28.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.636+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:00.69 +54:10:29.6: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:00.69 +54:10:29.6: 12.67 +/- 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
ATO J115.2469+54.1755,2461199.6803,11.51,0.05,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
ATO J115.2469+54.1755 20260608.1803 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 06 08.1803 2461199.6803 11.35 07:37:48.24 +54:19:24.4
163.40659 28.33981 galactic Lyn Second-epoch detections are separated by 2.3" and 5.6 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 985396721840059904 | 07:37:48.31 +54:19:25.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.720+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:48.24 +54:19:24.4: 13.97 +/- 0.07 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:48.24 +54:19:24.4: 12.65 +/- 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 985396721840059904,2461199.6803,11.35,0.05,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 985396721840059904 20260608.1803 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 06 08.1803 2461199.6803 11.26 08:23:36.19 +55:24:14.5
162.54515 34.96918 galactic Lyn Second-epoch detections are separated by 0.9" and 4.7 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 1032378407017240704 | 08:23:36.16 +55:24:14.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5) J-Ks=0.246+/-0.026 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:36.19 +55:24:14.5: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:36.19 +55:24:14.5: 12.48 +/- 0.01 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 1032378407017240704,2461199.6803,11.26,0.05,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 1032378407017240704 20260608.1803 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 06 08.1803 2461199.6803 11.38 07:38:18.66 +54:32:43.9
163.16779 28.44288 galactic Lyn Second-epoch detections are separated by 2.1" and 4.9 pix
The object was found in VSX 1" ASASSN-V J073818.59+543243.7
Type: ROT
# Max. Min./Amp. JD0 Period
12.700 V 12.790 V 2457408.80200 1.202950000000
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:38:18.66 +54:32:43.9: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:38:18.66 +54:32:43.9: 12.65 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 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
ASASSN-V J073818.59+543243.7,2461199.6803,11.38,0.05,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
ASASSN-V J073818.59+543243.7 20260608.1803 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 06 08.1803 2461199.6803 11.49 07:44:05.45 +53:47:06.7
164.15136 29.18516 galactic Lyn Second-epoch detections are separated by 1.0" and 5.2 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 984560882548211712 | 07:44:05.51 +53:47:07.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.296+/-0.027 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:05.45 +53:47:06.7: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:05.45 +53:47:06.7: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 984560882548211712,2461199.6803,11.49,0.05,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
Gaia DR3 984560882548211712 20260608.1803 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 06 08.1803 2461199.6803 11.64 08:22:26.66 +53:32:01.4
164.82948 34.83919 galactic Lyn Second-epoch detections are separated by 0.6" and 4.8 pix
The object was found in VSX 1" Gaia DR3 1031968289180198400
Type: ROT
# Max. Min./Amp. JD0 Period
12.730 G 12.760 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:26.66 +53:32:01.4: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:26.66 +53:32:01.4: 12.90 +/- 0.02 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 1031968289180198400,2461199.6803,11.64,0.05,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
Gaia DR3 1031968289180198400 20260608.1803 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 06 08.1803 2461199.6803 11.95 07:48:35.73 +52:59:32.6
165.14643 29.75883 galactic Lyn Second-epoch detections are separated by 2.4" and 5.4 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 | 07:48:35.73 +52:59:32.6 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.456+/-0.035 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:48:35.73 +52:59:32.6: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:48:35.73 +52:59:32.6: 13.28 +/- 0.03 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,2461199.6803,11.95,0.05,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
target 20260608.1803 11.95CV 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 06 08.1803 2461199.6803 11.46 07:49:53.36 +53:05:26.1
165.05891 29.96304 galactic Lyn Second-epoch detections are separated by 2.4" and 5.0 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 | 07:49:53.36 +53:05:26.1 (user input) | T | P | (position from user input) J-Ks=0.258+/-0.039 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:49:53.36 +53:05:26.1: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:49:53.36 +53:05:26.1: 12.53 +/- 0.01 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
target,2461199.6803,11.46,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.36 07:45:59.28 +53:44:56.4
164.23062 29.45925 galactic Lyn Second-epoch detections are separated by 1.4" and 5.3 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 | 07:45:59.28 +53:44:56.4 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.386+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:45:59.28 +53:44:56.4: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:45:59.28 +53:44:56.4: 12.63 +/- 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
target,2461199.6803,11.36,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.36 08:22:55.28 +53:36:27.3
164.73873 34.90939 galactic Lyn Second-epoch detections are separated by 0.8" and 4.8 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 | Gaia DR3 1031970415188327040 | 08:22:55.24 +53:36:27.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.231+/-0.031 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:55.28 +53:36:27.3: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:55.28 +53:36:27.3: 12.51 +/- 0.01 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 1031970415188327040,2461199.6803,11.36,0.05,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 1031970415188327040 20260608.1803 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 06 08.1803 2461199.6803 11.38 08:23:40.92 +54:46:16.5
163.31671 34.99960 galactic Lyn Second-epoch detections are separated by 1.6" and 4.7 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 | ATO J125.9187+54.7805 | 08:23:39.89 +54:46:40.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.629+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:40.92 +54:46:16.5: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:40.92 +54:46:16.5: 12.43 +/- 0.01 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
ATO J125.9187+54.7805,2461199.6803,11.38,0.05,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
ATO J125.9187+54.7805 20260608.1803 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 06 08.1803 2461199.6803 11.03 07:36:22.29 +56:24:37.3
161.02473 28.40900 galactic Lyn Second-epoch detections are separated by 0.5" and 5.1 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 | ATO J114.0928+56.4104 | 07:36:22.27 +56:24:37.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:22.29 +56:24:37.3: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:22.29 +56:24:37.3: 12.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 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 J114.0928+56.4104,2461199.6803,11.03,0.05,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
ATO J114.0928+56.4104 20260608.1803 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 06 08.1803 2461199.6803 12.15 08:22:49.52 +55:15:05.6
162.73527 34.86343 galactic Lyn Second-epoch detections are separated by 2.0" and 4.8 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 | 08:22:49.52 +55:15:05.6 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:49.52 +55:15:05.6: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:49.52 +55:15:05.6: 13.95 +/- 0.05 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,2461199.6803,12.15,0.05,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 20260608.1803 12.15CV 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 06 08.1803 2461199.6803 11.87 08:22:13.07 +54:58:34.6
163.07329 34.78390 galactic Lyn Second-epoch detections are separated by 1.7" and 5.0 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 | 08:22:13.07 +54:58:34.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.257+/-0.036 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:13.07 +54:58:34.6: 16.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:13.07 +54:58:34.6: 13.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 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,2461199.6803,11.87,0.05,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
target 20260608.1803 11.87CV 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 06 08.1803 2461199.6803 11.22 07:37:53.68 +55:27:34.6
162.12791 28.50234 galactic Lyn Second-epoch detections are separated by 0.9" and 5.0 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 986026535843733376 | 07:37:53.66 +55:27:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.358+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:53.68 +55:27:34.6: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:53.68 +55:27:34.6: 12.58 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 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 986026535843733376,2461199.6803,11.22,0.05,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 986026535843733376 20260608.1803 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 06 08.1803 2461199.6803 11.39 07:43:01.13 +54:24:35.6
163.41968 29.10415 galactic Lyn Second-epoch detections are separated by 0.8" and 5.2 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 | 07:43:01.13 +54:24:35.6 (user input) | T | P | (position from user input) SpType: F7 (LAMOST DR5) J-Ks=0.285+/-0.032 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:01.13 +54:24:35.6: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:01.13 +54:24:35.6: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 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,2461199.6803,11.39,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 12.07 07:39:52.30 +55:41:14.5
161.90910 28.80743 galactic Lyn Second-epoch detections are separated by 3.6" and 5.6 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 | 07:39:52.30 +55:41:14.5 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5) J-Ks=0.592+/-0.030 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:52.30 +55:41:14.5: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:52.30 +55:41:14.5: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 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,2461199.6803,12.07,0.05,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 20260608.1803 12.07CV 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 06 08.1803 2461199.6803 11.77 07:45:22.97 +53:44:34.4
164.22564 29.36968 galactic Lyn Second-epoch detections are separated by 2.2" and 5.5 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 J116.3428+53.7467 | 07:45:22.97 +53:44:34.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.389+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:45:22.97 +53:44:34.4: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:45:22.97 +53:44:34.4: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 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
ATO J116.3428+53.7467,2461199.6803,11.77,0.05,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
ATO J116.3428+53.7467 20260608.1803 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 06 08.1803 2461199.6803 11.39 07:40:54.44 +54:44:27.3
163.00181 28.84042 galactic Lyn Second-epoch detections are separated by 0.4" and 5.1 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 985423586859128832 | 07:40:54.42 +54:44:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.297+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:54.44 +54:44:27.3: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:54.44 +54:44:27.3: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 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 985423586859128832,2461199.6803,11.39,0.05,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
Gaia DR3 985423586859128832 20260608.1803 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 06 08.1803 2461199.6803 10.86 08:21:35.48 +54:36:01.3
163.53290 34.70125 galactic Lyn Second-epoch detections are separated by 0.8" and 4.7 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 1032327657683742848 | 08:21:35.50 +54:36:02.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.694+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:35.48 +54:36:01.3: 15.25 +/- 0.15 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:35.48 +54:36:01.3: 12.01 +/- 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 1032327657683742848,2461199.6803,10.86,0.05,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 1032327657683742848 20260608.1803 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 06 08.1803 2461199.6803 11.14 07:43:18.92 +55:00:17.6
162.74855 29.21542 galactic Lyn Second-epoch detections are separated by 0.9" and 5.2 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 | ATO J115.8251+55.0043 | 07:43:18.94 +55:00:17.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.334+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:18.92 +55:00:17.6: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:18.92 +55:00:17.6: 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
ATO J115.8251+55.0043,2461199.6803,11.14,0.05,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
ATO J115.8251+55.0043 20260608.1803 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 06 08.1803 2461199.6803 10.89 08:18:15.86 +54:52:42.3
163.20307 34.21761 galactic Lyn Second-epoch detections are separated by 1.3" and 4.6 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 J124.5515+54.8884 | 08:18:15.86 +54:52:42.9 (Gaia DR3) | PULSE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5) J-Ks=0.570+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:18:15.86 +54:52:42.3: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:18:15.86 +54:52:42.3: 12.03 +/- 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
ATO J124.5515+54.8884,2461199.6803,10.89,0.05,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
ATO J124.5515+54.8884 20260608.1803 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 06 08.1803 2461199.6803 11.51 08:27:23.91 +52:26:37.0
166.15546 35.59459 galactic Lyn Second-epoch detections are separated by 2.4" and 4.5 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 1028812553369939200 | 08:27:23.79 +52:26:37.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.352+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:27:23.91 +52:26:37.0: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:27:23.91 +52:26:37.0: 12.50 +/- 0.01 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 1028812553369939200,2461199.6803,11.51,0.05,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
Gaia DR3 1028812553369939200 20260608.1803 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 06 08.1803 2461199.6803 11.38 08:21:08.91 +54:34:15.1
163.57001 34.63758 galactic Lyn Second-epoch detections are separated by 1.4" and 4.8 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 | 08:21:08.91 +54:34:15.1 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.599+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:08.91 +54:34:15.1: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:08.91 +54:34:15.1: 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,2461199.6803,11.38,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.58 07:35:20.98 +55:46:23.8
161.72179 28.18654 galactic Lyn Second-epoch detections are separated by 0.8" and 5.2 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 | 07:35:20.98 +55:46:23.8 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.324+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:20.98 +55:46:23.8: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:20.98 +55:46:23.8: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 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,2461199.6803,11.58,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 10.91 07:37:35.63 +54:44:12.2
162.93661 28.36561 galactic Lyn Second-epoch detections are separated by 1.2" and 5.4 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 | ATO J114.3983+54.7367 | 07:37:35.60 +54:44:12.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.694+/-0.029 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:35.63 +54:44:12.2: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:35.63 +54:44:12.2: 12.15 +/- 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
ATO J114.3983+54.7367,2461199.6803,10.91,0.05,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
ATO J114.3983+54.7367 20260608.1803 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 06 08.1803 2461199.6803 10.85 08:22:47.67 +55:41:20.1
162.20273 34.84512 galactic Lyn Second-epoch detections are separated by 0.5" and 4.7 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 1033933322617308928 | 08:22:47.66 +55:41:20.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.636+/-0.023 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:47.67 +55:41:20.1: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:47.67 +55:41:20.1: 11.96 +/- 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 1033933322617308928,2461199.6803,10.85,0.05,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 1033933322617308928 20260608.1803 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 06 08.1803 2461199.6803 10.97 07:37:48.36 +54:57:19.2
162.69490 28.42487 galactic Lyn Second-epoch detections are separated by 0.5" and 5.3 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 985625282819207296 | 07:37:48.33 +54:57:20.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5) J-Ks=0.441+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:37:48.36 +54:57:19.2: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:37:48.36 +54:57:19.2: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 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 985625282819207296,2461199.6803,10.97,0.05,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 985625282819207296 20260608.1803 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 06 08.1803 2461199.6803 10.96 07:34:31.07 +56:44:46.8
160.61008 28.19748 galactic Lyn Second-epoch detections are separated by 1.0" and 5.2 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 989155157524638336 | 07:34:31.09 +56:44:46.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5) J-Ks=0.299+/-0.032 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:34:31.07 +56:44:46.8: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:34:31.07 +56:44:46.8: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 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 989155157524638336,2461199.6803,10.96,0.05,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 989155157524638336 20260608.1803 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 06 08.1803 2461199.6803 10.99 07:41:15.74 +54:25:12.5
163.37249 28.85177 galactic Lyn Second-epoch detections are separated by 1.8" and 5.5 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 985409327567718912 | 07:41:15.71 +54:25:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=11.289+/- (unrealisitic color!)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:15.74 +54:25:12.5: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:15.74 +54:25:12.5: 12.03 +/- 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 985409327567718912,2461199.6803,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 985409327567718912 20260608.1803 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 08.1803 2461199.6803 11.71 07:53:10.49 +52:11:45.9
166.14965 30.36198 galactic Lyn Second-epoch detections are separated by 0.6" and 5.2 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 | 07:53:10.49 +52:11:45.9 (user input) | T | P | (position from user input) J-Ks=0.538+/-0.032 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:53:10.49 +52:11:45.9: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:53:10.49 +52:11:45.9: 12.90 +/- 0.02 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,2461199.6803,11.71,0.05,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
target 20260608.1803 11.71CV 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 06 08.1803 2461199.6803 10.75 08:20:05.67 +54:56:32.2
163.12190 34.47984 galactic Lyn Second-epoch detections are separated by 0.7" and 4.7 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 | ATO J125.0218+54.9395 | 08:20:05.75 +54:56:33.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.677+/-0.026 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:05.67 +54:56:32.2: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:05.67 +54:56:32.2: 11.94 +/- 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
ATO J125.0218+54.9395,2461199.6803,10.75,0.05,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
ATO J125.0218+54.9395 20260608.1803 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 06 08.1803 2461199.6803 10.86 08:22:45.55 +54:48:16.4
163.28017 34.86578 galactic Lyn Second-epoch detections are separated by 0.3" and 4.8 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 | ATO J125.6899+54.8045 | 08:22:45.59 +54:48:16.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.357+/-0.026 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:22:45.55 +54:48:16.4: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:22:45.55 +54:48:16.4: 11.94 +/- 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
ATO J125.6899+54.8045,2461199.6803,10.86,0.05,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
ATO J125.6899+54.8045 20260608.1803 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 06 08.1803 2461199.6803 11.02 08:18:00.98 +54:09:28.7
164.07430 34.18424 galactic Lyn Second-epoch detections are separated by 0.7" and 4.7 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 1032247908730938880 | 08:18:00.96 +54:09:28.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.465+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:18:00.98 +54:09:28.7: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:18:00.98 +54:09:28.7: 11.94 +/- 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 1032247908730938880,2461199.6803,11.02,0.05,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 1032247908730938880 20260608.1803 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 06 08.1803 2461199.6803 10.94 07:39:04.24 +54:47:15.5
162.91100 28.58348 galactic Lyn Second-epoch detections are separated by 1.7" and 5.0 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 | ATO J114.7676+54.7875 | 07:39:04.24 +54:47:15.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.797+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:04.24 +54:47:15.5: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:04.24 +54:47:15.5: 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
ATO J114.7676+54.7875,2461199.6803,10.94,0.05,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
ATO J114.7676+54.7875 20260608.1803 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 06 08.1803 2461199.6803 10.97 07:36:59.57 +56:15:00.8
161.21746 28.47489 galactic Lyn Second-epoch detections are separated by 0.3" and 5.1 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 986127033782490752 | 07:36:59.60 +56:15:01.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.753+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:36:59.57 +56:15:00.8: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:36:59.57 +56:15:00.8: 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 986127033782490752,2461199.6803,10.97,0.05,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 986127033782490752 20260608.1803 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 06 08.1803 2461199.6803 11.36 08:21:58.92 +54:51:27.6
163.21857 34.75270 galactic Lyn Second-epoch detections are separated by 0.7" and 4.8 pix
The object was found in VSX 1" Gaia DR3 1032337622007862528
Type: ROT
# Max. Min./Amp. JD0 Period
12.580 G 12.610 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:58.92 +54:51:27.6: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:58.92 +54:51:27.6: 12.84 +/- 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
Gaia DR3 1032337622007862528,2461199.6803,11.36,0.05,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 1032337622007862528 20260608.1803 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 06 08.1803 2461199.6803 11.78 07:35:52.42 +56:41:08.9
160.70444 28.37457 galactic Lyn Second-epoch detections are separated by 2.4" and 4.8 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 | 07:35:52.42 +56:41:08.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.345+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:52.42 +56:41:08.9: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:52.42 +56:41:08.9: 13.31 +/- 0.03 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,2461199.6803,11.78,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.75 08:20:39.37 +54:15:45.2
163.94562 34.56974 galactic Lyn Second-epoch detections are separated by 3.2" and 4.5 pix
The object was found in VSX19" Gaia DR3 1032212174603011584
Type: ROT
# Max. Min./Amp. JD0 Period
14.480 G 14.500 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:39.37 +54:15:45.2: 16.28 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:39.37 +54:15:45.2: 13.30 +/- 0.02 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
Gaia DR3 1032212174603011584,2461199.6803,11.75,0.05,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 1032212174603011584 20260608.1803 11.75CV 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 06 08.1803 2461199.6803 11.74 07:53:37.95 +52:35:22.3
