This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p
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 09 17.3978 2461300.8978 10.82 04:57:49.20 +34:05:02.5
169.97156 -5.45694 galactic Aur Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 161001144057864320 | 04:57:49.17 +34:05:02.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.383+/-0.022 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:49.20 +34:05:02.5: 11.81 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:49.20 +34:05:02.5: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 161001144057864320,2461300.8978,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 161001144057864320 20260917.3978 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 10.83 04:58:58.72 +36:01:58.3
168.58007 -4.06721 galactic Aur Second-epoch detections are separated by 0.1" and 7.2 pix
The object was found in VSX 2" Gaia DR3 186207860442334464
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.740 G 11.760 G A
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:58.72 +36:01:58.3: 11.83 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:58.72 +36:01:58.3: 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 186207860442334464,2461300.8978,10.83,0.05,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 186207860442334464 20260917.3978 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 09 17.3978 2461300.8978 10.94 04:59:28.28 +36:27:44.1
168.30265 -3.72423 galactic Aur Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.8677+36.4623 | 04:59:28.25 +36:27:44.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.026 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:28.28 +36:27:44.1: 11.84 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:28.28 +36:27:44.1: 11.80 +/- 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 J074.8677+36.4623,2461300.8978,10.94,0.05,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 J074.8677+36.4623 20260917.3978 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 09 17.3978 2461300.8978 10.90 04:59:24.43 +36:06:11.1
168.57817 -3.95574 galactic Aur Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186231229361784704 | 04:59:24.40 +36:06:11.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.261+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:24.43 +36:06:11.1: 11.89 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:24.43 +36:06:11.1: 11.85 +/- 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 186231229361784704,2461300.8978,10.90,0.05,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 186231229361784704 20260917.3978 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 09 17.3978 2461300.8978 10.93 04:57:29.96 +34:29:10.1
169.61299 -5.26040 galactic Aur Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185791905746199808 | 04:57:30.00 +34:29:09.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.874+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:29.96 +34:29:10.1: 11.97 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:29.96 +34:29:10.1: 11.95 +/- 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 185791905746199808,2461300.8978,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 185791905746199808 20260917.3978 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 9.68 04:58:32.07 +35:00:45.8
169.32929 -4.76782 galactic Aur Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.6407+35.0029 | 04:58:32.09 +35:00:45.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 1949AnHar.112....1C HD 280327 J-Ks=0.641+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:32.07 +35:00:45.8: 10.63 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:32.07 +35:00:45.8: 10.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.61 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.6407+35.0029,2461300.8978,9.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.6407+35.0029 20260917.3978 9.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 11.03 04:59:06.07 +36:04:21.6
168.56398 -4.02316 galactic Aur Second-epoch detections are separated by 0.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186208032241024512 | 04:59:06.03 +36:04:21.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.208+/-0.029 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:06.07 +36:04:21.6: 12.05 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:06.07 +36:04:21.6: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186208032241024512,2461300.8978,11.03,0.05,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 186208032241024512 20260917.3978 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 09 17.3978 2461300.8978 11.03 04:56:48.20 +34:47:38.9
169.28117 -5.18190 galactic Aur Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185847534162582656 | 04:56:48.27 +34:47:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.211+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:48.20 +34:47:38.9: 12.13 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:48.20 +34:47:38.9: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185847534162582656,2461300.8978,11.03,0.05,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 185847534162582656 20260917.3978 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 09 17.3978 2461300.8978 10.13 04:56:41.63 +34:38:39.5
169.38513 -5.29253 galactic Aur Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185844269987467904 | 04:56:41.59 +34:38:40.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3 1949AnHar.112....1C HD 280266 J-Ks=0.192+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:41.63 +34:38:39.5: 11.12 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:41.63 +34:38:39.5: 11.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185844269987467904,2461300.8978,10.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 185844269987467904 20260917.3978 10.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 11.35 04:55:28.70 +35:21:46.5
168.66478 -5.04020 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186081523981444480 | 04:55:28.71 +35:21:46.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.471+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:28.70 +35:21:46.5: 12.27 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:28.70 +35:21:46.5: 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 186081523981444480,2461300.8978,11.35,0.05,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 186081523981444480 20260917.3978 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 09 17.3978 2461300.8978 11.36 04:59:26.11 +36:32:16.1