165.70434 30.47245 galactic Lyn Second-epoch detections are separated by 1.4" and 5.0 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 | 07:53:37.95 +52:35:22.3 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.607+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:53:37.95 +52:35:22.3: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:53:37.95 +52:35:22.3: 12.89 +/- 0.02 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,2461199.6803,11.74,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.53 07:41:20.66 +54:21:52.3
163.43718 28.85667 galactic Lyn Second-epoch detections are separated by 2.1" and 5.4 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 | 07:41:20.66 +54:21:52.3 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.337+/-0.035 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:20.66 +54:21:52.3: 15.85 +/- 0.34 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:20.66 +54:21:52.3: 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
target,2461199.6803,11.53,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.55 07:44:41.74 +53:52:22.7
164.06375 29.28428 galactic Lyn Second-epoch detections are separated by 0.8" and 5.1 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 | 07:44:41.74 +53:52:22.7 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.326+/-0.026 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:41.74 +53:52:22.7: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:41.74 +53:52:22.7: 12.86 +/- 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,2461199.6803,11.55,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.59 07:39:04.30 +55:12:49.1
162.42967 28.63753 galactic Lyn Second-epoch detections are separated by 0.8" and 5.0 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 | ATO J114.7667+55.2153 | 07:39:04.30 +55:12:49.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.275+/-0.036 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:04.30 +55:12:49.1: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:04.30 +55:12:49.1: 12.96 +/- 0.02 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
ATO J114.7667+55.2153,2461199.6803,11.59,0.05,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
ATO J114.7667+55.2153 20260608.1803 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 06 08.1803 2461199.6803 11.71 07:40:50.18 +55:35:46.9
162.03036 28.93204 galactic Lyn Second-epoch detections are separated by 0.8" and 5.3 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 | 07:40:50.18 +55:35:46.9 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.233+/-0.035 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:40:50.18 +55:35:46.9: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:40:50.18 +55:35:46.9: 12.95 +/- 0.02 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,2461199.6803,11.71,0.05,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
target 20260608.1803 11.71CV 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 06 08.1803 2461199.6803 11.46 08:29:53.95 +52:11:45.2
166.45432 35.98010 galactic Lyn Second-epoch detections are separated by 2.1" and 5.0 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 1028608417868225664 | 08:29:53.91 +52:11:45.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.387+/-0.029 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:29:53.95 +52:11:45.2: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:29:53.95 +52:11:45.2: 12.59 +/- 0.01 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 1028608417868225664,2461199.6803,11.46,0.05,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 1028608417868225664 20260608.1803 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 06 08.1803 2461199.6803 11.81 07:43:47.59 +53:50:56.9
164.07256 29.14932 galactic Lyn Second-epoch detections are separated by 1.4" and 4.9 pix
The object was found in VSX 0" Gaia DR3 984563463824361984
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.150 G 13.180 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:47.59 +53:50:56.9: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:47.59 +53:50:56.9: 13.31 +/- 0.03 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
Gaia DR3 984563463824361984,2461199.6803,11.81,0.05,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 984563463824361984 20260608.1803 11.81CV 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 06 08.1803 2461199.6803 11.40 08:24:00.01 +53:29:07.2
164.88583 35.07095 galactic Lyn Second-epoch detections are separated by 0.8" and 4.9 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 1031941553008102912 | 08:23:59.98 +53:29:07.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.242+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:00.01 +53:29:07.2: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:00.01 +53:29:07.2: 12.48 +/- 0.01 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 1031941553008102912,2461199.6803,11.40,0.05,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 1031941553008102912 20260608.1803 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 06 08.1803 2461199.6803 11.88 07:50:57.44 +53:13:44.6
164.91952 30.13695 galactic Lyn Second-epoch detections are separated by 1.7" and 5.4 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 | 07:50:57.44 +53:13:44.6 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:50:57.44 +53:13:44.6: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:50:57.44 +53:13:44.6: 13.17 +/- 0.02 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,2461199.6803,11.88,0.05,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
target 20260608.1803 11.88CV 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 06 08.1803 2461199.6803 11.62 07:39:41.30 +55:00:42.1
162.67055 28.69989 galactic Lyn Second-epoch detections are separated by 0.8" and 5.3 pix
The object was found in VSX 1" Gaia DR3 985442970047841664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.060 G 13.090 G F
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:41.30 +55:00:42.1: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:41.30 +55:00:42.1: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 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 985442970047841664,2461199.6803,11.62,0.05,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
Gaia DR3 985442970047841664 20260608.1803 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 06 08.1803 2461199.6803 11.34 07:39:08.76 +54:49:25.6
162.87177 28.59888 galactic Lyn Second-epoch detections are separated by 2.0" and 5.0 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 985434242674302720 | 07:39:08.73 +54:49:25.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5) J-Ks=0.402+/-0.030 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:08.76 +54:49:25.6: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:08.76 +54:49:25.6: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 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 985434242674302720,2461199.6803,11.34,0.05,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
Gaia DR3 985434242674302720 20260608.1803 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 06 08.1803 2461199.6803 11.38 08:27:56.28 +50:40:42.4
168.32733 35.67995 galactic Lyn Second-epoch detections are separated by 1.8" and 4.8 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 | Gaia DR3 1028011662227718656 | 08:27:56.23 +50:40:43.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G6 (LAMOST DR5) J-Ks=0.527+/-0.027 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:27:56.28 +50:40:42.4: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:27:56.28 +50:40:42.4: 12.55 +/- 0.01 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 1028011662227718656,2461199.6803,11.38,0.05,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 1028011662227718656 20260608.1803 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 06 08.1803 2461199.6803 11.47 07:42:24.42 +53:51:11.6
164.03895 28.94698 galactic Lyn Second-epoch detections are separated by 0.6" and 5.3 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 985310581976079232 | 07:42:24.45 +53:51:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.308+/-0.028 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:24.42 +53:51:11.6: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:24.42 +53:51:11.6: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 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 985310581976079232,2461199.6803,11.47,0.05,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
Gaia DR3 985310581976079232 20260608.1803 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 06 08.1803 2461199.6803 11.80 07:35:55.79 +56:20:54.4
161.08597 28.34068 galactic Lyn Second-epoch detections are separated by 2.7" and 5.3 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 | 07:35:55.79 +56:20:54.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.285+/-0.033 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:35:55.79 +56:20:54.4: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:35:55.79 +56:20:54.4: 13.27 +/- 0.03 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,2461199.6803,11.80,0.05,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
target 20260608.1803 11.80CV 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 06 08.1803 2461199.6803 11.72 07:41:45.24 +54:35:30.2
163.18802 28.94370 galactic Lyn Second-epoch detections are separated by 1.5" and 5.0 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 | 07:41:45.24 +54:35:30.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.614+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:45.24 +54:35:30.2: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:45.24 +54:35:30.2: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 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,2461199.6803,11.72,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.42 07:50:03.77 +52:27:27.8
165.78805 29.91842 galactic Lyn Second-epoch detections are separated by 0.5" and 5.1 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 984154853519393664 | 07:50:03.64 +52:27:27.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.336+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:50:03.77 +52:27:27.8: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:50:03.77 +52:27:27.8: 12.51 +/- 0.01 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 984154853519393664,2461199.6803,11.42,0.05,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 984154853519393664 20260608.1803 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 06 08.1803 2461199.6803 11.70 08:23:04.26 +54:08:51.7
164.07975 34.92432 galactic Lyn Second-epoch detections are separated by 1.7" and 4.6 pix
The object was found in VSX 1" Gaia DR3 1032022680646019712
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.960 G 12.980 G G
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:04.26 +54:08:51.7: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:04.26 +54:08:51.7: 13.08 +/- 0.02 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
Gaia DR3 1032022680646019712,2461199.6803,11.70,0.05,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
Gaia DR3 1032022680646019712 20260608.1803 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 06 08.1803 2461199.6803 11.65 08:23:26.01 +56:13:04.6
161.55411 34.91392 galactic Lyn Second-epoch detections are separated by 2.1" and 4.4 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 | ATO J125.8600+56.2148 | 08:23:26.01 +56:13:04.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.404+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:23:26.01 +56:13:04.6: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:23:26.01 +56:13:04.6: 12.78 +/- 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
ATO J125.8600+56.2148,2461199.6803,11.65,0.05,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
ATO J125.8600+56.2148 20260608.1803 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 06 08.1803 2461199.6803 11.59 08:24:10.77 +54:33:44.8
163.56935 35.07696 galactic Lyn Second-epoch detections are separated by 1.4" and 4.5 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 | 08:24:10.77 +54:33:44.8 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.320+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:10.77 +54:33:44.8: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:10.77 +54:33:44.8: 12.78 +/- 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
target,2461199.6803,11.59,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.35 08:21:21.61 +54:39:08.7
163.47029 34.66692 galactic Lyn Second-epoch detections are separated by 1.6" and 5.0 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 | 08:21:21.61 +54:39:08.7 (user input) | T | P | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.378+/-0.072 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:21.61 +54:39:08.7: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:21.61 +54:39:08.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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,2461199.6803,11.35,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.03 07:42:15.94 +55:05:09.1
162.63690 29.07524 galactic Lyn Second-epoch detections are separated by 0.8" and 5.2 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 985809515440110464 | 07:42:15.98 +55:05:08.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.316+/-0.030 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:15.94 +55:05:09.1: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:15.94 +55:05:09.1: 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 985809515440110464,2461199.6803,11.03,0.05,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 985809515440110464 20260608.1803 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 06 08.1803 2461199.6803 10.96 08:24:36.23 +55:23:44.8
162.54902 35.11144 galactic Lyn Second-epoch detections are separated by 0.6" and 4.7 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 | ATO J126.1442+55.3930 | 08:24:36.14 +55:23:44.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5) J-Ks=0.681+/-0.028 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:24:36.23 +55:23:44.8: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:24:36.23 +55:23:44.8: 11.91 +/- 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
ATO J126.1442+55.3930,2461199.6803,10.96,0.05,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
ATO J126.1442+55.3930 20260608.1803 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 06 08.1803 2461199.6803 10.94 07:46:38.01 +53:27:12.3
164.58065 29.52017 galactic Lyn Second-epoch detections are separated by 0.3" and 5.1 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 | ATO J116.6667+53.4555 | 07:46:38.01 +53:27:12.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.451+/-0.034 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:46:38.01 +53:27:12.3: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:46:38.01 +53:27:12.3: 11.97 +/- 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
ATO J116.6667+53.4555,2461199.6803,10.94,0.05,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
ATO J116.6667+53.4555 20260608.1803 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 06 08.1803 2461199.6803 11.47 07:42:32.80 +53:57:04.7
163.93068 28.97970 galactic Lyn Second-epoch detections are separated by 1.9" and 5.4 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 985316869808193024 | 07:42:32.90 +53:57:05.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.477+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:42:32.80 +53:57:04.7: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:42:32.80 +53:57:04.7: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 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 985316869808193024,2461199.6803,11.47,0.05,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
Gaia DR3 985316869808193024 20260608.1803 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 06 08.1803 2461199.6803 11.51 07:44:07.41 +54:46:12.7
163.03079 29.30463 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 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 985751864095629184 | 07:44:07.43 +54:46:13.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5) J-Ks=0.347+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:44:07.41 +54:46:12.7: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:44:07.41 +54:46:12.7: 12.50 +/- 0.01 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 985751864095629184,2461199.6803,11.51,0.05,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
Gaia DR3 985751864095629184 20260608.1803 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 06 08.1803 2461199.6803 11.30 07:48:40.33 +53:10:16.0
164.94335 29.79048 galactic Lyn Second-epoch detections are separated by 1.2" and 4.9 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 | ATO J117.1681+53.1708 | 07:48:40.36 +53:10:15.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.651+/-0.034 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:48:40.33 +53:10:16.0: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:48:40.33 +53:10:16.0: 12.51 +/- 0.01 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
ATO J117.1681+53.1708,2461199.6803,11.30,0.05,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
ATO J117.1681+53.1708 20260608.1803 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 06 08.1803 2461199.6803 11.38 08:25:03.30 +54:21:28.6
163.81529 35.20948 galactic Lyn Second-epoch detections are separated by 0.5" and 4.8 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 | Gaia DR3 1032112531361679360 | 08:25:03.32 +54:21:28.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.645+/-0.027 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:03.30 +54:21:28.6: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:03.30 +54:21:28.6: 12.43 +/- 0.01 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 1032112531361679360,2461199.6803,11.38,0.05,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 1032112531361679360 20260608.1803 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 06 08.1803 2461199.6803 11.42 07:41:49.86 +54:54:21.4
162.83296 28.99236 galactic Lyn Second-epoch detections are separated by 0.9" and 5.2 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 985800826722823680 | 07:41:49.93 +54:54:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.556+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:41:49.86 +54:54:21.4: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:41:49.86 +54:54:21.4: 12.54 +/- 0.01 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 985800826722823680,2461199.6803,11.42,0.05,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 985800826722823680 20260608.1803 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 06 08.1803 2461199.6803 11.37 07:43:23.87 +54:32:38.3
163.27465 29.17458 galactic Lyn Second-epoch detections are separated by 0.4" and 5.1 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 985367894019575168 | 07:43:23.86 +54:32:37.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5) J-Ks=0.265+/-0.032 (F)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:43:23.87 +54:32:38.3: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:43:23.87 +54:32:38.3: 12.56 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 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 985367894019575168,2461199.6803,11.37,0.05,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
Gaia DR3 985367894019575168 20260608.1803 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 06 08.1803 2461199.6803 11.24 07:39:43.66 +55:32:36.0
162.06954 28.77020 galactic Lyn Second-epoch detections are separated by 0.1" and 5.1 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 986022412675110784 | 07:39:43.68 +55:32:34.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.597+/-0.033 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:43.66 +55:32:36.0: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:43.66 +55:32:36.0: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 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 986022412675110784,2461199.6803,11.24,0.05,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
Gaia DR3 986022412675110784 20260608.1803 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 06 08.1803 2461199.6803 11.29 08:20:01.93 +54:08:55.3
164.08467 34.47939 galactic Lyn Second-epoch detections are separated by 1.0" and 4.6 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 1032209730766254720 | 08:20:01.93 +54:08:55.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.369+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:20:01.93 +54:08:55.3: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:20:01.93 +54:08:55.3: 12.47 +/- 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 1032209730766254720,2461199.6803,11.29,0.05,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 1032209730766254720 20260608.1803 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 06 08.1803 2461199.6803 11.47 08:25:50.51 +53:25:39.8
164.95135 35.34592 galactic Lyn Second-epoch detections are separated by 1.1" and 4.7 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 1031926469082753152 | 08:25:50.40 +53:25:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.572+/-0.031 (K)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:50.51 +53:25:39.8: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:50.51 +53:25:39.8: 12.47 +/- 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 1031926469082753152,2461199.6803,11.47,0.05,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
Gaia DR3 1031926469082753152 20260608.1803 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 06 08.1803 2461199.6803 11.48 07:46:20.22 +53:26:35.0
164.58656 29.47512 galactic Lyn Second-epoch detections are separated by 2.0" and 5.5 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 | 07:46:20.22 +53:26:35.0 (user input) | T | P | (position from user input) J-Ks=0.346+/-0.033 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:46:20.22 +53:26:35.0: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:46:20.22 +53:26:35.0: 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,2461199.6803,11.48,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.71 08:25:40.78 +53:36:12.7
164.73644 35.31856 galactic Lyn Second-epoch detections are separated by 2.4" and 5.2 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 | ATO J126.4203+53.6035 | 08:25:40.78 +53:36:12.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.404+/-0.031 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:25:40.78 +53:36:12.7: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:25:40.78 +53:36:12.7: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 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
ATO J126.4203+53.6035,2461199.6803,11.71,0.05,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
ATO J126.4203+53.6035 20260608.1803 11.71CV 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 06 08.1803 2461199.6803 11.27 07:39:34.92 +54:57:16.6
162.73294 28.67763 galactic Lyn Second-epoch detections are separated by 0.7" and 5.2 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 985441286420663680 | 07:39:34.90 +54:57:17.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5) J-Ks=0.345+/-0.032 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:39:34.92 +54:57:16.6: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:39:34.92 +54:57:16.6: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 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 985441286420663680,2461199.6803,11.27,0.05,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 985441286420663680 20260608.1803 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 06 08.1803 2461199.6803 11.37 07:49:12.58 +52:57:39.1
165.19460 29.84712 galactic Lyn Second-epoch detections are separated by 1.7" and 5.4 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 | 07:49:12.58 +52:57:39.1 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5) J-Ks=0.424+/-0.037 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:49:12.58 +52:57:39.1: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:49:12.58 +52:57:39.1: 12.51 +/- 0.01 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
target,2461199.6803,11.37,0.05,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 20260608.1803 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 06 08.1803 2461199.6803 11.39 07:49:09.01 +52:56:11.4
165.22134 29.83547 galactic Lyn Second-epoch detections are separated by 1.7" and 5.1 pix
The object was found in VSX 0" Gaia DR3 984278617297024384
Type: ROT
# Max. Min./Amp. JD0 Period
12.340 G 12.370 G G
The object was not found in astcheck.
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 07:49:09.01 +52:56:11.4: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 07:49:09.01 +52:56:11.4: 12.51 +/- 0.01 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 984278617297024384,2461199.6803,11.39,0.05,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
Gaia DR3 984278617297024384 20260608.1803 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 06 08.1803 2461199.6803 11.46 08:31:03.57 +52:28:11.3
166.11108 36.15176 galactic Lyn Second-epoch detections are separated by 0.5" and 4.7 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 | ATO J127.7651+52.4700 | 08:31:03.63 +52:28:12.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.395+/-0.028 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:31:03.57 +52:28:11.3: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:31:03.57 +52:28:11.3: 12.50 +/- 0.01 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
ATO J127.7651+52.4700,2461199.6803,11.46,0.05,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
ATO J127.7651+52.4700 20260608.1803 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 06 08.1803 2461199.6803 10.73 08:21:01.17 +54:50:26.5
163.24251 34.61452 galactic Lyn Second-epoch detections are separated by 0.9" and 4.8 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 | Gaia DR3 1032335319905399936 | 08:21:01.19 +54:50:26.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.326+/-0.024 (G)
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits at 08:21:01.17 +54:50:26.5: 15.15 +/- 0.13 detection
Forced photometry on wcs_Lyn-02-Q1b1x1_2026-03-21_00-15-59_20.00sec_-14.90C_LIGHT_0207.fits at 08:21:01.17 +54:50:26.5: 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 1032335319905399936,2461199.6803,10.73,0.05,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 1032335319905399936 20260608.1803 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
ERROR running VaST on the field Lyn-02-Q1b1x1 (wrong field? clouds? very bad focus?)