168.23854 -3.68339 galactic Aur Second-epoch detections are separated by 0.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.8490+36.5375 | 04:59:26.12 +36:32:16.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.219+/-0.035 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:26.11 +36:32:16.1: 12.27 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:26.11 +36:32:16.1: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.8490+36.5375,2461300.8978,11.36,0.05,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
ATO J074.8490+36.5375 20260917.3978 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 09 17.3978 2461300.8978 11.33 04:56:32.96 +34:57:09.3
169.12398 -5.12436 galactic Aur Second-epoch detections are separated by 1.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1451+34.9539 | 04:56:32.97 +34:57:09.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.526+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:32.96 +34:57:09.3: 12.29 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:32.96 +34:57:09.3: 12.24 +/- 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
ATO J074.1451+34.9539,2461300.8978,11.33,0.05,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 J074.1451+34.9539 20260917.3978 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 09 17.3978 2461300.8978 10.59 04:58:54.48 +35:09:37.5
169.25993 -4.61658 galactic Aur Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185887872496487168 | 04:58:54.51 +35:09:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1949AnHar.112....1C HD 280326 J-Ks=0.412+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:54.48 +35:09:37.5: 11.47 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:54.48 +35:09:37.5: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185887872496487168,2461300.8978,10.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 185887872496487168 20260917.3978 10.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 10.64 04:58:46.97 +36:01:10.5
168.56605 -4.10655 galactic Aur Second-epoch detections are separated by 0.2" and 7.3 pix
The object was found in VSX 0" Gaia DR3 186206627789143040
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.400 G 11.430 G B
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:46.97 +36:01:10.5: 11.59 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:46.97 +36:01:10.5: 11.61 +/- 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
Gaia DR3 186206627789143040,2461300.8978,10.64,0.05,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 186206627789143040 20260917.3978 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 09 17.3978 2461300.8978 10.75 04:58:10.21 +35:05:57.4
169.21477 -4.77301 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5465+35.0975 | 04:58:10.13 +35:05:58.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.494+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:10.21 +35:05:57.4: 11.66 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:10.21 +35:05:57.4: 11.67 +/- 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
ATO J074.5465+35.0975,2461300.8978,10.75,0.05,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 J074.5465+35.0975 20260917.3978 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 09 17.3978 2461300.8978 10.54 04:58:44.55 +35:38:54.9
168.85365 -4.34201 galactic Aur Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186004214569725440 | 04:58:44.58 +35:38:54.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.814+/-0.037 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:44.55 +35:38:54.9: 11.63 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:44.55 +35:38:54.9: 11.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 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 186004214569725440,2461300.8978,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 186004214569725440 20260917.3978 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 11.32 04:57:45.33 +34:48:49.7
169.38725 -5.01629 galactic Aur Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185806229460829056 | 04:57:45.41 +34:48:49.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.990+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:45.33 +34:48:49.7: 12.41 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:45.33 +34:48:49.7: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185806229460829056,2461300.8978,11.32,0.05,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 185806229460829056 20260917.3978 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 09 17.3978 2461300.8978 11.34 04:56:15.55 +34:41:28.6
169.29240 -5.33340 galactic Aur Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 161829110674615296 | 04:56:15.52 +34:41:28.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.407+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:15.55 +34:41:28.6: 12.42 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:15.55 +34:41:28.6: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 161829110674615296,2461300.8978,11.34,0.05,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 161829110674615296 20260917.3978 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 09 17.3978 2461300.8978 11.31 04:58:17.10 +35:42:22.3
168.75066 -4.37948 galactic Aur Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5711+35.7063 | 04:58:17.07 +35:42:22.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.651+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:17.10 +35:42:22.3: 12.38 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:17.10 +35:42:22.3: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.5711+35.7063,2461300.8978,11.31,0.05,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 J074.5711+35.7063 20260917.3978 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 09 17.3978 2461300.8978 11.32 04:58:13.23 +34:27:21.1
169.72913 -5.16226 galactic Aur Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185780253497666560 | 04:58:13.14 +34:27:22.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.316+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:13.23 +34:27:21.1: 12.36 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:13.23 +34:27:21.1: 12.33 +/- 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 185780253497666560,2461300.8978,11.32,0.05,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 185780253497666560 20260917.3978 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 09 17.3978 2461300.8978 11.25 04:58:57.30 +35:34:06.9