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.73517407 22.02.2026 05:38:29.040 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461093.73517407 22.02.2026 05:38:29.040 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461199.68049156 08.06.2026 04:19:44.471 /data_ssd/NMW-TexasTech/workdir//img_2026-06-07_CI_Lyn-02-Q1b1x1_232445_TTUQ1b1x1_306739_sGz00Y8F/fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 548
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.22
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: 13 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 50941
Objects passed selection criteria: 50785
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: 31195
Average stars matched: 30085.2 (96.4425 %)
Memory usage VmPeak: 154984 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Jun 7 22:21:29 CDT 2026
VaST build number 1.0rc89-90-g333d5534
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 7 23:27:26 CDT 2026
Host name: tau
############################################################
**** FOUND 08:18:09.63 +54:10:19.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 23850_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23850_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29520_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29520_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28851_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28851_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22892_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22892_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 33499_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33499_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31878_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31878_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21744_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21744_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 11539_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 11539_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 27271_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27271_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23235_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23235_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 16920_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 16920_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 43238_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 43238_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30436_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30436_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18423_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18423_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 36531_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 36531_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27826_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27826_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19097_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19097_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 12999_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 12999_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 42779_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 42779_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24004_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24004_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 33864_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33864_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27911_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27911_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 57661_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 57661_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21266_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21266_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 59128_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 59128_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23994_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23994_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26138_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26138_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28382_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28382_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27418_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27418_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 32520_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 32520_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27392_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27392_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23564_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23564_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26047_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26047_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 43468_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 43468_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23600_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23600_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20241_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20241_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 51816_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 51816_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26731_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26731_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 16820_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 16820_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 27114_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27114_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23614_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23614_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31915_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31915_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 33808_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33808_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26409_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26409_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22911_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22911_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29907_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29907_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31465_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31465_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23504_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23504_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 60071_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 60071_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22819_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22819_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 14298_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 14298_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25045_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 25045_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 22671_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 22671_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 17785_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 17785_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 34318_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 34318_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26004_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26004_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 14218_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 14218_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20256_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20256_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26789_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26789_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26535_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 26535_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 23189_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23189_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21318_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21318_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28702_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28702_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 58971_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 58971_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30526_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30526_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18577_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18577_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22301_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22301_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 15806_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 15806_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27546_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27546_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19512_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 19512_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 30527_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30527_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30784_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30784_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 15327_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 15327_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17065_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17065_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27510_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 27510_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 24771_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24771_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21040_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21040_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26807_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26807_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26129_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26129_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19898_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19898_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28194_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28194_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22567_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22567_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20074_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20074_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24095_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24095_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26161_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26161_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 13724_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 13724_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 22799_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22799_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21104_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21104_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31216_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31216_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26766_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26766_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 13618_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 13618_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26710_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26710_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 57216_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 57216_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20533_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20533_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21175_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21175_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 43671_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 43671_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28470_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28470_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 60468_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 60468_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 34377_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 34377_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27781_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27781_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22250_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22250_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27347_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27347_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22111_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22111_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25166_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25166_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17333_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17333_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26596_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26596_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18040_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18040_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18873_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18873_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27795_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27795_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30637_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30637_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26721_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 26721_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 08463_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 08463_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 43051_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 43051_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 13753_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 13753_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17373_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 17373_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 17732_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17732_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31358_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31358_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24507_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24507_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21330_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21330_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19546_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19546_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25401_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25401_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25869_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25869_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24166_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24166_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19118_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19118_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 57583_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 57583_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 11247_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 11247_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 43859_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 43859_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28435_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28435_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 43746_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 43746_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26312_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26312_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25266_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25266_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25209_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25209_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 58055_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 58055_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22027_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22027_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23260_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 23260_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 22245_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22245_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22743_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22743_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25923_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25923_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27530_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27530_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25297_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25297_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 13374_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 13374_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 24733_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24733_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 16225_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 16225_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 32104_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 32104_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 12150_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 12150_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24226_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24226_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 13193_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 13193_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 27921_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27921_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30136_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30136_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 42126_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 42126_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29558_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29558_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27970_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27970_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19825_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19825_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28819_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28819_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20390_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20390_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 13740_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 13740_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 59518_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 59518_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27393_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27393_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24097_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24097_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29428_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29428_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19947_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19947_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20394_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20394_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 32791_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 32791_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24751_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24751_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30297_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30297_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27692_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27692_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18328_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18328_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31865_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31865_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 33751_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33751_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26918_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26918_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 15112_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 15112_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25127_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25127_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 33645_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33645_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24546_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24546_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19065_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 19065_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 44150_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 44150_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17648_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17648_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 11580_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 11580_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22057_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22057_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20815_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20815_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24519_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24519_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 15634_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 15634_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28018_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28018_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25741_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25741_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26140_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26140_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 14528_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 14528_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28850_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28850_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21831_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21831_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18264_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18264_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30278_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30278_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 41617_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 41617_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22873_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22873_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19408_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19408_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 08830_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 08830_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 25584_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25584_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17287_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17287_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18604_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18604_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20426_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20426_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19176_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19176_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19494_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19494_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30777_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30777_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18901_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18901_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25947_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25947_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 57204_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 57204_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 15892_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 15892_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 10216_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 10216_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 15026_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 15026_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 34149_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 34149_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22493_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22493_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 35104_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 35104_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27649_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27649_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 13160_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 13160_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 15314_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 15314_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 32536_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 32536_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26059_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26059_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28278_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28278_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18402_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18402_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 14518_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 14518_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 22975_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22975_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24891_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 24891_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 27910_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27910_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23468_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23468_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18847_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18847_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27434_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27434_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 32811_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 32811_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 05315_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 05315_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 23960_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23960_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 43243_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 43243_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 42348_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 42348_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 13886_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 13886_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22482_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22482_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25178_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25178_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31146_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31146_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 