168.94352 -4.35737 galactic Aur Second-epoch detections are separated by 0.7" and 7.3 pix
The object was found in VSX 1" Gaia DR3 186002801525366528
Type: ROT
# Max. Min./Amp. JD0 Period
12.020 G 12.050 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:57.30 +35:34:06.9: 12.31 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:57.30 +35:34:06.9: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186002801525366528,2461300.8978,11.25,0.05,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 186002801525366528 20260917.3978 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 09 17.3978 2461300.8978 11.19 04:58:17.59 +35:59:57.3
168.52072 -4.19698 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX 2" ASASSN-V J045817.69+355956.1
Type: SR
# Max. Min./Amp. JD0 Period
13.760 g Y 0.190 g 2458819.88900 174.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:17.59 +35:59:57.3: 12.27 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:17.59 +35:59:57.3: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045817.69+355956.1,2461300.8978,11.19,0.05,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
ASASSN-V J045817.69+355956.1 20260917.3978 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 09 17.3978 2461300.8978 10.35 04:58:01.44 +34:22:45.0
169.76459 -5.24149 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5184+34.3784 | 04:58:01.39 +34:22:46.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 1949AnHar.112....1C HD 280271 J-Ks=0.508+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:01.44 +34:22:45.0: 11.30 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:01.44 +34:22:45.0: 11.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.5184+34.3784,2461300.8978,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.5184+34.3784 20260917.3978 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 11.21 04:57:06.67 +34:24:03.2
169.63046 -5.37602 galactic Aur Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 161772039147942016 | 04:57:06.66 +34:24:03.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0/2 2015MNRAS.449.1401H LAMOST J045706.66+342403.0 J-Ks=0.273+/-0.024 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:06.67 +34:24:03.2: 12.22 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:06.67 +34:24:03.2: 12.26 +/- 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 161772039147942016,2461300.8978,11.21,0.05,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 161772039147942016 20260917.3978 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 09 17.3978 2461300.8978 11.21 04:55:37.36 +34:47:51.6
169.12703 -5.36953 galactic Aur Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 161843232527081984 | 04:55:37.34 +34:47:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.418+/-0.023 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:37.36 +34:47:51.6: 12.17 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:37.36 +34:47:51.6: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 161843232527081984,2461300.8978,11.21,0.05,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 161843232527081984 20260917.3978 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 09 17.3978 2461300.8978 9.99 04:58:38.72 +34:53:44.6
169.43576 -4.82213 galactic Aur Second-epoch detections are separated by 0.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185827880393322112 | 04:58:38.71 +34:53:45.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1949AnHar.112....1C HD 280328 J-Ks=0.376+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:38.72 +34:53:44.6: 11.00 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:38.72 +34:53:44.6: 10.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.00 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185827880393322112,2461300.8978,9.99,0.05,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 185827880393322112 20260917.3978 9.99CV 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 09 17.3978 2461300.8978 11.15 04:57:19.27 +35:40:25.1
168.65474 -4.55331 galactic Aur Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186104025313178240 | 04:57:19.31 +35:40:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.265+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:19.27 +35:40:25.1: 12.06 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:19.27 +35:40:25.1: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186104025313178240,2461300.8978,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 186104025313178240 20260917.3978 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 11.11 04:54:46.89 +35:30:30.4
168.46169 -5.06012 galactic Aur Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186087257759814784 | 04:54:46.90 +35:30:30.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.560+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:46.89 +35:30:30.4: 12.05 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:46.89 +35:30:30.4: 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 186087257759814784,2461300.8978,11.11,0.05,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 186087257759814784 20260917.3978 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 09 17.3978 2461300.8978 10.97 04:57:52.38 +34:17:23.0
169.81589 -5.32125 galactic Aur Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4747+34.2913 | 04:57:52.34 +34:17:23.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.431+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:52.38 +34:17:23.0: 12.01 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:52.38 +34:17:23.0: 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
ATO J074.4747+34.2913,2461300.8978,10.97,0.05,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 J074.4747+34.2913 20260917.3978 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 09 17.3978 2461300.8978 10.97 04:58:41.44 +35:58:36.6
168.58822 -4.14762 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.6800+35.9811 | 04:58:41.43 +35:58:36.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.405+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:41.44 +35:58:36.6: 12.00 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:41.44 +35:58:36.6: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.6800+35.9811,2461300.8978,10.97,0.05,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 J074.6800+35.9811 20260917.3978 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 09 17.3978 2461300.8978 10.84 04:58:34.50 +35:00:37.5
169.33625 -4.76271 galactic Aur Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.6407+35.0029 | 04:58:32.09 +35:00:45.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 1949AnHar.112....1C HD 280327 J-Ks=1.289+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:34.50 +35:00:37.5: 11.92 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:34.50 +35:00:37.5: 11.88 +/- 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 J074.6407+35.0029,2461300.8978,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.6407+35.0029 20260917.3978 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 10.93 04:56:26.04 +34:37:19.7
169.36925 -5.34819 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 161825709060519552 | 04:56:26.05 +34:37:17.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A 1949AnHar.112....1C HD 280267 J-Ks=0.220+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:26.04 +34:37:19.7: 12.04 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:26.04 +34:37:19.7: 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 161825709060519552,2461300.8978,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 161825709060519552 20260917.3978 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 10.91 04:58:04.74 +35:44:00.0
168.70333 -4.39556 galactic Aur Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186196010630044288 | 04:58:04.73 +35:44:00.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: kA1mA6 2015MNRAS.449.1401H LAMOST J045804.72+354359.8 J-Ks=0.407+/-0.024 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:04.74 +35:44:00.0: 11.88 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:04.74 +35:44:00.0: 11.86 +/- 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 186196010630044288,2461300.8978,10.91,0.05,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 186196010630044288 20260917.3978 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 09 17.3978 2461300.8978 10.75 04:58:56.05 +35:05:23.5
169.31898 -4.65586 galactic Aur Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185834683620315776 | 04:58:56.11 +35:05:23.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.878+/-0.034 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:56.05 +35:05:23.5: 11.74 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:56.05 +35:05:23.5: 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 185834683620315776,2461300.8978,10.75,0.05,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 185834683620315776 20260917.3978 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 09 17.3978 2461300.8978 13.12 04:57:05.54 +36:01:50.9
168.34497 -4.36799 galactic Aur Second-epoch detections are separated by 1.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.2702+36.0187 | 04:57:05.54 +36:01:50.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.869+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:05.54 +36:01:50.9: 14.05 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:05.54 +36:01:50.9: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.11 +/- 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
ATO J074.2702+36.0187,2461300.8978,13.12,0.05,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
ATO J074.2702+36.0187 20260917.3978 13.12CV 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 09 17.3978 2461300.8978 13.07 04:54:47.51 +35:13:42.7
168.68232 -5.23353 galactic Aur Second-epoch detections are separated by 1.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:47.51 +35:13:42.7 (user input) | T | P | (position from user input) J-Ks=0.581+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:47.51 +35:13:42.7: 14.22 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:47.51 +35:13:42.7: 14.17 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 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,2461300.8978,13.07,0.05,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 20260917.3978 13.07CV 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 09 17.3978 2461300.8978 11.01 04:59:34.00 +36:43:33.1
168.10644 -3.54671 galactic Aur Second-epoch detections are separated by 0.2" and 7.1 pix
The object was found in VSX 3" Gaia DR3 186265550442204544
Type: ROT
# Max. Min./Amp. JD0 Period
11.760 G 11.790 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:34.00 +36:43:33.1: 11.87 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:34.00 +36:43:33.1: 11.90 +/- 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 186265550442204544,2461300.8978,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 186265550442204544 20260917.3978 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.99 04:58:07.35 +35:57:00.8
168.53793 -4.25443 galactic Aur Second-epoch detections are separated by 2.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5361+35.9540 | 04:58:07.35 +35:57:00.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.867+/-0.029 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:07.35 +35:57:00.8: 14.22 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:07.35 +35:57:00.8: 14.44 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.5361+35.9540,2461300.8978,12.99,0.05,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
ATO J074.5361+35.9540 20260917.3978 12.99CV 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 09 17.3978 2461300.8978 12.98 04:59:20.50 +36:02:23.8
168.61985 -4.00507 galactic Aur Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186207521142323200 | 04:59:16.87 +36:02:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: em? 1983VatOP...2...73C VES 856 J-Ks=0.682+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:20.50 +36:02:23.8: 14.24 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:20.50 +36:02:23.8: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.21 +/- 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
Gaia DR3 186207521142323200,2461300.8978,12.98,0.05,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 186207521142323200 20260917.3978 12.98CV 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 09 17.3978 2461300.8978 12.98 04:57:45.98 +34:01:46.9