51909_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 51909_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 42592_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 42592_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19180_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19180_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 55602_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 55602_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 32839_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 32839_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23729_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23729_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 14474_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 14474_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 15736_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 15736_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30015_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30015_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 32928_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 32928_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19162_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19162_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30822_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30822_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24828_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24828_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 33196_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33196_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 54688_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 54688_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19132_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19132_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29895_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29895_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 16872_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 16872_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22811_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22811_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19374_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 19374_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 27760_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27760_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26658_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26658_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24060_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24060_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 42113_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 42113_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19517_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19517_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25688_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25688_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19400_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19400_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20575_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20575_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24268_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24268_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29415_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29415_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 07070_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 07070_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 28973_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 28973_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 23404_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23404_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19742_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19742_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 35659_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 35659_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 15667_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 15667_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21961_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21961_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 07352_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 07352_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 10959_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 10959_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 23834_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23834_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24535_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24535_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23304_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23304_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18418_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18418_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25750_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25750_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28615_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28615_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20846_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20846_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31179_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31179_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18175_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18175_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25981_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25981_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28185_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28185_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22280_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22280_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25277_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25277_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17475_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17475_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 07093_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 07093_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 22100_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22100_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17396_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17396_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17543_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17543_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29254_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29254_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25388_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25388_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 16773_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 16773_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31249_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31249_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 09270_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 09270_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25791_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25791_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 57622_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 57622_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 12094_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 12094_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30749_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30749_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 12819_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 12819_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 35528_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 35528_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27462_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27462_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26694_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26694_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 55607_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 55607_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24032_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24032_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28610_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28610_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 60407_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 60407_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21535_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21535_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 16011_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 16011_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 35075_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 35075_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 42591_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 42591_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20901_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20901_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25254_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25254_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20456_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20456_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27487_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 27487_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 44377_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 44377_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 49807_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 49807_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27448_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27448_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22794_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22794_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25699_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25699_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27070_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27070_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 12357_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 12357_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17608_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17608_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18890_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18890_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25110_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25110_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30598_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30598_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23234_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23234_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30406_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30406_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 57545_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 57545_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 34693_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 34693_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27019_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27019_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 10058_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 10058_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 28428_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28428_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24003_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24003_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25402_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25402_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23415_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23415_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27828_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27828_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29458_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29458_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28195_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28195_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27859_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27859_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 59756_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 59756_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17816_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17816_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 15849_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 15849_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24254_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 24254_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 22783_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22783_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26847_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26847_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29766_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29766_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18747_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18747_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28161_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28161_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 32374_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 32374_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 16024_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 16024_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 27753_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27753_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 16695_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 16695_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26894_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26894_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27653_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27653_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 59715_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 59715_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24369_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24369_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17253_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 17253_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 17293_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17293_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 44105_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 44105_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23670_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23670_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 33246_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33246_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17733_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17733_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24583_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24583_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 44576_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 44576_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30150_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30150_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24892_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24892_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30265_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30265_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28121_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28121_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27013_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27013_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23942_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23942_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31750_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31750_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21276_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21276_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 06112_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 06112_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 31549_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31549_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28160_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28160_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28112_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28112_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21398_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21398_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17711_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17711_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25021_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25021_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28042_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28042_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28450_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28450_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26783_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26783_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28772_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 28772_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 27616_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27616_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21591_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21591_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22110_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 22110_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 25389_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25389_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 44288_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 44288_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23848_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23848_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29567_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29567_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 43754_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 43754_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30181_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30181_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 16149_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 16149_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23294_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 23294_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18912_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18912_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24615_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24615_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29886_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29886_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22784_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22784_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27513_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27513_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 14747_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 14747_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22171_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22171_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58238_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 58238_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 12019_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 12019_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24798_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24798_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24548_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24548_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23261_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23261_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 13460_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 13460_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20967_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20967_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 22679_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22679_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23052_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23052_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28578_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28578_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30276_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30276_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24085_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24085_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26891_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26891_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29463_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29463_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 32162_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 32162_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28300_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28300_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27143_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27143_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21874_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21874_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25882_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25882_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31029_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31029_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 33281_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33281_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 14220_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 14220_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 36274_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 36274_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 35759_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 35759_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31404_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31404_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 32805_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 32805_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25733_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25733_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 14566_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 14566_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 07711_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 07711_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 22845_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22845_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 11574_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 11574_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 24540_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24540_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20310_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20310_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27111_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27111_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19165_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19165_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 31412_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 31412_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24932_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24932_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26750_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26750_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23465_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23465_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25158_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25158_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 60370_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 60370_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26953_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26953_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 18193_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 18193_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24584_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24584_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20143_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 20143_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23265_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23265_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 12397_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 12397_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26858_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26858_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 58868_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 58868_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24750_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24750_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26971_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 26971_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 19725_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 19725_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 25462_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25462_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29566_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29566_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24375_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24375_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 15499_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 15499_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 07329_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 07329_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 15133_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 15133_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 25257_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25257_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 12940_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 12940_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27030_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 27030_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 28922_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28922_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 42486_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 42486_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 27312_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 27312_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30538_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30538_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 21906_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21906_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19743_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19743_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 59306_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 59306_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30643_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30643_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 33462_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33462_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 34960_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 34960_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23162_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23162_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 24224_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 24224_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 51018_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 51018_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 30461_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 30461_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 14952_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 14952_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25912_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25912_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 60337_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 60337_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29561_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29561_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 17100_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 17100_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26919_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26919_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26506_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26506_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 20413_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 20413_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 22881_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 22881_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 12566_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 12566_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 21825_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 21825_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 33204_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33204_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29930_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29930_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 25034_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25034_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 35145_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 35145_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 28102_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 28102_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 23961_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23961_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 26347_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 26347_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 19931_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 19931_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 29595_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 29595_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 33777_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33777_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33299_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 33299_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32760_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 32760_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23470_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 23470_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
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Considering the candidate 11622_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