170.00759 -5.49925 galactic Aur Second-epoch detections are separated by 2.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4419+34.0277 | 04:57:45.98 +34:01:46.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.252+/-0.030 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:45.98 +34:01:46.9: 14.32 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:45.98 +34:01:46.9: 14.25 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.28 +/- 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
ATO J074.4419+34.0277,2461300.8978,12.98,0.05,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
ATO J074.4419+34.0277 20260917.3978 12.98CV 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 09 17.3978 2461300.8978 13.19 04:58:55.62 +35:39:57.6
168.86310 -4.30177 galactic Aur Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:55.62 +35:39:57.6 (user input) | T | P | (position from user input) J-Ks=0.354+/-0.031 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:55.62 +35:39:57.6: 14.32 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:55.62 +35:39:57.6: 14.39 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.19CV 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 09 17.3978 2461300.8978 13.04 04:57:12.09 +34:36:17.8
169.48117 -5.23500 galactic Aur Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:12.09 +34:36:17.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:12.09 +34:36:17.8: 14.26 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:12.09 +34:36:17.8: 14.28 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.04CV 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 09 17.3978 2461300.8978 11.67 04:59:15.41 +36:42:37.9
168.08018 -3.60505 galactic Aur Second-epoch detections are separated by 0.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186265344283775744 | 04:59:15.38 +36:42:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.392+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:15.41 +36:42:37.9: 12.55 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:15.41 +36:42:37.9: 12.52 +/- 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 186265344283775744,2461300.8978,11.67,0.05,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
Gaia DR3 186265344283775744 20260917.3978 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 09 17.3978 2461300.8978 11.46 04:59:16.83 +36:02:12.4
168.61471 -4.01676 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186207521142323200 | 04:59:16.87 +36:02:12.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: em? 1983VatOP...2...73C VES 856 J-Ks=0.297+/-0.029 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:16.83 +36:02:12.4: 12.57 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:16.83 +36:02:12.4: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186207521142323200,2461300.8978,11.46,0.05,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 186207521142323200 20260917.3978 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 09 17.3978 2461300.8978 11.76 04:55:57.17 +34:25:54.0
169.45725 -5.54421 galactic Aur Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:57.17 +34:25:54.0 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.428+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:57.17 +34:25:54.0: 12.83 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:57.17 +34:25:54.0: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,11.76,0.05,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 20260917.3978 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 09 17.3978 2461300.8978 13.12 04:57:58.76 +34:32:19.6
169.63284 -5.15014 galactic Aur Second-epoch detections are separated by 3.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:58.76 +34:32:19.6 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.416+/-0.033 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:58.76 +34:32:19.6: 14.56 +/- 0.10 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:58.76 +34:32:19.6: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.12CV 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 09 17.3978 2461300.8978 11.82 04:58:49.84 +36:07:08.1
168.49369 -4.03762 galactic Aur Second-epoch detections are separated by 0.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.7077+36.1187 | 04:58:49.84 +36:07:08.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.582+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:49.84 +36:07:08.1: 12.89 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:49.84 +36:07:08.1: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 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
ATO J074.7077+36.1187,2461300.8978,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.7077+36.1187 20260917.3978 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 11.78 04:59:29.06 +35:55:19.3
168.73079 -4.05497 galactic Aur Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:29.06 +35:55:19.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.482+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:29.06 +35:55:19.3: 12.96 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:29.06 +35:55:19.3: 12.94 +/- 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,2461300.8978,11.78,0.05,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 20260917.3978 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 09 17.3978 2461300.8978 13.10 04:56:39.45 +34:40:25.2
169.35735 -5.28016 galactic Aur Second-epoch detections are separated by 2.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:39.45 +34:40:25.2 (user input) | T | P | (position from user input) J-Ks=0.558+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:39.45 +34:40:25.2: 14.53 +/- 0.11 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:39.45 +34:40:25.2: 14.43 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.10CV 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 09 17.3978 2461300.8978 12.12 04:54:48.66 +35:39:42.8
168.34528 -4.95945 galactic Aur Second-epoch detections are separated by 0.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:48.66 +35:39:42.8 (user input) | T | P | (position from user input) J-Ks=0.502+/-0.025 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:48.66 +35:39:42.8: 13.10 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:48.66 +35:39:42.8: 13.12 +/- 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,2461300.8978,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.12CV 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 09 17.3978 2461300.8978 12.47 05:00:03.85 +36:50:48.8
168.07235 -3.39370 galactic Aur Second-epoch detections are separated by 2.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 186643202624995840 | 05:00:03.85 +36:50:48.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.270+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:03.85 +36:50:48.8: 13.42 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:03.85 +36:50:48.8: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 186643202624995840,2461300.8978,12.47,0.05,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
Large-amplitude variable Gaia DR2 186643202624995840 20260917.3978 12.47CV 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 09 17.3978 2461300.8978 12.38 05:00:00.55 +36:34:56.6
168.27446 -3.56512 galactic Aur Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:00:00.55 +36:34:56.6 (user input) | T | P | (position from user input) J-Ks=0.459+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:00.55 +36:34:56.6: 13.46 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:00.55 +36:34:56.6: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.38,0.05,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 20260917.3978 12.38CV 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 09 17.3978 2461300.8978 12.41 04:57:18.59 +34:16:18.5
169.75778 -5.42376 galactic Aur Second-epoch detections are separated by 0.5" and 7.5 pix
The object was found in VSX 1" Gaia DR3 161758299549843328
Type: RS
# Max. Min./Amp. JD0 Period
13.240 G 13.310 G G
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:18.59 +34:16:18.5: 13.58 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:18.59 +34:16:18.5: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 161758299549843328,2461300.8978,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 161758299549843328 20260917.3978 12.41CV 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 09 17.3978 2461300.8978 12.53 04:54:06.61 +35:51:03.9
168.10785 -4.95176 galactic Aur Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.5273+35.8508 | 04:54:06.61 +35:51:03.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.627+/-0.025 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:06.61 +35:51:03.9: 13.56 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:06.61 +35:51:03.9: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.5273+35.8508,2461300.8978,12.53,0.05,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
ATO J073.5273+35.8508 20260917.3978 12.53CV 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 09 17.3978 2461300.8978 12.46 04:58:26.58 +35:56:58.5
168.57866 -4.20386 galactic Aur Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:26.58 +35:56:58.5 (user input) | T | P | (position from user input) J-Ks=0.410+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:26.58 +35:56:58.5: 13.56 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:26.58 +35:56:58.5: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.46,0.05,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 20260917.3978 12.46CV 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 09 17.3978 2461300.8978 12.66 04:57:34.69 +36:05:34.4
168.35725 -4.25247 galactic Aur Second-epoch detections are separated by 1.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 186217107509367040 | 04:57:34.69 +36:05:34.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.960+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:34.69 +36:05:34.4: 13.61 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:34.69 +36:05:34.4: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 186217107509367040,2461300.8978,12.66,0.05,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
Large-amplitude variable Gaia DR2 186217107509367040 20260917.3978 12.66CV 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 09 17.3978 2461300.8978 12.48 04:58:03.19 +35:57:57.9
168.51673 -4.25564 galactic Aur Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:03.19 +35:57:57.9 (user input) | T | P | (position from user input) J-Ks=0.904+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:03.19 +35:57:57.9: 13.66 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:03.19 +35:57:57.9: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.48,0.05,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 20260917.3978 12.48CV 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 09 17.3978 2461300.8978 12.51 04:57:46.02 +33:33:36.5
170.37881 -5.78909 galactic Aur Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:46.02 +33:33:36.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.005+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:46.02 +33:33:36.5: 13.83 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:46.02 +33:33:36.5: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.51,0.05,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 20260917.3978 12.51CV 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 09 17.3978 2461300.8978 12.78 04:58:40.91 +35:31:39.2
168.94152 -4.42641 galactic Aur Second-epoch detections are separated by 0.8" and 7.4 pix
The object was found in VSX11" Gaia DR3 185908621482406912
Type: S
# Max. Min./Amp. JD0 Period
18.270 G 19.270 G
ATTENTION: measured mag 12.78 is 5.5 mag brighter than the VSX record maximum brightness 18.27 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:40.91 +35:31:39.2: 13.95 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:40.91 +35:31:39.2: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185908621482406912,2461300.8978,12.78,0.05,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 185908621482406912 20260917.3978 12.78CV 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 09 17.3978 2461300.8978 12.69 04:58:22.63 +34:23:43.3
169.79695 -5.17417 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.852 Wladilena -558 -41 559 14.5 -0 0
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:22.63 +34:23:43.3: 14.01 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:22.63 +34:23:43.3: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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
VARIABLE_NAME,2461300.8978,12.69,0.05,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