The candidate 11622_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087 did not pass the final checks
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Considering the candidate 36497_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 36497_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44743_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 44743_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60586_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 60586_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25328_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
Preparing report for the candidate 25328_fd_Lyn-02-Q1b1x1_2026-06-07_23-19-44_20.00sec_-0.00C_LIGHTs_0087
make_report_in_HTML.sh Phase 2 (HTML assembly): 24s
make_report_in_HTML.sh TOTAL: 869s
Prepared the HTML report for the field Lyn-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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07:46:38.01 +53:27:12.3
07:48:12.81 +53:28:36.0
08:22:26.66 +53:32:01.4
07:46:20.22 +53:26:35.0
08:24:00.01 +53:29:07.2
08:25:03.71 +53:28:32.5
08:24:38.04 +53:27:22.1
07:47:19.74 +53:23:26.8
08:25:50.51 +53:25:39.8
07:48:00.97 +53:23:03.7
08:31:24.58 +53:21:19.4
08:23:49.90 +53:22:50.8
07:47:19.19 +53:17:11.6
07:49:09.67 +53:17:30.8
07:46:26.89 +53:12:40.4
07:50:57.44 +53:13:44.6
07:50:20.44 +53:11:57.7
07:46:56.91 +53:09:44.8
07:48:40.33 +53:10:16.0
07:47:51.84 +53:06:16.7
07:50:26.70 +53:06:24.0
07:49:53.36 +53:05:26.1
07:48:35.73 +52:59:32.6
07:49:12.58 +52:57:39.1
07:51:21.45 +52:58:24.8
07:56:24.25 +51:18:20.8
07:53:35.42 +52:02:03.4
07:50:53.27 +52:02:00.8
07:53:52.09 +52:21:54.6
07:53:37.95 +52:35:22.3
08:27:13.12 +52:34:44.1
07:50:14.95 +52:35:55.8
08:31:04.65 +52:33:39.0
08:30:35.78 +52:40:01.8
08:29:58.98 +52:39:36.2
08:29:30.29 +52:42:36.3
08:26:10.66 +52:46:37.9
08:28:55.29 +52:46:49.2
07:49:35.56 +52:46:57.8
08:25:06.57 +52:50:43.1
07:50:12.59 +52:50:49.4
07:48:53.14 +52:51:05.1
07:50:10.27 +52:52:47.8
08:30:03.09 +52:51:45.9
07:48:07.62 +52:54:29.8
07:49:09.01 +52:56:11.4
08:29:06.02 +50:27:08.2
08:27:56.28 +50:40:42.4
08:29:35.69 +50:46:26.4
08:30:26.59 +50:48:42.7
08:30:15.42 +51:18:45.9
07:57:21.96 +51:38:20.2
08:30:07.81 +51:31:28.6
07:54:46.95 +51:55:10.4
07:52:37.90 +51:53:24.3
07:55:24.96 +51:59:57.6
07:52:50.93 +51:56:21.6
07:55:01.80 +51:57:11.9
08:28:16.57 +51:54:40.2
07:51:47.99 +52:02:46.5
08:29:00.74 +51:59:48.2
07:53:10.49 +52:11:45.9
07:53:59.56 +52:13:15.1
07:55:04.71 +52:15:16.7
08:29:53.95 +52:11:45.2
07:51:42.67 +52:18:52.1
08:26:08.55 +52:18:31.3
07:51:07.20 +52:19:45.7
08:29:11.10 +52:20:44.7
07:50:03.77 +52:27:27.8
08:27:23.91 +52:26:37.0
07:52:57.47 +52:27:42.3
08:28:27.72 +52:26:36.5
08:31:03.57 +52:28:11.3
########### Completed Lyn-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 ####
07:41:29.79 +54:55:00.1
08:24:00.81 +54:08:22.1
08:23:32.17 +54:14:46.8
07:40:04.76 +55:03:36.6
08:25:03.71 +53:28:32.5
08:23:51.64 +53:44:49.9
07:37:29.78 +55:13:06.1
08:25:57.72 +54:29:22.2
07:40:03.23 +55:00:00.4
08:30:35.78 +52:40:01.8
08:16:57.81 +54:01:28.8
07:39:09.96 +55:47:49.8
07:51:21.45 +52:58:24.8
08:20:41.34 +54:24:53.0
08:21:40.12 +55:53:12.0
07:36:41.06 +56:41:14.3
08:31:04.65 +52:33:39.0
07:39:54.67 +54:51:50.3
08:31:24.58 +53:21:19.4
07:41:53.68 +54:15:59.6
08:28:16.57 +51:54:40.2
07:36:02.19 +55:16:12.9
07:55:04.71 +52:15:16.7
08:21:35.05 +55:03:26.9
07:38:13.63 +54:29:54.6
07:46:09.06 +54:14:31.2
08:17:35.39 +54:31:08.8
07:43:51.41 +53:32:09.1
08:19:35.98 +54:30:32.0
07:39:48.96 +54:56:12.8
08:21:50.21 +54:43:16.5
08:29:30.29 +52:42:36.3
08:20:42.39 +55:07:06.1
07:37:35.52 +55:27:56.4
08:29:35.69 +50:46:26.4
07:45:41.00 +54:29:58.7
08:18:11.02 +54:33:37.0
08:23:40.48 +55:06:30.6
07:44:51.57 +53:39:04.0
07:48:00.97 +53:23:03.7
07:38:37.01 +54:28:01.6
08:22:20.43 +55:13:53.6
08:22:09.31 +54:05:44.2
08:20:47.18 +53:50:31.3
08:24:43.36 +55:07:09.6
08:29:11.10 +52:20:44.7
08:21:05.41 +55:15:28.2
07:35:06.39 +56:25:49.4
07:47:19.19 +53:17:11.6
08:23:32.85 +54:43:15.6
07:36:53.55 +56:28:46.4
07:41:15.81 +55:31:02.6
08:20:32.05 +54:36:18.0
08:22:11.83 +55:10:59.1
07:38:52.63 +55:18:01.4
07:43:11.97 +54:08:56.3
07:53:59.56 +52:13:15.1
08:23:25.31 +53:58:35.1
07:38:33.04 +55:46:12.3
07:38:43.19 +55:08:18.5
07:36:15.61 +56:11:10.5
08:23:35.28 +54:26:58.8
07:46:24.07 +53:53:07.4
07:44:50.85 +53:49:29.2
07:35:55.33 +56:16:01.8
07:37:56.12 +56:00:26.4
08:21:56.67 +54:55:13.9
08:24:18.65 +55:32:22.0
08:20:25.65 +54:36:08.0
07:40:37.52 +54:31:57.3
07:37:37.69 +55:30:54.0
08:19:52.27 +54:23:11.1
07:36:16.56 +55:02:53.2
07:38:49.79 +55:30:13.0
07:36:19.16 +54:47:41.2
08:20:23.52 +54:43:10.0
08:22:32.72 +55:14:19.4
07:42:57.85 +55:23:49.5
08:25:21.22 +53:50:55.1
07:41:55.54 +54:26:56.1
07:37:29.05 +56:35:29.5
08:23:00.37 +54:36:02.2
07:52:37.90 +51:53:24.3
08:23:47.35 +55:37:40.6
07:41:11.23 +55:21:33.9
08:26:10.66 +52:46:37.9
08:21:44.81 +54:19:59.5
08:28:27.72 +52:26:36.5
07:49:09.67 +53:17:30.8
08:22:09.54 +54:25:50.2
07:39:58.65 +55:09:48.5
08:17:35.36 +54:32:08.6
07:38:05.50 +55:09:25.6
07:39:06.38 +54:40:18.3
07:38:06.68 +55:57:53.4
08:21:46.32 +54:37:10.4
08:22:25.51 +56:03:00.2
07:36:55.95 +55:41:28.8
08:19:57.25 +54:26:07.0
07:45:12.60 +53:51:05.8
07:36:02.24 +56:32:40.2
07:39:16.74 +55:55:09.1
07:48:52.53 +53:47:11.8
07:39:17.77 +54:46:55.1
08:23:28.28 +55:29:36.3
07:40:01.35 +55:37:17.0
08:22:07.97 +54:49:05.8
08:22:53.87 +54:43:53.5
07:37:06.18 +54:48:15.3
07:35:54.03 +55:37:17.7
07:52:50.93 +51:56:21.6
07:36:14.89 +56:59:44.3
08:25:06.57 +52:50:43.1
07:42:06.78 +54:10:48.9
08:28:55.29 +52:46:49.2
07:38:50.12 +54:28:35.1
08:18:25.59 +54:52:09.2
08:21:09.51 +54:52:49.0
07:51:47.99 +52:02:46.5
08:20:13.16 +55:24:10.1
08:23:06.53 +55:21:06.2
08:21:34.56 +55:16:32.5
07:40:58.34 +54:34:29.0
07:43:37.81 +54:20:34.7
08:20:31.20 +54:51:57.2
07:39:35.36 +54:45:36.3
07:37:07.12 +56:08:12.9
08:21:52.15 +53:44:08.1
07:34:47.64 +56:48:18.1
07:40:28.25 +54:50:55.9
07:42:17.58 +54:16:12.4
07:42:49.87 +53:55:21.5
07:50:53.27 +52:02:00.8
07:44:18.63 +54:02:10.9
08:20:20.60 +54:25:09.5
08:22:40.17 +55:45:09.4
08:18:00.44 +54:14:37.9
07:36:42.06 +55:25:31.8
07:35:57.44 +56:32:21.2
07:51:42.67 +52:18:52.1
08:25:25.27 +54:28:25.1
07:41:58.99 +54:53:17.2
08:21:31.30 +54:10:09.5
08:23:14.65 +55:43:12.6
08:24:03.76 +55:39:09.9
07:46:32.64 +53:32:12.8
08:23:03.29 +54:55:55.7
08:23:07.38 +54:01:29.0
07:37:24.57 +54:13:19.4
07:39:38.17 +55:48:47.4
08:22:02.47 +53:46:30.7
07:47:19.74 +53:23:26.8
07:46:14.97 +54:29:08.2
07:35:36.22 +56:18:23.6
08:18:40.44 +54:53:54.8
08:24:38.04 +53:27:22.1
08:22:37.10 +54:57:33.1
07:48:53.14 +52:51:05.1
07:36:54.13 +55:53:12.8
07:34:37.63 +56:53:42.1
08:22:26.98 +55:21:55.0
08:21:49.94 +55:34:36.4
07:38:41.65 +54:45:44.0
07:38:42.35 +56:15:56.9
07:41:51.68 +54:14:53.6
07:42:36.30 +54:37:51.7
08:24:30.55 +54:40:25.7
07:35:07.53 +56:24:08.6
07:41:50.86 +54:06:49.1
07:39:48.71 +55:13:56.6
07:38:05.39 +55:48:16.8
07:45:45.34 +53:56:15.1
07:56:24.25 +51:18:20.8
08:22:18.69 +55:14:58.2
08:22:19.19 +55:49:25.3
08:22:57.08 +54:47:31.3
07:37:55.92 +55:58:52.9
07:36:26.43 +55:43:01.1
07:38:27.15 +55:26:21.1
07:40:06.52 +55:41:14.5
08:24:04.86 +55:47:30.2
07:41:36.53 +53:47:29.7
07:37:14.26 +55:41:09.7
07:39:43.97 +54:33:22.6
07:54:46.95 +51:55:10.4
07:34:56.89 +57:09:27.7
08:23:49.90 +53:22:50.8
07:41:45.73 +55:08:48.5
07:46:56.91 +53:09:44.8
07:41:27.42 +54:17:45.6
07:35:06.70 +56:38:01.5
08:23:37.39 +53:38:58.1
08:22:59.77 +54:42:06.7
07:45:48.55 +54:15:16.3
07:38:10.52 +55:46:39.3
07:36:35.60 +54:58:12.0
07:46:43.83 +54:19:28.3
08:25:06.82 +55:07:08.6
07:37:02.14 +55:41:37.4
08:20:29.59 +54:29:58.5
08:22:47.67 +53:36:29.4
07:44:28.28 +54:56:12.7
08:29:58.98 +52:39:36.2
07:53:52.09 +52:21:54.6
07:36:52.27 +56:32:22.5
07:40:21.75 +55:07:44.6
07:43:47.07 +54:44:17.4
07:43:25.33 +53:45:35.5
08:30:26.59 +50:48:42.7
07:50:14.95 +52:35:55.8
08:21:17.65 +55:52:24.3
07:57:21.96 +51:38:20.2
07:48:20.02 +53:32:46.9
07:43:16.14 +54:57:39.5
07:35:59.53 +56:25:04.9
07:36:46.02 +56:13:11.0
07:42:20.10 +53:55:41.9
07:46:00.03 +53:30:06.5
08:21:29.96 +55:52:09.2
08:22:47.63 +53:55:31.4
08:25:07.47 +54:53:40.7
07:45:23.81 +53:26:10.0
08:30:15.42 +51:18:45.9
07:36:46.57 +55:38:36.3
07:42:24.01 +53:56:43.2
08:22:29.37 +56:15:05.1
08:19:32.42 +55:15:19.1
08:18:10.08 +54:27:07.2
07:44:18.47 +54:30:05.6
08:23:19.57 +55:02:07.5
07:53:35.42 +52:02:03.4
08:21:57.74 +55:47:38.9
07:44:13.32 +54:39:52.6
08:23:36.29 +55:44:19.2
07:37:12.32 +55:23:32.6
08:23:24.65 +54:58:57.1
08:20:39.80 +54:09:46.5
08:21:26.25 +55:09:16.6
07:36:03.84 +55:31:10.8
07:50:26.70 +53:06:24.0
07:39:04.20 +56:15:54.4
07:41:29.74 +55:14:29.8
07:33:43.17 +57:39:46.0
08:20:21.71 +55:04:59.9
07:42:38.37 +54:49:25.3
07:36:08.84 +54:55:50.8
08:21:03.10 +56:00:39.6
08:21:35.81 +54:46:36.6
08:22:08.53 +54:17:21.7
07:39:17.70 +55:23:16.0
07:48:08.25 +53:48:43.9
07:39:21.84 +55:50:02.9
07:41:03.34 +54:33:56.2
08:17:42.27 +54:23:25.7
07:43:27.24 +55:12:08.2
07:40:04.45 +54:40:36.9
07:35:50.66 +55:51:21.7
08:24:24.22 +55:21:18.2
07:35:13.81 +55:53:47.1
08:22:01.99 +56:08:09.4
07:43:27.66 +54:04:31.3
08:23:39.92 +54:46:40.2
07:37:36.07 +56:03:44.1
07:43:24.84 +53:44:53.4
07:34:16.59 +57:19:06.4
07:38:20.12 +54:33:14.5
07:55:01.80 +51:57:11.9
07:35:35.48 +56:49:28.6
07:48:18.46 +53:53:11.7
07:34:41.23 +56:39:58.6
07:47:51.84 +53:06:16.7
08:22:29.44 +54:29:24.4
08:21:04.81 +54:37:13.0
08:30:07.81 +51:31:28.6
07:39:26.57 +54:51:37.2
08:18:35.58 +54:19:26.4
07:52:57.47 +52:27:42.3
07:39:14.89 +55:16:20.8
07:37:46.20 +56:11:21.2
07:50:20.44 +53:11:57.7
08:27:13.12 +52:34:44.1
08:22:10.59 +55:34:38.0
08:22:52.05 +54:50:30.2
08:24:07.27 +55:38:10.7
08:30:03.09 +52:51:45.9
08:29:06.02 +50:27:08.2
08:19:46.18 +54:30:16.5
08:19:50.90 +55:16:23.2
07:39:03.82 +54:35:34.8
08:23:40.68 +54:32:47.6
07:34:49.31 +56:46:00.1
07:38:27.23 +55:55:44.3
08:21:28.35 +55:55:30.5
07:41:40.62 +54:43:25.3
08:23:01.42 +53:58:13.5
07:43:55.30 +55:02:42.7
08:25:10.76 +53:58:41.6
07:55:24.96 +51:59:57.6
07:46:26.89 +53:12:40.4
08:21:15.19 +54:33:43.7
08:22:36.28 +54:19:34.6
07:39:26.44 +54:52:11.4
08:20:44.12 +54:50:49.5
07:38:11.55 +54:56:55.7
08:19:18.59 +54:26:52.2
07:43:21.52 +54:02:15.9
08:25:15.13 +54:20:44.1
08:22:50.92 +54:25:04.6
07:51:07.20 +52:19:45.7
08:22:40.52 +56:06:17.7
07:37:30.68 +56:12:49.8
08:24:57.97 +55:14:32.0
08:22:34.71 +54:35:25.5
07:45:33.34 +54:01:06.8
08:23:32.26 +55:55:42.3
07:42:09.60 +54:13:47.9
07:44:38.90 +53:34:46.4
08:20:22.08 +54:27:04.1
07:36:14.73 +56:02:36.2
08:22:49.24 +54:34:15.5
07:37:35.89 +54:14:28.7
08:26:08.55 +52:18:31.3
08:18:53.48 +55:00:48.8
07:36:10.39 +55:55:50.5
07:50:12.59 +52:50:49.4
07:37:04.40 +54:52:40.1
07:48:12.81 +53:28:36.0
07:37:58.07 +55:54:11.3
07:37:01.75 +54:44:06.1
07:48:07.62 +52:54:29.8
08:23:38.69 +54:02:34.5
07:43:48.01 +54:47:39.5
07:46:19.67 +53:56:13.3
08:19:29.06 +54:23:31.3
07:40:58.31 +54:23:59.2
08:19:02.89 +55:03:45.0
08:22:47.07 +53:46:45.6
07:38:01.34 +55:17:50.6
08:23:26.79 +53:48:34.0
07:41:25.85 +54:13:11.0
07:37:32.36 +54:09:45.7
07:40:36.19 +55:18:33.5
07:38:02.61 +55:53:42.3
08:19:33.42 +54:53:34.6
08:19:25.81 +54:23:56.9
08:24:38.92 +54:18:14.7
08:23:53.47 +54:35:02.7
07:38:29.72 +54:15:26.6
07:36:43.96 +55:13:09.0
07:39:51.24 +54:38:15.0
07:50:10.27 +52:52:47.8
08:22:31.19 +55:03:51.3
07:44:22.96 +54:01:23.9
07:49:35.56 +52:46:57.8
08:21:06.79 +54:02:48.9
07:37:26.97 +56:09:51.9
07:38:53.07 +55:42:39.7
07:39:10.36 +54:45:52.7
08:24:26.80 +54:03:54.0
07:38:04.77 +55:03:01.7
08:23:42.64 +54:28:03.8
07:35:28.16 +56:19:03.1
07:38:46.84 +55:09:13.2
08:29:00.74 +51:59:48.2
07:35:37.12 +56:50:12.9
07:44:39.02 +54:49:01.2
07:39:33.19 +54:46:50.8
07:39:44.46 +54:59:44.5
07:35:32.80 +56:35:01.5
07:35:50.19 +55:18:14.2
07:38:39.15 +55:04:11.9
07:40:55.12 +55:03:00.8
08:22:37.49 +54:18:22.1
07:45:26.17 +53:55:16.8
07:40:35.14 +54:52:08.2
07:44:21.86 +54:27:42.3
08:18:43.13 +54:11:04.4
07:47:48.82 +53:39:22.0
07:41:00.69 +54:10:29.6
07:37:48.24 +54:19:24.4
08:23:36.19 +55:24:14.5
07:38:18.66 +54:32:43.9
07:44:05.45 +53:47:06.7
08:22:26.66 +53:32:01.4
07:48:35.73 +52:59:32.6
07:49:53.36 +53:05:26.1
07:45:59.28 +53:44:56.4
08:22:55.28 +53:36:27.3
08:23:40.92 +54:46:16.5
07:36:22.29 +56:24:37.3
08:22:49.52 +55:15:05.6
08:22:13.07 +54:58:34.6
07:37:53.68 +55:27:34.6
07:43:01.13 +54:24:35.6
07:39:52.30 +55:41:14.5
07:45:22.97 +53:44:34.4
07:40:54.44 +54:44:27.3
08:21:35.48 +54:36:01.3
07:43:18.92 +55:00:17.6
08:18:15.86 +54:52:42.3
08:27:23.91 +52:26:37.0
08:21:08.91 +54:34:15.1
07:35:20.98 +55:46:23.8
07:37:35.63 +54:44:12.2
08:22:47.67 +55:41:20.1
07:37:48.36 +54:57:19.2
07:34:31.07 +56:44:46.8
07:41:15.74 +54:25:12.5
07:53:10.49 +52:11:45.9
08:20:05.67 +54:56:32.2
08:22:45.55 +54:48:16.4
08:18:00.98 +54:09:28.7
07:39:04.24 +54:47:15.5
07:36:59.57 +56:15:00.8
08:21:58.92 +54:51:27.6
07:35:52.42 +56:41:08.9
08:20:39.37 +54:15:45.2
07:53:37.95 +52:35:22.3
07:41:20.66 +54:21:52.3
07:44:41.74 +53:52:22.7
07:39:04.30 +55:12:49.1
07:40:50.18 +55:35:46.9
08:29:53.95 +52:11:45.2
07:43:47.59 +53:50:56.9
08:24:00.01 +53:29:07.2
07:50:57.44 +53:13:44.6
07:39:41.30 +55:00:42.1
07:39:08.76 +54:49:25.6
08:27:56.28 +50:40:42.4
07:42:24.42 +53:51:11.6
07:35:55.79 +56:20:54.4
07:41:45.24 +54:35:30.2
07:50:03.77 +52:27:27.8
08:23:04.26 +54:08:51.7
08:23:26.01 +56:13:04.6
08:24:10.77 +54:33:44.8
08:21:21.61 +54:39:08.7
07:42:15.94 +55:05:09.1
08:24:36.23 +55:23:44.8
07:46:38.01 +53:27:12.3
07:42:32.80 +53:57:04.7
07:44:07.41 +54:46:12.7
07:48:40.33 +53:10:16.0
08:25:03.30 +54:21:28.6
07:41:49.86 +54:54:21.4
07:43:23.87 +54:32:38.3
07:39:43.66 +55:32:36.0
08:20:01.93 +54:08:55.3
08:25:50.51 +53:25:39.8
07:46:20.22 +53:26:35.0
08:25:40.78 +53:36:12.7
07:39:34.92 +54:57:16.6
07:49:12.58 +52:57:39.1
07:49:09.01 +52:56:11.4
08:31:03.57 +52:28:11.3
08:21:01.17 +54:50:26.5
###################################################################################
07:41:29.79 +54:55:00.1 -- not an asteroid (will add it to exclusion list)
08:24:00.81 +54:08:22.1 -- not an asteroid (will add it to exclusion list)
08:23:32.17 +54:14:46.8 -- not an asteroid (will add it to exclusion list)
07:40:04.76 +55:03:36.6 -- not an asteroid (will add it to exclusion list)
08:25:03.71 +53:28:32.5 -- not an asteroid (will add it to exclusion list)
08:23:51.64 +53:44:49.9 -- not an asteroid (will add it to exclusion list)
07:37:29.78 +55:13:06.1 -- not an asteroid (will add it to exclusion list)
08:25:57.72 +54:29:22.2 -- not an asteroid (will add it to exclusion list)
07:40:03.23 +55:00:00.4 -- not an asteroid (will add it to exclusion list)
08:30:35.78 +52:40:01.8 -- not an asteroid (will add it to exclusion list)
08:16:57.81 +54:01:28.8 -- not an asteroid (will add it to exclusion list)
07:39:09.96 +55:47:49.8 -- not an asteroid (will add it to exclusion list)
07:51:21.45 +52:58:24.8 -- not an asteroid (will add it to exclusion list)
08:20:41.34 +54:24:53.0 -- not an asteroid (will add it to exclusion list)
08:21:40.12 +55:53:12.0 -- not an asteroid (will add it to exclusion list)
07:36:41.06 +56:41:14.3 -- not an asteroid (will add it to exclusion list)
08:31:04.65 +52:33:39.0 -- not an asteroid (will add it to exclusion list)
07:39:54.67 +54:51:50.3 -- not an asteroid (will add it to exclusion list)
08:31:24.58 +53:21:19.4 -- not an asteroid (will add it to exclusion list)
07:41:53.68 +54:15:59.6 -- not an asteroid (will add it to exclusion list)
08:28:16.57 +51:54:40.2 -- not an asteroid (will add it to exclusion list)
07:36:02.19 +55:16:12.9 -- not an asteroid (will add it to exclusion list)
07:55:04.71 +52:15:16.7 -- not an asteroid (will add it to exclusion list)
08:21:35.05 +55:03:26.9 -- not an asteroid (will add it to exclusion list)
07:38:13.63 +54:29:54.6 -- not an asteroid (will add it to exclusion list)
07:46:09.06 +54:14:31.2 -- not an asteroid (will add it to exclusion list)
08:17:35.39 +54:31:08.8 -- not an asteroid (will add it to exclusion list)
07:43:51.41 +53:32:09.1 -- not an asteroid (will add it to exclusion list)
08:19:35.98 +54:30:32.0 -- not an asteroid (will add it to exclusion list)
07:39:48.96 +54:56:12.8 -- not an asteroid (will add it to exclusion list)
08:21:50.21 +54:43:16.5 -- not an asteroid (will add it to exclusion list)
08:29:30.29 +52:42:36.3 -- not an asteroid (will add it to exclusion list)
08:20:42.39 +55:07:06.1 -- not an asteroid (will add it to exclusion list)
07:37:35.52 +55:27:56.4 -- not an asteroid (will add it to exclusion list)
08:29:35.69 +50:46:26.4 -- not an asteroid (will add it to exclusion list)
07:45:41.00 +54:29:58.7 -- not an asteroid (will add it to exclusion list)
08:18:11.02 +54:33:37.0 -- not an asteroid (will add it to exclusion list)
08:23:40.48 +55:06:30.6 -- not an asteroid (will add it to exclusion list)
07:44:51.57 +53:39:04.0 -- not an asteroid (will add it to exclusion list)
07:48:00.97 +53:23:03.7 -- not an asteroid (will add it to exclusion list)
07:38:37.01 +54:28:01.6 -- not an asteroid (will add it to exclusion list)
08:22:20.43 +55:13:53.6 -- not an asteroid (will add it to exclusion list)
08:22:09.31 +54:05:44.2 -- not an asteroid (will add it to exclusion list)
08:20:47.18 +53:50:31.3 -- not an asteroid (will add it to exclusion list)
08:24:43.36 +55:07:09.6 -- not an asteroid (will add it to exclusion list)
08:29:11.10 +52:20:44.7 -- not an asteroid (will add it to exclusion list)
08:21:05.41 +55:15:28.2 -- not an asteroid (will add it to exclusion list)
07:35:06.39 +56:25:49.4 -- not an asteroid (will add it to exclusion list)
07:47:19.19 +53:17:11.6 -- not an asteroid (will add it to exclusion list)
08:23:32.85 +54:43:15.6 -- not an asteroid (will add it to exclusion list)
07:36:53.55 +56:28:46.4 -- not an asteroid (will add it to exclusion list)
07:41:15.81 +55:31:02.6 -- not an asteroid (will add it to exclusion list)
08:20:32.05 +54:36:18.0 -- not an asteroid (will add it to exclusion list)
08:22:11.83 +55:10:59.1 -- not an asteroid (will add it to exclusion list)
07:38:52.63 +55:18:01.4 -- not an asteroid (will add it to exclusion list)
07:43:11.97 +54:08:56.3 -- not an asteroid (will add it to exclusion list)
07:53:59.56 +52:13:15.1 -- not an asteroid (will add it to exclusion list)
08:23:25.31 +53:58:35.1 -- not an asteroid (will add it to exclusion list)
07:38:33.04 +55:46:12.3 -- not an asteroid (will add it to exclusion list)
07:38:43.19 +55:08:18.5 -- not an asteroid (will add it to exclusion list)
07:36:15.61 +56:11:10.5 -- not an asteroid (will add it to exclusion list)
08:23:35.28 +54:26:58.8 -- not an asteroid (will add it to exclusion list)
07:46:24.07 +53:53:07.4 -- not an asteroid (will add it to exclusion list)
07:44:50.85 +53:49:29.2 -- not an asteroid (will add it to exclusion list)
07:35:55.33 +56:16:01.8 -- not an asteroid (will add it to exclusion list)
07:37:56.12 +56:00:26.4 -- not an asteroid (will add it to exclusion list)
08:21:56.67 +54:55:13.9 -- not an asteroid (will add it to exclusion list)
08:24:18.65 +55:32:22.0 -- not an asteroid (will add it to exclusion list)
08:20:25.65 +54:36:08.0 -- not an asteroid (will add it to exclusion list)
07:40:37.52 +54:31:57.3 -- not an asteroid (will add it to exclusion list)
07:37:37.69 +55:30:54.0 -- not an asteroid (will add it to exclusion list)
08:19:52.27 +54:23:11.1 -- not an asteroid (will add it to exclusion list)
07:36:16.56 +55:02:53.2 -- not an asteroid (will add it to exclusion list)
07:38:49.79 +55:30:13.0 -- not an asteroid (will add it to exclusion list)
07:36:19.16 +54:47:41.2 -- not an asteroid (will add it to exclusion list)
08:20:23.52 +54:43:10.0 -- not an asteroid (will add it to exclusion list)
08:22:32.72 +55:14:19.4 -- not an asteroid (will add it to exclusion list)
07:42:57.85 +55:23:49.5 -- not an asteroid (will add it to exclusion list)
08:25:21.22 +53:50:55.1 -- not an asteroid (will add it to exclusion list)
07:41:55.54 +54:26:56.1 -- not an asteroid (will add it to exclusion list)
07:37:29.05 +56:35:29.5 -- not an asteroid (will add it to exclusion list)
08:23:00.37 +54:36:02.2 -- not an asteroid (will add it to exclusion list)
07:52:37.90 +51:53:24.3 -- not an asteroid (will add it to exclusion list)
08:23:47.35 +55:37:40.6 -- not an asteroid (will add it to exclusion list)
07:41:11.23 +55:21:33.9 -- not an asteroid (will add it to exclusion list)
08:26:10.66 +52:46:37.9 -- not an asteroid (will add it to exclusion list)
08:21:44.81 +54:19:59.5 -- not an asteroid (will add it to exclusion list)
08:28:27.72 +52:26:36.5 -- not an asteroid (will add it to exclusion list)
07:49:09.67 +53:17:30.8 -- not an asteroid (will add it to exclusion list)
08:22:09.54 +54:25:50.2 -- not an asteroid (will add it to exclusion list)
07:39:58.65 +55:09:48.5 -- not an asteroid (will add it to exclusion list)
08:17:35.36 +54:32:08.6 -- not an asteroid (will add it to exclusion list)
07:38:05.50 +55:09:25.6 -- not an asteroid (will add it to exclusion list)
07:39:06.38 +54:40:18.3 -- not an asteroid (will add it to exclusion list)
07:38:06.68 +55:57:53.4 -- not an asteroid (will add it to exclusion list)
08:21:46.32 +54:37:10.4 -- not an asteroid (will add it to exclusion list)
08:22:25.51 +56:03:00.2 -- not an asteroid (will add it to exclusion list)
07:36:55.95 +55:41:28.8 -- not an asteroid (will add it to exclusion list)
08:19:57.25 +54:26:07.0 -- not an asteroid (will add it to exclusion list)
07:45:12.60 +53:51:05.8 -- not an asteroid (will add it to exclusion list)
07:36:02.24 +56:32:40.2 -- not an asteroid (will add it to exclusion list)
07:39:16.74 +55:55:09.1 -- not an asteroid (will add it to exclusion list)
07:48:52.53 +53:47:11.8 -- not an asteroid (will add it to exclusion list)
07:39:17.77 +54:46:55.1 -- not an asteroid (will add it to exclusion list)
08:23:28.28 +55:29:36.3 -- not an asteroid (will add it to exclusion list)
07:40:01.35 +55:37:17.0 -- not an asteroid (will add it to exclusion list)
08:22:07.97 +54:49:05.8 -- not an asteroid (will add it to exclusion list)
08:22:53.87 +54:43:53.5 -- not an asteroid (will add it to exclusion list)
07:37:06.18 +54:48:15.3 -- not an asteroid (will add it to exclusion list)
07:35:54.03 +55:37:17.7 -- not an asteroid (will add it to exclusion list)
07:52:50.93 +51:56:21.6 -- not an asteroid (will add it to exclusion list)
07:36:14.89 +56:59:44.3 -- not an asteroid (will add it to exclusion list)
08:25:06.57 +52:50:43.1 -- not an asteroid (will add it to exclusion list)
07:42:06.78 +54:10:48.9 -- not an asteroid (will add it to exclusion list)
08:28:55.29 +52:46:49.2 -- not an asteroid (will add it to exclusion list)
07:38:50.12 +54:28:35.1 -- not an asteroid (will add it to exclusion list)
08:18:25.59 +54:52:09.2 -- not an asteroid (will add it to exclusion list)
08:21:09.51 +54:52:49.0 -- not an asteroid (will add it to exclusion list)
07:51:47.99 +52:02:46.5 -- not an asteroid (will add it to exclusion list)
08:20:13.16 +55:24:10.1 -- not an asteroid (will add it to exclusion list)
08:23:06.53 +55:21:06.2 -- not an asteroid (will add it to exclusion list)
08:21:34.56 +55:16:32.5 -- not an asteroid (will add it to exclusion list)
07:40:58.34 +54:34:29.0 -- not an asteroid (will add it to exclusion list)
07:43:37.81 +54:20:34.7 -- not an asteroid (will add it to exclusion list)
08:20:31.20 +54:51:57.2 -- not an asteroid (will add it to exclusion list)
07:39:35.36 +54:45:36.3 -- not an asteroid (will add it to exclusion list)
07:37:07.12 +56:08:12.9 -- not an asteroid (will add it to exclusion list)
08:21:52.15 +53:44:08.1 -- not an asteroid (will add it to exclusion list)
07:34:47.64 +56:48:18.1 -- not an asteroid (will add it to exclusion list)
07:40:28.25 +54:50:55.9 -- not an asteroid (will add it to exclusion list)
07:42:17.58 +54:16:12.4 -- not an asteroid (will add it to exclusion list)
07:42:49.87 +53:55:21.5 -- not an asteroid (will add it to exclusion list)
07:50:53.27 +52:02:00.8 -- not an asteroid (will add it to exclusion list)
07:44:18.63 +54:02:10.9 -- not an asteroid (will add it to exclusion list)
08:20:20.60 +54:25:09.5 -- not an asteroid (will add it to exclusion list)
08:22:40.17 +55:45:09.4 -- not an asteroid (will add it to exclusion list)
08:18:00.44 +54:14:37.9 -- not an asteroid (will add it to exclusion list)
07:36:42.06 +55:25:31.8 -- not an asteroid (will add it to exclusion list)
07:35:57.44 +56:32:21.2 -- not an asteroid (will add it to exclusion list)
07:51:42.67 +52:18:52.1 -- not an asteroid (will add it to exclusion list)
08:25:25.27 +54:28:25.1 -- not an asteroid (will add it to exclusion list)
07:41:58.99 +54:53:17.2 -- not an asteroid (will add it to exclusion list)
08:21:31.30 +54:10:09.5 -- not an asteroid (will add it to exclusion list)
08:23:14.65 +55:43:12.6 -- not an asteroid (will add it to exclusion list)
08:24:03.76 +55:39:09.9 -- not an asteroid (will add it to exclusion list)
07:46:32.64 +53:32:12.8 -- not an asteroid (will add it to exclusion list)
08:23:03.29 +54:55:55.7 -- not an asteroid (will add it to exclusion list)
08:23:07.38 +54:01:29.0 -- not an asteroid (will add it to exclusion list)
07:37:24.57 +54:13:19.4 -- not an asteroid (will add it to exclusion list)
07:39:38.17 +55:48:47.4 -- not an asteroid (will add it to exclusion list)
08:22:02.47 +53:46:30.7 -- not an asteroid (will add it to exclusion list)
07:47:19.74 +53:23:26.8 -- not an asteroid (will add it to exclusion list)
07:46:14.97 +54:29:08.2 -- not an asteroid (will add it to exclusion list)
07:35:36.22 +56:18:23.6 -- not an asteroid (will add it to exclusion list)
08:18:40.44 +54:53:54.8 -- not an asteroid (will add it to exclusion list)
08:24:38.04 +53:27:22.1 -- not an asteroid (will add it to exclusion list)
08:22:37.10 +54:57:33.1 -- not an asteroid (will add it to exclusion list)
07:48:53.14 +52:51:05.1 -- not an asteroid (will add it to exclusion list)
07:36:54.13 +55:53:12.8 -- not an asteroid (will add it to exclusion list)
07:34:37.63 +56:53:42.1 -- not an asteroid (will add it to exclusion list)
08:22:26.98 +55:21:55.0 -- not an asteroid (will add it to exclusion list)
08:21:49.94 +55:34:36.4 -- not an asteroid (will add it to exclusion list)
07:38:41.65 +54:45:44.0 -- not an asteroid (will add it to exclusion list)
07:38:42.35 +56:15:56.9 -- not an asteroid (will add it to exclusion list)
07:41:51.68 +54:14:53.6 -- not an asteroid (will add it to exclusion list)
07:42:36.30 +54:37:51.7 -- not an asteroid (will add it to exclusion list)
08:24:30.55 +54:40:25.7 -- not an asteroid (will add it to exclusion list)
07:35:07.53 +56:24:08.6 -- not an asteroid (will add it to exclusion list)
07:41:50.86 +54:06:49.1 -- not an asteroid (will add it to exclusion list)
07:39:48.71 +55:13:56.6 -- not an asteroid (will add it to exclusion list)
07:38:05.39 +55:48:16.8 -- not an asteroid (will add it to exclusion list)
07:45:45.34 +53:56:15.1 -- not an asteroid (will add it to exclusion list)
07:56:24.25 +51:18:20.8 -- not an asteroid (will add it to exclusion list)
08:22:18.69 +55:14:58.2 -- not an asteroid (will add it to exclusion list)
08:22:19.19 +55:49:25.3 -- not an asteroid (will add it to exclusion list)
08:22:57.08 +54:47:31.3 -- not an asteroid (will add it to exclusion list)
07:37:55.92 +55:58:52.9 -- not an asteroid (will add it to exclusion list)
07:36:26.43 +55:43:01.1 -- not an asteroid (will add it to exclusion list)
07:38:27.15 +55:26:21.1 -- not an asteroid (will add it to exclusion list)
07:40:06.52 +55:41:14.5 -- not an asteroid (will add it to exclusion list)
08:24:04.86 +55:47:30.2 -- not an asteroid (will add it to exclusion list)
07:41:36.53 +53:47:29.7 -- not an asteroid (will add it to exclusion list)
07:37:14.26 +55:41:09.7 -- not an asteroid (will add it to exclusion list)
07:39:43.97 +54:33:22.6 -- not an asteroid (will add it to exclusion list)
07:54:46.95 +51:55:10.4 -- not an asteroid (will add it to exclusion list)
07:34:56.89 +57:09:27.7 -- not an asteroid (will add it to exclusion list)
08:23:49.90 +53:22:50.8 -- not an asteroid (will add it to exclusion list)
07:41:45.73 +55:08:48.5 -- not an asteroid (will add it to exclusion list)
07:46:56.91 +53:09:44.8 -- not an asteroid (will add it to exclusion list)
07:41:27.42 +54:17:45.6 -- not an asteroid (will add it to exclusion list)
07:35:06.70 +56:38:01.5 -- not an asteroid (will add it to exclusion list)
08:23:37.39 +53:38:58.1 -- not an asteroid (will add it to exclusion list)
08:22:59.77 +54:42:06.7 -- not an asteroid (will add it to exclusion list)
07:45:48.55 +54:15:16.3 -- not an asteroid (will add it to exclusion list)
07:38:10.52 +55:46:39.3 -- not an asteroid (will add it to exclusion list)
07:36:35.60 +54:58:12.0 -- not an asteroid (will add it to exclusion list)
07:46:43.83 +54:19:28.3 -- not an asteroid (will add it to exclusion list)
08:25:06.82 +55:07:08.6 -- not an asteroid (will add it to exclusion list)
07:37:02.14 +55:41:37.4 -- not an asteroid (will add it to exclusion list)
08:20:29.59 +54:29:58.5 -- not an asteroid (will add it to exclusion list)
08:22:47.67 +53:36:29.4 -- not an asteroid (will add it to exclusion list)
07:44:28.28 +54:56:12.7 -- not an asteroid (will add it to exclusion list)
08:29:58.98 +52:39:36.2 -- not an asteroid (will add it to exclusion list)
07:53:52.09 +52:21:54.6 -- not an asteroid (will add it to exclusion list)
07:36:52.27 +56:32:22.5 -- not an asteroid (will add it to exclusion list)
07:40:21.75 +55:07:44.6 -- not an asteroid (will add it to exclusion list)
07:43:47.07 +54:44:17.4 -- not an asteroid (will add it to exclusion list)
07:43:25.33 +53:45:35.5 -- not an asteroid (will add it to exclusion list)
08:30:26.59 +50:48:42.7 -- not an asteroid (will add it to exclusion list)
07:50:14.95 +52:35:55.8 -- not an asteroid (will add it to exclusion list)
08:21:17.65 +55:52:24.3 -- not an asteroid (will add it to exclusion list)
07:57:21.96 +51:38:20.2 -- not an asteroid (will add it to exclusion list)
07:48:20.02 +53:32:46.9 -- not an asteroid (will add it to exclusion list)
07:43:16.14 +54:57:39.5 -- not an asteroid (will add it to exclusion list)
07:35:59.53 +56:25:04.9 -- not an asteroid (will add it to exclusion list)
07:36:46.02 +56:13:11.0 -- not an asteroid (will add it to exclusion list)
07:42:20.10 +53:55:41.9 -- not an asteroid (will add it to exclusion list)
07:46:00.03 +53:30:06.5 -- not an asteroid (will add it to exclusion list)
08:21:29.96 +55:52:09.2 -- not an asteroid (will add it to exclusion list)
08:22:47.63 +53:55:31.4 -- not an asteroid (will add it to exclusion list)
08:25:07.47 +54:53:40.7 -- not an asteroid (will add it to exclusion list)
07:45:23.81 +53:26:10.0 -- not an asteroid (will add it to exclusion list)
08:30:15.42 +51:18:45.9 -- not an asteroid (will add it to exclusion list)
07:36:46.57 +55:38:36.3 -- not an asteroid (will add it to exclusion list)
07:42:24.01 +53:56:43.2 -- not an asteroid (will add it to exclusion list)
08:22:29.37 +56:15:05.1 -- not an asteroid (will add it to exclusion list)
08:19:32.42 +55:15:19.1 -- not an asteroid (will add it to exclusion list)
08:18:10.08 +54:27:07.2 -- not an asteroid (will add it to exclusion list)
07:44:18.47 +54:30:05.6 -- not an asteroid (will add it to exclusion list)
08:23:19.57 +55:02:07.5 -- not an asteroid (will add it to exclusion list)
07:53:35.42 +52:02:03.4 -- not an asteroid (will add it to exclusion list)
08:21:57.74 +55:47:38.9 -- not an asteroid (will add it to exclusion list)
07:44:13.32 +54:39:52.6 -- not an asteroid (will add it to exclusion list)
08:23:36.29 +55:44:19.2 -- not an asteroid (will add it to exclusion list)
07:37:12.32 +55:23:32.6 -- not an asteroid (will add it to exclusion list)
08:23:24.65 +54:58:57.1 -- not an asteroid (will add it to exclusion list)
08:20:39.80 +54:09:46.5 -- not an asteroid (will add it to exclusion list)
08:21:26.25 +55:09:16.6 -- not an asteroid (will add it to exclusion list)
07:36:03.84 +55:31:10.8 -- not an asteroid (will add it to exclusion list)
07:50:26.70 +53:06:24.0 -- not an asteroid (will add it to exclusion list)
07:39:04.20 +56:15:54.4 -- not an asteroid (will add it to exclusion list)
07:41:29.74 +55:14:29.8 -- not an asteroid (will add it to exclusion list)
07:33:43.17 +57:39:46.0 -- not an asteroid (will add it to exclusion list)
08:20:21.71 +55:04:59.9 -- not an asteroid (will add it to exclusion list)
07:42:38.37 +54:49:25.3 -- not an asteroid (will add it to exclusion list)
07:36:08.84 +54:55:50.8 -- not an asteroid (will add it to exclusion list)
08:21:03.10 +56:00:39.6 -- not an asteroid (will add it to exclusion list)
08:21:35.81 +54:46:36.6 -- not an asteroid (will add it to exclusion list)
08:22:08.53 +54:17:21.7 -- not an asteroid (will add it to exclusion list)
07:39:17.70 +55:23:16.0 -- not an asteroid (will add it to exclusion list)
07:48:08.25 +53:48:43.9 -- not an asteroid (will add it to exclusion list)
07:39:21.84 +55:50:02.9 -- not an asteroid (will add it to exclusion list)
07:41:03.34 +54:33:56.2 -- not an asteroid (will add it to exclusion list)
08:17:42.27 +54:23:25.7 -- not an asteroid (will add it to exclusion list)
07:43:27.24 +55:12:08.2 -- not an asteroid (will add it to exclusion list)
07:40:04.45 +54:40:36.9 -- not an asteroid (will add it to exclusion list)
07:35:50.66 +55:51:21.7 -- not an asteroid (will add it to exclusion list)
08:24:24.22 +55:21:18.2 -- not an asteroid (will add it to exclusion list)
07:35:13.81 +55:53:47.1 -- not an asteroid (will add it to exclusion list)
08:22:01.99 +56:08:09.4 -- not an asteroid (will add it to exclusion list)
07:43:27.66 +54:04:31.3 -- not an asteroid (will add it to exclusion list)
08:23:39.92 +54:46:40.2 -- not an asteroid (will add it to exclusion list)
07:37:36.07 +56:03:44.1 -- not an asteroid (will add it to exclusion list)
07:43:24.84 +53:44:53.4 -- not an asteroid (will add it to exclusion list)
07:34:16.59 +57:19:06.4 -- not an asteroid (will add it to exclusion list)
07:38:20.12 +54:33:14.5 -- not an asteroid (will add it to exclusion list)
07:55:01.80 +51:57:11.9 -- not an asteroid (will add it to exclusion list)
07:35:35.48 +56:49:28.6 -- not an asteroid (will add it to exclusion list)
07:48:18.46 +53:53:11.7 -- not an asteroid (will add it to exclusion list)
07:34:41.23 +56:39:58.6 -- not an asteroid (will add it to exclusion list)
07:47:51.84 +53:06:16.7 -- not an asteroid (will add it to exclusion list)
08:22:29.44 +54:29:24.4 -- not an asteroid (will add it to exclusion list)
08:21:04.81 +54:37:13.0 -- not an asteroid (will add it to exclusion list)
08:30:07.81 +51:31:28.6 -- not an asteroid (will add it to exclusion list)
07:39:26.57 +54:51:37.2 -- not an asteroid (will add it to exclusion list)
08:18:35.58 +54:19:26.4 -- not an asteroid (will add it to exclusion list)
07:52:57.47 +52:27:42.3 -- not an asteroid (will add it to exclusion list)
07:39:14.89 +55:16:20.8 -- not an asteroid (will add it to exclusion list)
07:37:46.20 +56:11:21.2 -- not an asteroid (will add it to exclusion list)
07:50:20.44 +53:11:57.7 -- not an asteroid (will add it to exclusion list)
08:27:13.12 +52:34:44.1 -- not an asteroid (will add it to exclusion list)
08:22:10.59 +55:34:38.0 -- not an asteroid (will add it to exclusion list)
08:22:52.05 +54:50:30.2 -- not an asteroid (will add it to exclusion list)
08:24:07.27 +55:38:10.7 -- not an asteroid (will add it to exclusion list)
08:30:03.09 +52:51:45.9 -- not an asteroid (will add it to exclusion list)
08:29:06.02 +50:27:08.2 -- not an asteroid (will add it to exclusion list)
08:19:46.18 +54:30:16.5 -- not an asteroid (will add it to exclusion list)
08:19:50.90 +55:16:23.2 -- not an asteroid (will add it to exclusion list)
07:39:03.82 +54:35:34.8 -- not an asteroid (will add it to exclusion list)
08:23:40.68 +54:32:47.6 -- not an asteroid (will add it to exclusion list)
07:34:49.31 +56:46:00.1 -- not an asteroid (will add it to exclusion list)
07:38:27.23 +55:55:44.3 -- not an asteroid (will add it to exclusion list)
08:21:28.35 +55:55:30.5 -- not an asteroid (will add it to exclusion list)
07:41:40.62 +54:43:25.3 -- not an asteroid (will add it to exclusion list)
08:23:01.42 +53:58:13.5 -- not an asteroid (will add it to exclusion list)
07:43:55.30 +55:02:42.7 -- not an asteroid (will add it to exclusion list)
08:25:10.76 +53:58:41.6 -- not an asteroid (will add it to exclusion list)
07:55:24.96 +51:59:57.6 -- not an asteroid (will add it to exclusion list)
07:46:26.89 +53:12:40.4 -- not an asteroid (will add it to exclusion list)
08:21:15.19 +54:33:43.7 -- not an asteroid (will add it to exclusion list)
08:22:36.28 +54:19:34.6 -- not an asteroid (will add it to exclusion list)
07:39:26.44 +54:52:11.4 -- not an asteroid (will add it to exclusion list)
08:20:44.12 +54:50:49.5 -- not an asteroid (will add it to exclusion list)
07:38:11.55 +54:56:55.7 -- not an asteroid (will add it to exclusion list)
08:19:18.59 +54:26:52.2 -- not an asteroid (will add it to exclusion list)
07:43:21.52 +54:02:15.9 -- not an asteroid (will add it to exclusion list)
08:25:15.13 +54:20:44.1 -- not an asteroid (will add it to exclusion list)
08:22:50.92 +54:25:04.6 -- not an asteroid (will add it to exclusion list)
07:51:07.20 +52:19:45.7 -- not an asteroid (will add it to exclusion list)
08:22:40.52 +56:06:17.7 -- not an asteroid (will add it to exclusion list)
07:37:30.68 +56:12:49.8 -- not an asteroid (will add it to exclusion list)
08:24:57.97 +55:14:32.0 -- not an asteroid (will add it to exclusion list)
08:22:34.71 +54:35:25.5 -- not an asteroid (will add it to exclusion list)
07:45:33.34 +54:01:06.8 -- not an asteroid (will add it to exclusion list)
08:23:32.26 +55:55:42.3 -- not an asteroid (will add it to exclusion list)
07:42:09.60 +54:13:47.9 -- not an asteroid (will add it to exclusion list)
07:44:38.90 +53:34:46.4 -- not an asteroid (will add it to exclusion list)
08:20:22.08 +54:27:04.1 -- not an asteroid (will add it to exclusion list)
07:36:14.73 +56:02:36.2 -- not an asteroid (will add it to exclusion list)
08:22:49.24 +54:34:15.5 -- not an asteroid (will add it to exclusion list)
07:37:35.89 +54:14:28.7 -- not an asteroid (will add it to exclusion list)
08:26:08.55 +52:18:31.3 -- not an asteroid (will add it to exclusion list)
08:18:53.48 +55:00:48.8 -- not an asteroid (will add it to exclusion list)
07:36:10.39 +55:55:50.5 -- not an asteroid (will add it to exclusion list)
07:50:12.59 +52:50:49.4 -- not an asteroid (will add it to exclusion list)
07:37:04.40 +54:52:40.1 -- not an asteroid (will add it to exclusion list)
07:48:12.81 +53:28:36.0 -- not an asteroid (will add it to exclusion list)
07:37:58.07 +55:54:11.3 -- not an asteroid (will add it to exclusion list)
07:37:01.75 +54:44:06.1 -- not an asteroid (will add it to exclusion list)
07:48:07.62 +52:54:29.8 -- not an asteroid (will add it to exclusion list)
08:23:38.69 +54:02:34.5 -- not an asteroid (will add it to exclusion list)
07:43:48.01 +54:47:39.5 -- not an asteroid (will add it to exclusion list)
07:46:19.67 +53:56:13.3 -- not an asteroid (will add it to exclusion list)
08:19:29.06 +54:23:31.3 -- not an asteroid (will add it to exclusion list)
07:40:58.31 +54:23:59.2 -- not an asteroid (will add it to exclusion list)
08:19:02.89 +55:03:45.0 -- not an asteroid (will add it to exclusion list)
08:22:47.07 +53:46:45.6 -- not an asteroid (will add it to exclusion list)
07:38:01.34 +55:17:50.6 -- not an asteroid (will add it to exclusion list)
08:23:26.79 +53:48:34.0 -- not an asteroid (will add it to exclusion list)
07:41:25.85 +54:13:11.0 -- not an asteroid (will add it to exclusion list)
07:37:32.36 +54:09:45.7 -- not an asteroid (will add it to exclusion list)
07:40:36.19 +55:18:33.5 -- not an asteroid (will add it to exclusion list)
07:38:02.61 +55:53:42.3 -- not an asteroid (will add it to exclusion list)
08:19:33.42 +54:53:34.6 -- not an asteroid (will add it to exclusion list)
08:19:25.81 +54:23:56.9 -- not an asteroid (will add it to exclusion list)
08:24:38.92 +54:18:14.7 -- not an asteroid (will add it to exclusion list)
08:23:53.47 +54:35:02.7 -- not an asteroid (will add it to exclusion list)
07:38:29.72 +54:15:26.6 -- not an asteroid (will add it to exclusion list)
07:36:43.96 +55:13:09.0 -- not an asteroid (will add it to exclusion list)
07:39:51.24 +54:38:15.0 -- not an asteroid (will add it to exclusion list)
07:50:10.27 +52:52:47.8 -- not an asteroid (will add it to exclusion list)
08:22:31.19 +55:03:51.3 -- not an asteroid (will add it to exclusion list)
07:44:22.96 +54:01:23.9 -- not an asteroid (will add it to exclusion list)
07:49:35.56 +52:46:57.8 -- not an asteroid (will add it to exclusion list)
08:21:06.79 +54:02:48.9 -- not an asteroid (will add it to exclusion list)
07:37:26.97 +56:09:51.9 -- not an asteroid (will add it to exclusion list)
07:38:53.07 +55:42:39.7 -- not an asteroid (will add it to exclusion list)
07:39:10.36 +54:45:52.7 -- not an asteroid (will add it to exclusion list)
08:24:26.80 +54:03:54.0 -- not an asteroid (will add it to exclusion list)
07:38:04.77 +55:03:01.7 -- not an asteroid (will add it to exclusion list)
08:23:42.64 +54:28:03.8 -- not an asteroid (will add it to exclusion list)
07:35:28.16 +56:19:03.1 -- not an asteroid (will add it to exclusion list)
07:38:46.84 +55:09:13.2 -- not an asteroid (will add it to exclusion list)
08:29:00.74 +51:59:48.2 -- not an asteroid (will add it to exclusion list)
07:35:37.12 +56:50:12.9 -- not an asteroid (will add it to exclusion list)
07:44:39.02 +54:49:01.2 -- not an asteroid (will add it to exclusion list)
07:39:33.19 +54:46:50.8 -- not an asteroid (will add it to exclusion list)
07:39:44.46 +54:59:44.5 -- not an asteroid (will add it to exclusion list)
07:35:32.80 +56:35:01.5 -- not an asteroid (will add it to exclusion list)
07:35:50.19 +55:18:14.2 -- not an asteroid (will add it to exclusion list)
07:38:39.15 +55:04:11.9 -- not an asteroid (will add it to exclusion list)
07:40:55.12 +55:03:00.8 -- not an asteroid (will add it to exclusion list)
08:22:37.49 +54:18:22.1 -- not an asteroid (will add it to exclusion list)
07:45:26.17 +53:55:16.8 -- not an asteroid (will add it to exclusion list)
07:40:35.14 +54:52:08.2 -- not an asteroid (will add it to exclusion list)
07:44:21.86 +54:27:42.3 -- not an asteroid (will add it to exclusion list)
08:18:43.13 +54:11:04.4 -- not an asteroid (will add it to exclusion list)
07:47:48.82 +53:39:22.0 -- not an asteroid (will add it to exclusion list)
07:41:00.69 +54:10:29.6 -- not an asteroid (will add it to exclusion list)
07:37:48.24 +54:19:24.4 -- not an asteroid (will add it to exclusion list)
08:23:36.19 +55:24:14.5 -- not an asteroid (will add it to exclusion list)
07:38:18.66 +54:32:43.9 -- not an asteroid (will add it to exclusion list)
07:44:05.45 +53:47:06.7 -- not an asteroid (will add it to exclusion list)
08:22:26.66 +53:32:01.4 -- not an asteroid (will add it to exclusion list)
07:48:35.73 +52:59:32.6 -- not an asteroid (will add it to exclusion list)
07:49:53.36 +53:05:26.1 -- not an asteroid (will add it to exclusion list)
07:45:59.28 +53:44:56.4 -- not an asteroid (will add it to exclusion list)
08:22:55.28 +53:36:27.3 -- not an asteroid (will add it to exclusion list)
08:23:40.92 +54:46:16.5 -- not an asteroid (will add it to exclusion list)
07:36:22.29 +56:24:37.3 -- not an asteroid (will add it to exclusion list)
08:22:49.52 +55:15:05.6 -- not an asteroid (will add it to exclusion list)
08:22:13.07 +54:58:34.6 -- not an asteroid (will add it to exclusion list)
07:37:53.68 +55:27:34.6 -- not an asteroid (will add it to exclusion list)
07:43:01.13 +54:24:35.6 -- not an asteroid (will add it to exclusion list)
07:39:52.30 +55:41:14.5 -- not an asteroid (will add it to exclusion list)
07:45:22.97 +53:44:34.4 -- not an asteroid (will add it to exclusion list)
07:40:54.44 +54:44:27.3 -- not an asteroid (will add it to exclusion list)
08:21:35.48 +54:36:01.3 -- not an asteroid (will add it to exclusion list)
07:43:18.92 +55:00:17.6 -- not an asteroid (will add it to exclusion list)
08:18:15.86 +54:52:42.3 -- not an asteroid (will add it to exclusion list)
08:27:23.91 +52:26:37.0 -- not an asteroid (will add it to exclusion list)
08:21:08.91 +54:34:15.1 -- not an asteroid (will add it to exclusion list)
07:35:20.98 +55:46:23.8 -- not an asteroid (will add it to exclusion list)
07:37:35.63 +54:44:12.2 -- not an asteroid (will add it to exclusion list)
08:22:47.67 +55:41:20.1 -- not an asteroid (will add it to exclusion list)
07:37:48.36 +54:57:19.2 -- not an asteroid (will add it to exclusion list)
07:34:31.07 +56:44:46.8 -- not an asteroid (will add it to exclusion list)
07:41:15.74 +54:25:12.5 -- not an asteroid (will add it to exclusion list)
07:53:10.49 +52:11:45.9 -- not an asteroid (will add it to exclusion list)
08:20:05.67 +54:56:32.2 -- not an asteroid (will add it to exclusion list)
08:22:45.55 +54:48:16.4 -- not an asteroid (will add it to exclusion list)
08:18:00.98 +54:09:28.7 -- not an asteroid (will add it to exclusion list)
07:39:04.24 +54:47:15.5 -- not an asteroid (will add it to exclusion list)
07:36:59.57 +56:15:00.8 -- not an asteroid (will add it to exclusion list)
08:21:58.92 +54:51:27.6 -- not an asteroid (will add it to exclusion list)
07:35:52.42 +56:41:08.9 -- not an asteroid (will add it to exclusion list)
08:20:39.37 +54:15:45.2 -- not an asteroid (will add it to exclusion list)
07:53:37.95 +52:35:22.3 -- not an asteroid (will add it to exclusion list)
07:41:20.66 +54:21:52.3 -- not an asteroid (will add it to exclusion list)
07:44:41.74 +53:52:22.7 -- not an asteroid (will add it to exclusion list)
07:39:04.30 +55:12:49.1 -- not an asteroid (will add it to exclusion list)
07:40:50.18 +55:35:46.9 -- not an asteroid (will add it to exclusion list)
08:29:53.95 +52:11:45.2 -- not an asteroid (will add it to exclusion list)
07:43:47.59 +53:50:56.9 -- not an asteroid (will add it to exclusion list)
08:24:00.01 +53:29:07.2 -- not an asteroid (will add it to exclusion list)
07:50:57.44 +53:13:44.6 -- not an asteroid (will add it to exclusion list)
07:39:41.30 +55:00:42.1 -- not an asteroid (will add it to exclusion list)
07:39:08.76 +54:49:25.6 -- not an asteroid (will add it to exclusion list)
08:27:56.28 +50:40:42.4 -- not an asteroid (will add it to exclusion list)
07:42:24.42 +53:51:11.6 -- not an asteroid (will add it to exclusion list)
07:35:55.79 +56:20:54.4 -- not an asteroid (will add it to exclusion list)
07:41:45.24 +54:35:30.2 -- not an asteroid (will add it to exclusion list)
07:50:03.77 +52:27:27.8 -- not an asteroid (will add it to exclusion list)
08:23:04.26 +54:08:51.7 -- not an asteroid (will add it to exclusion list)
08:23:26.01 +56:13:04.6 -- not an asteroid (will add it to exclusion list)
08:24:10.77 +54:33:44.8 -- not an asteroid (will add it to exclusion list)
08:21:21.61 +54:39:08.7 -- not an asteroid (will add it to exclusion list)
07:42:15.94 +55:05:09.1 -- not an asteroid (will add it to exclusion list)
08:24:36.23 +55:23:44.8 -- not an asteroid (will add it to exclusion list)
07:46:38.01 +53:27:12.3 -- not an asteroid (will add it to exclusion list)
07:42:32.80 +53:57:04.7 -- not an asteroid (will add it to exclusion list)
07:44:07.41 +54:46:12.7 -- not an asteroid (will add it to exclusion list)
07:48:40.33 +53:10:16.0 -- not an asteroid (will add it to exclusion list)
08:25:03.30 +54:21:28.6 -- not an asteroid (will add it to exclusion list)
07:41:49.86 +54:54:21.4 -- not an asteroid (will add it to exclusion list)
07:43:23.87 +54:32:38.3 -- not an asteroid (will add it to exclusion list)
07:39:43.66 +55:32:36.0 -- not an asteroid (will add it to exclusion list)
08:20:01.93 +54:08:55.3 -- not an asteroid (will add it to exclusion list)
08:25:50.51 +53:25:39.8 -- not an asteroid (will add it to exclusion list)
07:46:20.22 +53:26:35.0 -- not an asteroid (will add it to exclusion list)
08:25:40.78 +53:36:12.7 -- not an asteroid (will add it to exclusion list)
07:39:34.92 +54:57:16.6 -- not an asteroid (will add it to exclusion list)
07:49:12.58 +52:57:39.1 -- not an asteroid (will add it to exclusion list)
07:49:09.01 +52:56:11.4 -- not an asteroid (will add it to exclusion list)
08:31:03.57 +52:28:11.3 -- not an asteroid (will add it to exclusion list)
08:21:01.17 +54:50:26.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
07:33:43.17 +57:39:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:16.59 +57:19:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:31.07 +56:44:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:37.63 +56:53:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:41.23 +56:39:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:47.64 +56:48:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:49.31 +56:46:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:34:56.89 +57:09:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:06.39 +56:25:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:06.70 +56:38:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:07.53 +56:24:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:13.81 +55:53:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:20.98 +55:46:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:28.16 +56:19:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:32.80 +56:35:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:35.48 +56:49:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:36.22 +56:18:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:37.12 +56:50:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:50.19 +55:18:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:50.66 +55:51:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:52.42 +56:41:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:54.03 +55:37:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:55.33 +56:16:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:55.79 +56:20:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:57.44 +56:32:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:35:59.53 +56:25:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:02.19 +55:16:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:02.24 +56:32:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:03.84 +55:31:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:08.84 +54:55:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:10.39 +55:55:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:14.73 +56:02:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:14.89 +56:59:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:15.61 +56:11:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:16.56 +55:02:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:19.16 +54:47:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:22.29 +56:24:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:26.43 +55:43:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:35.60 +54:58:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:41.06 +56:41:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:42.06 +55:25:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:43.96 +55:13:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:46.02 +56:13:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:46.57 +55:38:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:52.27 +56:32:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:53.55 +56:28:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:54.13 +55:53:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:55.95 +55:41:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:36:59.57 +56:15:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:01.75 +54:44:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:02.14 +55:41:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:04.40 +54:52:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:06.18 +54:48:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:07.12 +56:08:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:12.32 +55:23:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:14.26 +55:41:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:24.57 +54:13:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:26.97 +56:09:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:29.05 +56:35:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:29.78 +55:13:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:30.68 +56:12:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:32.36 +54:09:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:35.52 +55:27:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:35.63 +54:44:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:35.89 +54:14:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:36.07 +56:03:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:37.69 +55:30:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:46.20 +56:11:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:48.24 +54:19:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:48.36 +54:57:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:53.68 +55:27:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:55.92 +55:58:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:56.12 +56:00:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:37:58.07 +55:54:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:01.34 +55:17:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:02.61 +55:53:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:04.77 +55:03:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:05.39 +55:48:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:05.50 +55:09:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:06.68 +55:57:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:10.52 +55:46:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:11.55 +54:56:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:13.63 +54:29:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:18.66 +54:32:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:20.12 +54:33:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:27.15 +55:26:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:27.23 +55:55:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:29.72 +54:15:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:33.04 +55:46:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:37.01 +54:28:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:39.15 +55:04:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:41.65 +54:45:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:42.35 +56:15:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:43.19 +55:08:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:46.84 +55:09:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:49.79 +55:30:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:50.12 +54:28:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:52.63 +55:18:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:38:53.07 +55:42:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:03.82 +54:35:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:04.20 +56:15:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:04.24 +54:47:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:04.30 +55:12:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:06.38 +54:40:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:08.76 +54:49:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:09.96 +55:47:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:10.36 +54:45:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:14.89 +55:16:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:16.74 +55:55:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:17.70 +55:23:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:17.77 +54:46:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:21.84 +55:50:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:26.44 +54:52:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:26.57 +54:51:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:33.19 +54:46:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:34.92 +54:57:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:35.36 +54:45:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:38.17 +55:48:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:41.30 +55:00:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:43.66 +55:32:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:43.97 +54:33:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:44.46 +54:59:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:48.71 +55:13:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:48.96 +54:56:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:51.24 +54:38:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:52.30 +55:41:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:54.67 +54:51:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:39:58.65 +55:09:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:01.35 +55:37:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:03.23 +55:00:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:04.45 +54:40:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:04.76 +55:03:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:06.52 +55:41:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:21.75 +55:07:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:28.25 +54:50:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:35.14 +54:52:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:36.19 +55:18:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:37.52 +54:31:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:50.18 +55:35:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:54.44 +54:44:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:55.12 +55:03:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:58.31 +54:23:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:40:58.34 +54:34:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:00.69 +54:10:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:03.34 +54:33:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:11.23 +55:21:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:15.74 +54:25:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:15.81 +55:31:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:20.66 +54:21:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:25.85 +54:13:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:27.42 +54:17:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:29.74 +55:14:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:29.79 +54:55:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:36.53 +53:47:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:40.62 +54:43:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:45.24 +54:35:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:45.73 +55:08:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:49.86 +54:54:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:50.86 +54:06:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:51.68 +54:14:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:53.68 +54:15:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:55.54 +54:26:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:41:58.99 +54:53:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:06.78 +54:10:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:09.60 +54:13:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:15.94 +55:05:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:17.58 +54:16:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:20.10 +53:55:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:24.01 +53:56:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:24.42 +53:51:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:32.80 +53:57:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:36.30 +54:37:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:38.37 +54:49:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:49.87 +53:55:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:42:57.85 +55:23:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:01.13 +54:24:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:11.97 +54:08:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:16.14 +54:57:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:18.92 +55:00:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:21.52 +54:02:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:23.87 +54:32:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:24.84 +53:44:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:25.33 +53:45:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:27.24 +55:12:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:27.66 +54:04:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:37.81 +54:20:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:47.07 +54:44:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:47.59 +53:50:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:48.01 +54:47:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:51.41 +53:32:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:43:55.30 +55:02:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:05.45 +53:47:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:07.41 +54:46:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:13.32 +54:39:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:18.47 +54:30:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:18.63 +54:02:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:21.86 +54:27:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:22.96 +54:01:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:28.28 +54:56:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:38.90 +53:34:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:39.02 +54:49:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:41.74 +53:52:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:50.85 +53:49:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:44:51.57 +53:39:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:12.60 +53:51:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:22.97 +53:44:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:23.81 +53:26:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:26.17 +53:55:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:33.34 +54:01:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:41.00 +54:29:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:45.34 +53:56:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:48.55 +54:15:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:45:59.28 +53:44:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:00.03 +53:30:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:09.06 +54:14:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:14.97 +54:29:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:19.67 +53:56:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:20.22 +53:26:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:24.07 +53:53:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:26.89 +53:12:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:32.64 +53:32:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:38.01 +53:27:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:43.83 +54:19:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:46:56.91 +53:09:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:47:19.19 +53:17:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:47:19.74 +53:23:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:47:48.82 +53:39:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:47:51.84 +53:06:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:48:00.97 +53:23:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:48:07.62 +52:54:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:48:08.25 +53:48:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:48:12.81 +53:28:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:48:18.46 +53:53:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:48:20.02 +53:32:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:48:35.73 +52:59:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:48:40.33 +53:10:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:48:52.53 +53:47:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:48:53.14 +52:51:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:49:09.01 +52:56:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:49:09.67 +53:17:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:49:12.58 +52:57:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:49:35.56 +52:46:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:49:53.36 +53:05:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:50:03.77 +52:27:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:50:10.27 +52:52:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:50:12.59 +52:50:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:50:14.95 +52:35:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:50:20.44 +53:11:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:50:26.70 +53:06:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:50:53.27 +52:02:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:50:57.44 +53:13:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:51:07.20 +52:19:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:51:21.45 +52:58:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:51:42.67 +52:18:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:51:47.99 +52:02:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:52:37.90 +51:53:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:52:50.93 +51:56:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:52:57.47 +52:27:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:53:10.49 +52:11:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:53:35.42 +52:02:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:53:37.95 +52:35:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:53:52.09 +52:21:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:53:59.56 +52:13:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:54:46.95 +51:55:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:55:01.80 +51:57:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:55:04.71 +52:15:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:55:24.96 +51:59:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:56:24.25 +51:18:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:57:21.96 +51:38:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:16:57.81 +54:01:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:35.36 +54:32:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:35.39 +54:31:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:17:42.27 +54:23:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:00.44 +54:14:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:00.98 +54:09:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:10.08 +54:27:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:11.02 +54:33:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:15.86 +54:52:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:25.59 +54:52:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:35.58 +54:19:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:40.44 +54:53:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:43.13 +54:11:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:18:53.48 +55:00:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:02.89 +55:03:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:18.59 +54:26:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:25.81 +54:23:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:29.06 +54:23:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:32.42 +55:15:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:33.42 +54:53:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:35.98 +54:30:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:46.18 +54:30:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:50.90 +55:16:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:52.27 +54:23:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:57.25 +54:26:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:01.93 +54:08:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:05.67 +54:56:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:13.16 +55:24:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:20.60 +54:25:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:21.71 +55:04:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:22.08 +54:27:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:23.52 +54:43:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:25.65 +54:36:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:29.59 +54:29:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:31.20 +54:51:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:32.05 +54:36:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:39.37 +54:15:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:39.80 +54:09:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:41.34 +54:24:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:42.39 +55:07:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:44.12 +54:50:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:47.18 +53:50:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:01.17 +54:50:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:03.10 +56:00:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:04.81 +54:37:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:05.41 +55:15:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:06.79 +54:02:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:08.91 +54:34:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:09.51 +54:52:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:15.19 +54:33:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:17.65 +55:52:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:21.61 +54:39:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:26.25 +55:09:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:28.35 +55:55:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:29.96 +55:52:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:31.30 +54:10:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:34.56 +55:16:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:35.05 +55:03:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:35.48 +54:36:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:35.81 +54:46:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:40.12 +55:53:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:44.81 +54:19:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:46.32 +54:37:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:49.94 +55:34:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:50.21 +54:43:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:52.15 +53:44:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:56.67 +54:55:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:57.74 +55:47:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:58.92 +54:51:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:01.99 +56:08:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:02.47 +53:46:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:07.97 +54:49:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:08.53 +54:17:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:09.31 +54:05:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:09.54 +54:25:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:10.59 +55:34:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:11.83 +55:10:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:13.07 +54:58:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:18.69 +55:14:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:19.19 +55:49:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:20.43 +55:13:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:25.51 +56:03:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:26.66 +53:32:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:26.98 +55:21:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:29.37 +56:15:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:29.44 +54:29:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:31.19 +55:03:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:32.72 +55:14:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:34.71 +54:35:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:36.28 +54:19:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:37.10 +54:57:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:37.49 +54:18:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:40.17 +55:45:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:40.52 +56:06:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:45.55 +54:48:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:47.07 +53:46:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:47.63 +53:55:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:47.67 +53:36:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:47.67 +55:41:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:49.24 +54:34:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:49.52 +55:15:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:50.92 +54:25:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:52.05 +54:50:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:53.87 +54:43:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:55.28 +53:36:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:57.08 +54:47:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:59.77 +54:42:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:00.37 +54:36:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:01.42 +53:58:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:03.29 +54:55:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:04.26 +54:08:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:06.53 +55:21:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:07.38 +54:01:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:14.65 +55:43:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:19.57 +55:02:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:24.65 +54:58:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:25.31 +53:58:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:26.01 +56:13:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:26.79 +53:48:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:28.28 +55:29:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:32.17 +54:14:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:32.26 +55:55:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:32.85 +54:43:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:35.28 +54:26:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:36.19 +55:24:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:36.29 +55:44:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:37.39 +53:38:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:38.69 +54:02:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:39.92 +54:46:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:40.48 +55:06:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:40.68 +54:32:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:40.92 +54:46:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:42.64 +54:28:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:47.35 +55:37:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:49.90 +53:22:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:51.64 +53:44:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:23:53.47 +54:35:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:00.01 +53:29:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:00.81 +54:08:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:03.76 +55:39:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:04.86 +55:47:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:07.27 +55:38:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:10.77 +54:33:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:18.65 +55:32:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:24.22 +55:21:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:26.80 +54:03:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:30.55 +54:40:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:36.23 +55:23:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:38.04 +53:27:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:38.92 +54:18:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:43.36 +55:07:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:57.97 +55:14:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:03.30 +54:21:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:03.71 +53:28:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:06.57 +52:50:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:06.82 +55:07:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:07.47 +54:53:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:10.76 +53:58:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:15.13 +54:20:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:21.22 +53:50:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:25.27 +54:28:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:40.78 +53:36:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:50.51 +53:25:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:57.72 +54:29:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:26:08.55 +52:18:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:26:10.66 +52:46:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:27:13.12 +52:34:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:27:23.91 +52:26:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:27:56.28 +50:40:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:28:16.57 +51:54:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:28:27.72 +52:26:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:28:55.29 +52:46:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:00.74 +51:59:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:06.02 +50:27:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:11.10 +52:20:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:30.29 +52:42:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:35.69 +50:46:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:53.95 +52:11:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:58.98 +52:39:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:30:03.09 +52:51:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:30:07.81 +51:31:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:30:15.42 +51:18:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:30:26.59 +50:48:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:30:35.78 +52:40:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:31:03.57 +52:28:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:31:04.65 +52:33:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:31:24.58 +53:21:19.4 -- 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)
07:33:43.17 +57:39:46.0 -- not a known variable star
07:34:16.59 +57:19:06.4 -- not a known variable star
07:34:31.07 +56:44:46.8 -- not a known variable star
07:34:37.63 +56:53:42.1 -- not a known variable star
07:34:41.23 +56:39:58.6 -- not a known variable star
07:34:47.64 +56:48:18.1 -- not a known variable star
07:34:49.31 +56:46:00.1 -- a known variable star
07:34:56.89 +57:09:27.7 -- not a known variable star
07:35:06.39 +56:25:49.4 -- not a known variable star
07:35:06.70 +56:38:01.5 -- not a known variable star
07:35:07.53 +56:24:08.6 -- not a known variable star
07:35:13.81 +55:53:47.1 -- not a known variable star
07:35:20.98 +55:46:23.8 -- not a known variable star
07:35:28.16 +56:19:03.1 -- not a known variable star
07:35:32.80 +56:35:01.5 -- not a known variable star
07:35:35.48 +56:49:28.6 -- not a known variable star
07:35:36.22 +56:18:23.6 -- not a known variable star
07:35:37.12 +56:50:12.9 -- not a known variable star
07:35:50.19 +55:18:14.2 -- not a known variable star
07:35:50.66 +55:51:21.7 -- not a known variable star
07:35:52.42 +56:41:08.9 -- not a known variable star
07:35:54.03 +55:37:17.7 -- not a known variable star
07:35:55.33 +56:16:01.8 -- not a known variable star
07:35:55.79 +56:20:54.4 -- not a known variable star
07:35:57.44 +56:32:21.2 -- not a known variable star
07:35:59.53 +56:25:04.9 -- not a known variable star
07:36:02.19 +55:16:12.9 -- not a known variable star
07:36:02.24 +56:32:40.2 -- not a known variable star
07:36:03.84 +55:31:10.8 -- not a known variable star
07:36:08.84 +54:55:50.8 -- not a known variable star
07:36:10.39 +55:55:50.5 -- not a known variable star
07:36:14.73 +56:02:36.2 -- not a known variable star
07:36:14.89 +56:59:44.3 -- not a known variable star
07:36:15.61 +56:11:10.5 -- not a known variable star
07:36:16.56 +55:02:53.2 -- not a known variable star
07:36:19.16 +54:47:41.2 -- not a known variable star
07:36:22.29 +56:24:37.3 -- not a known variable star
07:36:26.43 +55:43:01.1 -- not a known variable star
07:36:35.60 +54:58:12.0 -- not a known variable star
07:36:41.06 +56:41:14.3 -- not a known variable star
07:36:42.06 +55:25:31.8 -- not a known variable star
07:36:43.96 +55:13:09.0 -- not a known variable star
07:36:46.02 +56:13:11.0 -- not a known variable star
07:36:46.57 +55:38:36.3 -- not a known variable star
07:36:52.27 +56:32:22.5 -- not a known variable star
07:36:53.55 +56:28:46.4 -- not a known variable star
07:36:54.13 +55:53:12.8 -- not a known variable star
07:36:55.95 +55:41:28.8 -- not a known variable star
07:36:59.57 +56:15:00.8 -- not a known variable star
07:37:01.75 +54:44:06.1 -- not a known variable star
07:37:02.14 +55:41:37.4 -- not a known variable star
07:37:04.40 +54:52:40.1 -- not a known variable star
07:37:06.18 +54:48:15.3 -- not a known variable star
07:37:07.12 +56:08:12.9 -- not a known variable star
07:37:12.32 +55:23:32.6 -- not a known variable star
07:37:14.26 +55:41:09.7 -- a known variable star
07:37:24.57 +54:13:19.4 -- not a known variable star
07:37:26.97 +56:09:51.9 -- not a known variable star
07:37:29.05 +56:35:29.5 -- not a known variable star
07:37:29.78 +55:13:06.1 -- not a known variable star
07:37:30.68 +56:12:49.8 -- not a known variable star
07:37:32.36 +54:09:45.7 -- not a known variable star
07:37:35.52 +55:27:56.4 -- not a known variable star
07:37:35.63 +54:44:12.2 -- not a known variable star
07:37:35.89 +54:14:28.7 -- not a known variable star
07:37:36.07 +56:03:44.1 -- not a known variable star
07:37:37.69 +55:30:54.0 -- not a known variable star
07:37:46.20 +56:11:21.2 -- not a known variable star
07:37:48.24 +54:19:24.4 -- not a known variable star
07:37:48.36 +54:57:19.2 -- not a known variable star
07:37:53.68 +55:27:34.6 -- not a known variable star
07:37:55.92 +55:58:52.9 -- not a known variable star
07:37:56.12 +56:00:26.4 -- not a known variable star
07:37:58.07 +55:54:11.3 -- not a known variable star
07:38:01.34 +55:17:50.6 -- not a known variable star
07:38:02.61 +55:53:42.3 -- not a known variable star
07:38:04.77 +55:03:01.7 -- not a known variable star
07:38:05.39 +55:48:16.8 -- not a known variable star
07:38:05.50 +55:09:25.6 -- not a known variable star
07:38:06.68 +55:57:53.4 -- not a known variable star
07:38:10.52 +55:46:39.3 -- not a known variable star
07:38:11.55 +54:56:55.7 -- not a known variable star
07:38:13.63 +54:29:54.6 -- not a known variable star
07:38:18.66 +54:32:43.9 -- a known variable star
07:38:20.12 +54:33:14.5 -- not a known variable star
07:38:27.15 +55:26:21.1 -- not a known variable star
07:38:27.23 +55:55:44.3 -- not a known variable star
07:38:29.72 +54:15:26.6 -- not a known variable star
07:38:33.04 +55:46:12.3 -- not a known variable star
07:38:37.01 +54:28:01.6 -- not a known variable star
07:38:39.15 +55:04:11.9 -- not a known variable star
07:38:41.65 +54:45:44.0 -- not a known variable star
07:38:42.35 +56:15:56.9 -- not a known variable star
07:38:43.19 +55:08:18.5 -- not a known variable star
07:38:46.84 +55:09:13.2 -- not a known variable star
07:38:49.79 +55:30:13.0 -- not a known variable star
07:38:50.12 +54:28:35.1 -- not a known variable star
07:38:52.63 +55:18:01.4 -- a known variable star
07:38:53.07 +55:42:39.7 -- not a known variable star
07:39:03.82 +54:35:34.8 -- not a known variable star
07:39:04.20 +56:15:54.4 -- not a known variable star
07:39:04.24 +54:47:15.5 -- not a known variable star
07:39:04.30 +55:12:49.1 -- not a known variable star
07:39:06.38 +54:40:18.3 -- a known variable star
07:39:08.76 +54:49:25.6 -- not a known variable star
07:39:09.96 +55:47:49.8 -- not a known variable star
07:39:10.36 +54:45:52.7 -- not a known variable star
07:39:14.89 +55:16:20.8 -- not a known variable star
07:39:16.74 +55:55:09.1 -- not a known variable star
07:39:17.70 +55:23:16.0 -- not a known variable star
07:39:17.77 +54:46:55.1 -- a known variable star
07:39:21.84 +55:50:02.9 -- not a known variable star
07:39:26.44 +54:52:11.4 -- not a known variable star
07:39:26.57 +54:51:37.2 -- not a known variable star
07:39:33.19 +54:46:50.8 -- not a known variable star
07:39:34.92 +54:57:16.6 -- not a known variable star
07:39:35.36 +54:45:36.3 -- not a known variable star
07:39:38.17 +55:48:47.4 -- not a known variable star
07:39:41.30 +55:00:42.1 -- a known variable star
07:39:43.66 +55:32:36.0 -- not a known variable star
07:39:43.97 +54:33:22.6 -- not a known variable star
07:39:44.46 +54:59:44.5 -- not a known variable star
07:39:48.71 +55:13:56.6 -- not a known variable star
07:39:48.96 +54:56:12.8 -- not a known variable star
07:39:51.24 +54:38:15.0 -- not a known variable star
07:39:52.30 +55:41:14.5 -- not a known variable star
07:39:54.67 +54:51:50.3 -- not a known variable star
07:39:58.65 +55:09:48.5 -- not a known variable star
07:40:01.35 +55:37:17.0 -- not a known variable star
07:40:03.23 +55:00:00.4 -- not a known variable star
07:40:04.45 +54:40:36.9 -- not a known variable star
07:40:04.76 +55:03:36.6 -- not a known variable star
07:40:06.52 +55:41:14.5 -- not a known variable star
07:40:21.75 +55:07:44.6 -- a known variable star
07:40:28.25 +54:50:55.9 -- not a known variable star
07:40:35.14 +54:52:08.2 -- not a known variable star
07:40:36.19 +55:18:33.5 -- not a known variable star
07:40:37.52 +54:31:57.3 -- not a known variable star
07:40:50.18 +55:35:46.9 -- not a known variable star
07:40:54.44 +54:44:27.3 -- not a known variable star
07:40:55.12 +55:03:00.8 -- not a known variable star
07:40:58.31 +54:23:59.2 -- not a known variable star
07:40:58.34 +54:34:29.0 -- not a known variable star
07:41:00.69 +54:10:29.6 -- not a known variable star
07:41:03.34 +54:33:56.2 -- a known variable star
07:41:11.23 +55:21:33.9 -- not a known variable star
07:41:15.74 +54:25:12.5 -- not a known variable star
07:41:15.81 +55:31:02.6 -- not a known variable star
07:41:20.66 +54:21:52.3 -- not a known variable star
07:41:25.85 +54:13:11.0 -- not a known variable star
07:41:27.42 +54:17:45.6 -- not a known variable star
07:41:29.74 +55:14:29.8 -- not a known variable star
07:41:29.79 +54:55:00.1 -- not a known variable star
07:41:36.53 +53:47:29.7 -- a known variable star
07:41:40.62 +54:43:25.3 -- not a known variable star
07:41:45.24 +54:35:30.2 -- not a known variable star
07:41:45.73 +55:08:48.5 -- not a known variable star
07:41:49.86 +54:54:21.4 -- not a known variable star
07:41:50.86 +54:06:49.1 -- not a known variable star
07:41:51.68 +54:14:53.6 -- not a known variable star
07:41:53.68 +54:15:59.6 -- not a known variable star
07:41:55.54 +54:26:56.1 -- not a known variable star
07:41:58.99 +54:53:17.2 -- not a known variable star
07:42:06.78 +54:10:48.9 -- not a known variable star
07:42:09.60 +54:13:47.9 -- not a known variable star
07:42:15.94 +55:05:09.1 -- not a known variable star
07:42:17.58 +54:16:12.4 -- not a known variable star
07:42:20.10 +53:55:41.9 -- not a known variable star
07:42:24.01 +53:56:43.2 -- not a known variable star
07:42:24.42 +53:51:11.6 -- not a known variable star
07:42:32.80 +53:57:04.7 -- not a known variable star
07:42:36.30 +54:37:51.7 -- not a known variable star
07:42:38.37 +54:49:25.3 -- not a known variable star
07:42:49.87 +53:55:21.5 -- not a known variable star
07:42:57.85 +55:23:49.5 -- not a known variable star
07:43:01.13 +54:24:35.6 -- not a known variable star
07:43:11.97 +54:08:56.3 -- not a known variable star
07:43:16.14 +54:57:39.5 -- not a known variable star
07:43:18.92 +55:00:17.6 -- not a known variable star
07:43:21.52 +54:02:15.9 -- a known variable star
07:43:23.87 +54:32:38.3 -- not a known variable star
07:43:24.84 +53:44:53.4 -- not a known variable star
07:43:25.33 +53:45:35.5 -- not a known variable star
07:43:27.24 +55:12:08.2 -- not a known variable star
07:43:27.66 +54:04:31.3 -- not a known variable star
07:43:37.81 +54:20:34.7 -- not a known variable star
07:43:47.07 +54:44:17.4 -- not a known variable star
07:43:47.59 +53:50:56.9 -- a known variable star
07:43:48.01 +54:47:39.5 -- not a known variable star
07:43:51.41 +53:32:09.1 -- not a known variable star
07:43:55.30 +55:02:42.7 -- not a known variable star
07:44:05.45 +53:47:06.7 -- not a known variable star
07:44:07.41 +54:46:12.7 -- not a known variable star
07:44:13.32 +54:39:52.6 -- not a known variable star
07:44:18.47 +54:30:05.6 -- not a known variable star
07:44:18.63 +54:02:10.9 -- a known variable star
07:44:21.86 +54:27:42.3 -- not a known variable star
07:44:22.96 +54:01:23.9 -- not a known variable star
07:44:28.28 +54:56:12.7 -- not a known variable star
07:44:38.90 +53:34:46.4 -- not a known variable star
07:44:39.02 +54:49:01.2 -- not a known variable star
07:44:41.74 +53:52:22.7 -- not a known variable star
07:44:50.85 +53:49:29.2 -- not a known variable star
07:44:51.57 +53:39:04.0 -- not a known variable star
07:45:12.60 +53:51:05.8 -- not a known variable star
07:45:22.97 +53:44:34.4 -- not a known variable star
07:45:23.81 +53:26:10.0 -- not a known variable star
07:45:26.17 +53:55:16.8 -- not a known variable star
07:45:33.34 +54:01:06.8 -- a known variable star
07:45:41.00 +54:29:58.7 -- a known variable star
07:45:45.34 +53:56:15.1 -- not a known variable star
07:45:48.55 +54:15:16.3 -- not a known variable star
07:45:59.28 +53:44:56.4 -- not a known variable star
07:46:00.03 +53:30:06.5 -- not a known variable star
07:46:09.06 +54:14:31.2 -- not a known variable star
07:46:14.97 +54:29:08.2 -- a known variable star
07:46:19.67 +53:56:13.3 -- not a known variable star
07:46:20.22 +53:26:35.0 -- not a known variable star
07:46:24.07 +53:53:07.4 -- not a known variable star
07:46:26.89 +53:12:40.4 -- not a known variable star
07:46:32.64 +53:32:12.8 -- not a known variable star
07:46:38.01 +53:27:12.3 -- not a known variable star
07:46:43.83 +54:19:28.3 -- not a known variable star
07:46:56.91 +53:09:44.8 -- not a known variable star
07:47:19.19 +53:17:11.6 -- not a known variable star
07:47:19.74 +53:23:26.8 -- not a known variable star
07:47:48.82 +53:39:22.0 -- not a known variable star
07:47:51.84 +53:06:16.7 -- not a known variable star
07:48:00.97 +53:23:03.7 -- not a known variable star
07:48:07.62 +52:54:29.8 -- a known variable star
07:48:08.25 +53:48:43.9 -- not a known variable star
07:48:12.81 +53:28:36.0 -- not a known variable star
07:48:18.46 +53:53:11.7 -- a known variable star
07:48:20.02 +53:32:46.9 -- not a known variable star
07:48:35.73 +52:59:32.6 -- not a known variable star
07:48:40.33 +53:10:16.0 -- not a known variable star
07:48:52.53 +53:47:11.8 -- not a known variable star
07:48:53.14 +52:51:05.1 -- not a known variable star
07:49:09.01 +52:56:11.4 -- a known variable star
07:49:09.67 +53:17:30.8 -- not a known variable star
07:49:12.58 +52:57:39.1 -- not a known variable star
07:49:35.56 +52:46:57.8 -- not a known variable star
07:49:53.36 +53:05:26.1 -- not a known variable star
07:50:03.77 +52:27:27.8 -- not a known variable star
07:50:10.27 +52:52:47.8 -- not a known variable star
07:50:12.59 +52:50:49.4 -- a known variable star
07:50:14.95 +52:35:55.8 -- not a known variable star
07:50:20.44 +53:11:57.7 -- not a known variable star
07:50:26.70 +53:06:24.0 -- not a known variable star
07:50:53.27 +52:02:00.8 -- not a known variable star
07:50:57.44 +53:13:44.6 -- not a known variable star
07:51:07.20 +52:19:45.7 -- a known variable star
07:51:21.45 +52:58:24.8 -- not a known variable star
07:51:42.67 +52:18:52.1 -- not a known variable star
07:51:47.99 +52:02:46.5 -- not a known variable star
07:52:37.90 +51:53:24.3 -- not a known variable star
07:52:50.93 +51:56:21.6 -- not a known variable star
07:52:57.47 +52:27:42.3 -- not a known variable star
07:53:10.49 +52:11:45.9 -- not a known variable star
07:53:35.42 +52:02:03.4 -- not a known variable star
07:53:37.95 +52:35:22.3 -- not a known variable star
07:53:52.09 +52:21:54.6 -- not a known variable star
07:53:59.56 +52:13:15.1 -- not a known variable star
07:54:46.95 +51:55:10.4 -- a known variable star
07:55:01.80 +51:57:11.9 -- a known variable star
07:55:04.71 +52:15:16.7 -- not a known variable star
07:55:24.96 +51:59:57.6 -- not a known variable star
07:56:24.25 +51:18:20.8 -- not a known variable star
07:57:21.96 +51:38:20.2 -- not a known variable star
08:16:57.81 +54:01:28.8 -- not a known variable star
08:17:35.36 +54:32:08.6 -- not a known variable star
08:17:35.39 +54:31:08.8 -- not a known variable star
08:17:42.27 +54:23:25.7 -- not a known variable star
08:18:00.44 +54:14:37.9 -- not a known variable star
08:18:00.98 +54:09:28.7 -- not a known variable star
08:18:10.08 +54:27:07.2 -- not a known variable star
08:18:11.02 +54:33:37.0 -- not a known variable star
08:18:15.86 +54:52:42.3 -- not a known variable star
08:18:25.59 +54:52:09.2 -- not a known variable star
08:18:35.58 +54:19:26.4 -- not a known variable star
08:18:40.44 +54:53:54.8 -- a known variable star
08:18:43.13 +54:11:04.4 -- not a known variable star
08:18:53.48 +55:00:48.8 -- not a known variable star
08:19:02.89 +55:03:45.0 -- not a known variable star
08:19:18.59 +54:26:52.2 -- not a known variable star
08:19:25.81 +54:23:56.9 -- not a known variable star
08:19:29.06 +54:23:31.3 -- not a known variable star
08:19:32.42 +55:15:19.1 -- not a known variable star
08:19:33.42 +54:53:34.6 -- not a known variable star
08:19:35.98 +54:30:32.0 -- not a known variable star
08:19:46.18 +54:30:16.5 -- not a known variable star
08:19:50.90 +55:16:23.2 -- not a known variable star
08:19:52.27 +54:23:11.1 -- not a known variable star
08:19:57.25 +54:26:07.0 -- not a known variable star
08:20:01.93 +54:08:55.3 -- not a known variable star
08:20:05.67 +54:56:32.2 -- not a known variable star
08:20:13.16 +55:24:10.1 -- not a known variable star
08:20:20.60 +54:25:09.5 -- not a known variable star
08:20:21.71 +55:04:59.9 -- not a known variable star
08:20:22.08 +54:27:04.1 -- not a known variable star
08:20:23.52 +54:43:10.0 -- not a known variable star
08:20:25.65 +54:36:08.0 -- not a known variable star
08:20:29.59 +54:29:58.5 -- not a known variable star
08:20:31.20 +54:51:57.2 -- not a known variable star
08:20:32.05 +54:36:18.0 -- not a known variable star
08:20:39.37 +54:15:45.2 -- a known variable star
08:20:39.80 +54:09:46.5 -- not a known variable star
08:20:41.34 +54:24:53.0 -- not a known variable star
08:20:42.39 +55:07:06.1 -- not a known variable star
08:20:44.12 +54:50:49.5 -- not a known variable star
08:20:47.18 +53:50:31.3 -- not a known variable star
08:21:01.17 +54:50:26.5 -- not a known variable star
08:21:03.10 +56:00:39.6 -- a known variable star
08:21:04.81 +54:37:13.0 -- not a known variable star
08:21:05.41 +55:15:28.2 -- not a known variable star
08:21:06.79 +54:02:48.9 -- not a known variable star
08:21:08.91 +54:34:15.1 -- not a known variable star
08:21:09.51 +54:52:49.0 -- not a known variable star
08:21:15.19 +54:33:43.7 -- not a known variable star
08:21:17.65 +55:52:24.3 -- not a known variable star
08:21:21.61 +54:39:08.7 -- not a known variable star
08:21:26.25 +55:09:16.6 -- not a known variable star
08:21:28.35 +55:55:30.5 -- not a known variable star
08:21:29.96 +55:52:09.2 -- not a known variable star
08:21:31.30 +54:10:09.5 -- not a known variable star
08:21:34.56 +55:16:32.5 -- not a known variable star
08:21:35.05 +55:03:26.9 -- not a known variable star
08:21:35.48 +54:36:01.3 -- not a known variable star
08:21:35.81 +54:46:36.6 -- not a known variable star
08:21:40.12 +55:53:12.0 -- not a known variable star
08:21:44.81 +54:19:59.5 -- not a known variable star
08:21:46.32 +54:37:10.4 -- not a known variable star
08:21:49.94 +55:34:36.4 -- not a known variable star
08:21:50.21 +54:43:16.5 -- a known variable star
08:21:52.15 +53:44:08.1 -- not a known variable star
08:21:56.67 +54:55:13.9 -- not a known variable star
08:21:57.74 +55:47:38.9 -- not a known variable star
08:21:58.92 +54:51:27.6 -- a known variable star
08:22:01.99 +56:08:09.4 -- not a known variable star
08:22:02.47 +53:46:30.7 -- not a known variable star
08:22:07.97 +54:49:05.8 -- not a known variable star
08:22:08.53 +54:17:21.7 -- not a known variable star
08:22:09.31 +54:05:44.2 -- not a known variable star
08:22:09.54 +54:25:50.2 -- not a known variable star
08:22:10.59 +55:34:38.0 -- not a known variable star
08:22:11.83 +55:10:59.1 -- not a known variable star
08:22:13.07 +54:58:34.6 -- not a known variable star
08:22:18.69 +55:14:58.2 -- not a known variable star
08:22:19.19 +55:49:25.3 -- not a known variable star
08:22:20.43 +55:13:53.6 -- not a known variable star
08:22:25.51 +56:03:00.2 -- not a known variable star
08:22:26.66 +53:32:01.4 -- a known variable star
08:22:26.98 +55:21:55.0 -- not a known variable star
08:22:29.37 +56:15:05.1 -- not a known variable star
08:22:29.44 +54:29:24.4 -- not a known variable star
08:22:31.19 +55:03:51.3 -- not a known variable star
08:22:32.72 +55:14:19.4 -- not a known variable star
08:22:34.71 +54:35:25.5 -- not a known variable star
08:22:36.28 +54:19:34.6 -- not a known variable star
08:22:37.10 +54:57:33.1 -- not a known variable star
08:22:37.49 +54:18:22.1 -- not a known variable star
08:22:40.17 +55:45:09.4 -- not a known variable star
08:22:40.52 +56:06:17.7 -- not a known variable star
08:22:45.55 +54:48:16.4 -- not a known variable star
08:22:47.07 +53:46:45.6 -- not a known variable star
08:22:47.63 +53:55:31.4 -- not a known variable star
08:22:47.67 +53:36:29.4 -- not a known variable star
08:22:47.67 +55:41:20.1 -- not a known variable star
08:22:49.24 +54:34:15.5 -- not a known variable star
08:22:49.52 +55:15:05.6 -- not a known variable star
08:22:50.92 +54:25:04.6 -- not a known variable star
08:22:52.05 +54:50:30.2 -- a known variable star
08:22:53.87 +54:43:53.5 -- not a known variable star
08:22:55.28 +53:36:27.3 -- not a known variable star
08:22:57.08 +54:47:31.3 -- not a known variable star
08:22:59.77 +54:42:06.7 -- not a known variable star
08:23:00.37 +54:36:02.2 -- not a known variable star
08:23:01.42 +53:58:13.5 -- not a known variable star
08:23:03.29 +54:55:55.7 -- not a known variable star
08:23:04.26 +54:08:51.7 -- a known variable star
08:23:06.53 +55:21:06.2 -- not a known variable star
08:23:07.38 +54:01:29.0 -- not a known variable star
08:23:14.65 +55:43:12.6 -- not a known variable star
08:23:19.57 +55:02:07.5 -- not a known variable star
08:23:24.65 +54:58:57.1 -- not a known variable star
08:23:25.31 +53:58:35.1 -- not a known variable star
08:23:26.01 +56:13:04.6 -- not a known variable star
08:23:26.79 +53:48:34.0 -- not a known variable star
08:23:28.28 +55:29:36.3 -- not a known variable star
08:23:32.17 +54:14:46.8 -- not a known variable star
08:23:32.26 +55:55:42.3 -- a known variable star
08:23:32.85 +54:43:15.6 -- not a known variable star
08:23:35.28 +54:26:58.8 -- not a known variable star
08:23:36.19 +55:24:14.5 -- not a known variable star
08:23:36.29 +55:44:19.2 -- not a known variable star
08:23:37.39 +53:38:58.1 -- not a known variable star
08:23:38.69 +54:02:34.5 -- not a known variable star
08:23:39.92 +54:46:40.2 -- not a known variable star
08:23:40.48 +55:06:30.6 -- not a known variable star
08:23:40.68 +54:32:47.6 -- not a known variable star
08:23:40.92 +54:46:16.5 -- not a known variable star
08:23:42.64 +54:28:03.8 -- not a known variable star
08:23:47.35 +55:37:40.6 -- not a known variable star
08:23:49.90 +53:22:50.8 -- not a known variable star
08:23:51.64 +53:44:49.9 -- not a known variable star
08:23:53.47 +54:35:02.7 -- not a known variable star
08:24:00.01 +53:29:07.2 -- not a known variable star
08:24:00.81 +54:08:22.1 -- not a known variable star
08:24:03.76 +55:39:09.9 -- a known variable star
08:24:04.86 +55:47:30.2 -- not a known variable star
08:24:07.27 +55:38:10.7 -- not a known variable star
08:24:10.77 +54:33:44.8 -- not a known variable star
08:24:18.65 +55:32:22.0 -- not a known variable star
08:24:24.22 +55:21:18.2 -- not a known variable star
08:24:26.80 +54:03:54.0 -- not a known variable star
08:24:30.55 +54:40:25.7 -- not a known variable star
08:24:36.23 +55:23:44.8 -- not a known variable star
08:24:38.04 +53:27:22.1 -- not a known variable star
08:24:38.92 +54:18:14.7 -- not a known variable star
08:24:43.36 +55:07:09.6 -- not a known variable star
08:24:57.97 +55:14:32.0 -- not a known variable star
08:25:03.30 +54:21:28.6 -- not a known variable star
08:25:03.71 +53:28:32.5 -- not a known variable star
08:25:06.57 +52:50:43.1 -- not a known variable star
08:25:06.82 +55:07:08.6 -- not a known variable star
08:25:07.47 +54:53:40.7 -- not a known variable star
08:25:10.76 +53:58:41.6 -- not a known variable star
08:25:15.13 +54:20:44.1 -- not a known variable star
08:25:21.22 +53:50:55.1 -- not a known variable star
08:25:25.27 +54:28:25.1 -- not a known variable star
08:25:40.78 +53:36:12.7 -- not a known variable star
08:25:50.51 +53:25:39.8 -- not a known variable star
08:25:57.72 +54:29:22.2 -- not a known variable star
08:26:08.55 +52:18:31.3 -- not a known variable star
08:26:10.66 +52:46:37.9 -- not a known variable star
08:27:13.12 +52:34:44.1 -- not a known variable star
08:27:23.91 +52:26:37.0 -- not a known variable star
08:27:56.28 +50:40:42.4 -- not a known variable star
08:28:16.57 +51:54:40.2 -- not a known variable star
08:28:27.72 +52:26:36.5 -- not a known variable star
08:28:55.29 +52:46:49.2 -- not a known variable star
08:29:00.74 +51:59:48.2 -- not a known variable star
08:29:06.02 +50:27:08.2 -- not a known variable star
08:29:11.10 +52:20:44.7 -- not a known variable star
08:29:30.29 +52:42:36.3 -- not a known variable star
08:29:35.69 +50:46:26.4 -- not a known variable star
08:29:53.95 +52:11:45.2 -- not a known variable star
08:29:58.98 +52:39:36.2 -- not a known variable star
08:30:03.09 +52:51:45.9 -- not a known variable star
08:30:07.81 +51:31:28.6 -- not a known variable star
08:30:15.42 +51:18:45.9 -- not a known variable star
08:30:26.59 +50:48:42.7 -- not a known variable star
08:30:35.78 +52:40:01.8 -- not a known variable star
08:31:03.57 +52:28:11.3 -- not a known variable star
08:31:04.65 +52:33:39.0 -- not a known variable star
08:31:24.58 +53:21:19.4 -- not a known variable star
Found 423 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
456 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 456 (excluding asteroids and hot pixels, 423 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
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461199.68004350 -observatory V36
06:43:39.87 +25:00:12.8 Mercury (0.1mag)
07:42:47.62 +23:22:54.5 Venus (-4.0mag)
02:49:34.48 +15:42:40.9 Mars (1.3mag)
07:48:25.65 +21:31:28.6 Jupiter (-1.9mag)
00:49:22.25 +02:48:39.8 Saturn (0.9mag)
04:00:12.24 +20:25:27.3 Uranus (5.8mag)
00:16:08.50 +00:16:48.1 Neptune (7.8mag)
20:33:21.44 -23:04:32.5 Pluto (14.5mag)
23:02:42.66 -05:43:33.1 Moon (-10.4mag)
-rw-r--r-- 1 apache apache 362 Jun 7 23:27 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461199.68004350:
07:48:26.44 +21:31:28.5 Io (6.0mag)
07:48:25.77 +21:31:30.5 Europa (6.2mag)
07:48:09.74 +21:32:16.0 Ganymede (5.6mag)
07:48:44.34 +21:30:28.3 Callisto (6.7mag)
07:48:43.05 +21:07:46.2 Himalia (15.6mag)
07:48:30.30 +21:31:14.3 Thebe (16.5mag)
07:48:42.51 +21:23:13.1 Elara (17.5mag)
07:50:36.31 +21:43:10.9 Pasiphae (17.7mag)
07:55:00.77 +21:33:11.0 Carme (18.9mag)
00:49:12.80 +02:48:38.6 Titan (8.7mag)
00:49:19.20 +02:48:52.9 Rhea (9.9mag)
00:49:54.53 +02:50:49.1 Iapetus (11.3mag)
00:49:18.19 +02:48:16.7 Hyperion (14.7mag)
00:50:04.52 +02:50:36.4 Phoebe (16.7mag)
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461199.68004350:
17:26:42.30 -35:15:05.7 JWST
14:33:32.04 +57:23:05.9 Chandra
18:39:30.90 -22:05:02.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Jun 7 23:27 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461199.68004350 -observatory V36
18:43:31.26 -32:39:10.8 13.6mag P/2010 H2 (Vales)
05:53:27.40 -68:03:51.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:49:03.24 +31:58:04.2 17.5mag C/2017 K2 (PANSTARRS)
17:14:44.30 +15:21:04.4 17.8mag C/2021 G2 (ATLAS)
21:12:08.99 -49:29:44.8 16.9mag P/2021 N1 (ZTF)
23:12:38.22 +31:35:29.4 17.2mag C/2022 E2 (ATLAS)
05:34:01.47 +26:58:31.6 16.5mag C/2022 N2 (PANSTARRS)
09:29:43.04 +31:04:59.4 16.6mag C/2022 QE78 (ATLAS)
08:50:32.29 +03:55:52.6 17.7mag C/2022 R6 (PANSTARRS)
18:28:13.91 +21:36:07.6 17.8mag C/2023 A3 (Tsuchinshan-ATLAS)
15:19:22.71 -11:00:31.0 17.6mag P/2023 B1 (PANSTARRS)
22:14:26.23 +66:31:39.8 17.7mag C/2023 H5 (Lemmon)
17:46:25.40 -06:41:16.2 13.7mag C/2023 R1 (PANSTARRS)
13:18:06.21 +82:59:48.1 17.9mag C/2023 X2 (Lemmon)
07:10:23.65 +64:18:31.0 17.7mag C/2024 A1 (ATLAS)
06:47:14.94 +27:49:58.9 13.6mag C/2024 E1 (Wierzchos)
15:37:18.03 +13:31:30.6 17.4mag C/2024 G6 (ATLAS)
20:13:03.35 +31:07:51.9 14.0mag C/2024 J3 (ATLAS)
04:18:00.68 -15:57:08.3 16.0mag C/2024 T5 (ATLAS)
06:05:53.86 +34:29:38.6 17.9mag C/2025 J1 (Borisov)
11:34:54.74 +52:44:59.9 17.4mag C/2025 L1 (ATLAS)
06:44:55.50 -10:52:08.8 14.1mag C/2025 R3 (PANSTARRS)
09:24:08.98 +23:20:24.8 17.9mag C/2025 V2 (Rankin)
12:39:42.10 +04:41:28.0 17.2mag C/2025 Y1 (ATLAS)
18:12:54.62 +75:07:45.3 17.9mag C/2026 A2 (Bok)
02:00:38.40 +43:24:51.3 16.1mag C/2026 B2 (Sun-Gao)
11:11:18.55 -03:44:18.3 16.5mag A/2026 E1
20:23:37.46 -08:34:06.6 8.7mag 10P/Tempel
11:02:00.11 -00:58:04.0 16.0mag 29P/Schwassmann-Wachmann
03:11:41.89 +25:38:37.5 17.7mag 47P/Ashbrook-Jackson
08:59:56.92 +23:46:24.0 16.9mag 63P/Wild
00:26:54.88 -06:22:06.3 15.7mag 65P/Gunn
06:43:23.56 +33:25:42.9 16.9mag 76P/West-Kohoutek-Ikemura
03:09:08.74 +17:12:53.3 13.8mag 78P/Gehrels
01:20:43.63 +04:50:46.2 15.6mag 88P/Howell
04:54:35.59 +30:18:07.1 15.2mag 93P/Lovas
02:42:54.54 +27:37:25.5 17.6mag 114P/Wiseman-Skiff
06:50:30.75 +33:02:19.6 15.6mag 123P/West-Hartley
09:50:09.21 +14:38:37.5 16.5mag 124P/Mrkos
03:59:00.67 +19:14:58.2 16.4mag 128P/Shoemaker-Holt
04:33:32.06 +19:05:01.9 17.7mag 131P/Mueller
05:58:14.91 +18:40:01.5 14.6mag 141P/Machholz
06:00:53.10 +17:40:28.4 14.6mag 141P-A/Machholz
04:54:00.99 +16:10:18.2 11.6mag 141P-D/Machholz
02:57:40.06 -24:42:05.7 16.8mag 161P/Hartley-IRAS
03:41:29.92 +23:48:13.5 14.9mag 162P/SidingSpring
19:36:38.21 +01:43:29.9 16.9mag 169P/NEAT
00:18:17.80 +02:27:45.1 17.9mag 220P/McNaught
16:52:11.67 -08:28:35.5 16.4mag 235P/LINEAR
07:34:37.42 +35:29:33.2 17.5mag 240P/NEAT
00:32:18.73 -02:28:31.1 16.4mag 260P/McNaught
04:04:11.07 +32:28:42.2 17.6mag 295P/LINEAR
23:52:09.61 -09:43:44.5 17.6mag 320P/McNaught
15:15:14.70 +08:06:01.2 17.4mag 391P/Kowalski
08:07:07.50 +20:44:52.0 17.9mag 450P/LONEOS
06:59:56.91 +41:41:51.3 17.8mag 493P/LONEOS
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:32.95 -68:48:30.00 ASASSN-26no 2026-05-24 8.41
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
15:16:06.61 -79:16:32.40 ASASSN-26dm 2026-05-19.03 14.44
11:24:25.21 -59:23:19.10 ASASSN-26dl 2026-05-18.02 13.55
13:45:51.52 -53:16:01.00 ASASSN-26dk 2026-05-18.16 12.96
02:05:49.69 -30:29:09.60 ASASSN-26dh 2026-05-18.43 15.37
17:50:22.87 -39:42:33.90 ASASSN-26dj 2026-05-17.05 15.7
01:13:11.60 -33:25:16.10 ASASSN-26dg 2026-05-13.41 16.8
16:44:31.77 -27:15:18.40 AT2026mhn 2026-05-12.33 15.8
09:46:31.08 -33:41:51.00 ASASSN-26di 2026-05-12.14 14.63
21:23:11.57 -19:09:45.00 AT2026kwu 2026-05-12.26 16.9
14:20:14.30 -30:20:51.90 AT2026ktm 2026-05-12.06 17.21
14:41:39.01 -37:13:46.40 AT2026lkm 2026-05-11.18 16.89
12:59:50.45 -10:58:38.80 SN2026kep 2026-05-9.06 17.5
13:37:29.61 -29:50:30.90 AT2026lkd 2026-05-9.09 17.23
09:46:42.01 -14:52:03.60 SN2026kmo 2026-05-8.99 17.51
15:03:05.28 +22:02:03.40 AT2026lxf 2026-05-8.07 13.88
10:23:49.41 -20:57:25.30 ASASSN-26df 2026-05-8.21 16.52
22:14:40.56 +05:04:51.60 2026lda 2026-05-7.56 16.2
21:35:33.81 -14:05:16.30 ASASSN-26de 2026-05-6.29 14.51
16:21:48.82 -61:36:13.20 ASASSN-26dd 2026-05-5.21 15.15
14:26:40.22 -24:48:37.50 AT2026lig 2026-05-4.27 14.63
13:17:51.04 +30:25:13.50 SN2026kcp 2026-05-4.46 16.43
11:27:55.57 -13:38:56.90 SN2026kza 2026-05-1.08 15.59
22:28:27.10 +30:17:54.30 SN 2026fov 2026-04-29.6 14.36
21:00:10.71 -32:17:03.90 AT2026kis 2026-04-27.36 16.15
14:32:57.37 -58:13:26.40 ASASSN-26dc 2026-04-27.27 13.42
15:32:05.35 -43:54:34.60 ASASSN-26db 2026-04-27.37 16.06
16:34:34.97 -54:34:58.00 ASASSN-26da 2026-04-25.32 16.11
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
20:07:38.15 -21:07:05.40 2026-05-25.18 -1.12
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
21:14:03.38 +56:46:44.1 TCP J21140338+5646441 2026-05-05.3534 16.7mag
15:03:05.19 +22:02:04.1 TCP J15030519+2202041 2026-05-08.3260 13.9mag
07:15:18.25 +47:53:16.7 TCP J07151825+4753167 2026-05-09.1599 14.4mag
16:00:18.44 -22:30:10.6 TCP J16001844-2230106 2026-05-09.6135 13.3mag
00:42:47.45 +41:16:58.5 PNV J00424745+4116585 2026-05-10.030 16.8mag
09:55:02.89 +69:02:13.8 PNV J09550289+6902138 2026-05-18.925 20.7mag
00:43:01.82 +41:18:16.6 PNV J00430182+4118166 2026-05-21.8651 18.83Cmag
00:42:51.20 +41:16:59.4 PNV J00425120+4116594 2022-10-26.135 19.3mag
12:24:25.10 +28:47:12.0 TCP J12242510+2847120 2026-05-31.6015 14.8mag
00:56:07.13 +43:01:40.6 TCP J00560713+4301406 2026-06-01.4135 12.2mag
00:42:41.64 +41:15:16.2 PNV J00424164+4115162 2026-06-02.029 17.4mag
00:42:38.68 +41:15:58.2 PNV J00423868+4115582 2026-06-05.1224 19.97Umag
19:00:42.95 -48:31:01.7 PNV J19004295-4831017 2026-05-25.0752 14.2mag
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:39:35.110 +15:17:58.28 AT 2026nsc 2026-05-09.80 20.76
16:42:48.680 +20:27:18.30 AT 2026nsb 2026-05-09.80 20.54
13:34:03.440 +31:37:31.73 AT 2026nsa 2026-05-07.80 21.26
13:50:28.150 +02:34:54.72 AT 2026nrz 2026-05-22.72 21.54
13:43:59.750 +03:47:21.63 AT 2026nry 2026-05-22.69 22.05
13:17:26.150 -01:26:00.12 AT 2026nrx 2026-05-21.64 21.7
00:35:20.216 -08:28:38.64 AT 2026nrw 2026-05-19.42 18.74
23:50:43.016 -01:09:12.25 AT 2026nrv 2026-05-23.48 19.5028
22:36:47.715 +37:31:34.81 AT 2026nru 2026-05-22.43 19.4626
23:58:04.247 +20:56:44.66 AT 2026nrt 2026-05-23.48 20.1237
16:08:58.229 +36:53:23.76 AT 2026nrs 2026-05-21.36 20.3819
19:44:04.734 +84:44:44.91 SN 2026nrr 2026-05-25.47 17.808
21:42:24.388 -20:21:08.51 SN 2026nrq 2026-05-25.56 18.623
22:03:20.669 -84:55:27.45 AT 2026nrp 2026-05-22.30 19.244
23:07:53.376 -39:04:26.84 AT 2026nro 2026-05-22.38 19.567
00:40:07.848 -39:10:21.32 AT 2026nrn 2026-05-12.41 18.737
23:05:28.381 -21:25:50.28 AT 2026nrm 2026-05-25.58 18.887
19:27:28.750 -48:42:52.35 AT 2026nrl 2026-05-22.24 19.107
12:33:38.422 +12:02:05.88 AT 2026nrk 2026-05-25.29 21.322
12:32:27.199 +02:39:54.51 AT 2026nrj 2026-05-25.29 21.0728
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