VARIABLE_NAME 20260917.3978 12.69CV 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 09 17.3978 2461300.8978 13.04 04:53:07.59 +35:48:44.0
168.01245 -5.13128 galactic Aur Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:53:07.59 +35:48:44.0 (user input) | T | P | (position from user input) J-Ks=0.908+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:07.59 +35:48:44.0: 14.05 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:07.59 +35:48:44.0: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461300.8978,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.04CV 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 09 17.3978 2461300.8978 12.96 04:58:37.99 +36:03:35.2
168.51562 -4.10553 galactic Aur Second-epoch detections are separated by 2.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:37.99 +36:03:35.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:37.99 +36:03:35.2: 14.02 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:37.99 +36:03:35.2: 14.11 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461300.8978,12.96,0.05,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
target 20260917.3978 12.96CV 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 09 17.3978 2461300.8978 13.04 04:53:35.12 +35:40:33.1
168.17768 -5.14463 galactic Aur Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.3902+35.6808 | 04:53:35.12 +35:40:33.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.970+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:35.12 +35:40:33.1: 14.03 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:35.12 +35:40:33.1: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 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
ATO J073.3902+35.6808,2461300.8978,13.04,0.05,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
ATO J073.3902+35.6808 20260917.3978 13.04CV 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 09 17.3978 2461300.8978 12.95 04:56:32.93 +35:40:53.4
168.55083 -4.67135 galactic Aur Second-epoch detections are separated by 2.2" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:32.93 +35:40:53.4 (user input) | T | P | (position from user input) J-Ks=0.842+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:32.93 +35:40:53.4: 14.00 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:32.93 +35:40:53.4: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 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,2461300.8978,12.95,0.05,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 20260917.3978 12.95CV 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 09 17.3978 2461300.8978 12.92 04:59:55.75 +36:34:26.2
168.27123 -3.58297 galactic Aur Second-epoch detections are separated by 3.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:55.75 +36:34:26.2 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.031 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:55.75 +36:34:26.2: 14.00 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:55.75 +36:34:26.2: 14.04 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461300.8978,12.92,0.05,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
target 20260917.3978 12.92CV 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 09 17.3978 2461300.8978 12.70 04:58:48.20 +35:37:06.4
168.88509 -4.35088 galactic Aur Second-epoch detections are separated by 0.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:48.20 +35:37:06.4 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.526+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:48.20 +35:37:06.4: 14.02 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:48.20 +35:37:06.4: 14.08 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.05 +/- 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,2461300.8978,12.70,0.05,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 20260917.3978 12.70CV 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 09 17.3978 2461300.8978 12.70 04:57:22.48 +34:31:57.0
169.56046 -5.25187 galactic Aur Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:22.48 +34:31:57.0 (user input) | T | P | (position from user input) J-Ks=0.574+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:22.48 +34:31:57.0: 14.02 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:22.48 +34:31:57.0: 13.95 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 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,2461300.8978,12.70,0.05,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 20260917.3978 12.70CV 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 09 17.3978 2461300.8978 12.87 04:58:20.82 +35:32:50.8
168.88363 -4.46770 galactic Aur Second-epoch detections are separated by 4.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:20.82 +35:32:50.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.036+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:20.82 +35:32:50.8: 14.01 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:20.82 +35:32:50.8: 13.91 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 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,2461300.8978,12.87,0.05,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 20260917.3978 12.87CV 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 09 17.3978 2461300.8978 13.07 04:53:57.39 +35:32:17.9
168.33274 -5.17226 galactic Aur Second-epoch detections are separated by 2.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:53:57.39 +35:32:17.9 (user input) | T | P | (position from user input) J-Ks=0.452+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:57.39 +35:32:17.9: 13.99 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:57.39 +35:32:17.9: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 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,2461300.8978,13.07,0.05,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 20260917.3978 13.07CV 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 09 17.3978 2461300.8978 12.81 04:58:29.87 +35:43:51.1
168.75799 -4.33028 galactic Aur Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:29.87 +35:43:51.1 (user input) | T | P | (position from user input) J-Ks=0.811+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:29.87 +35:43:51.1: 14.00 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:29.87 +35:43:51.1: 14.07 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461300.8978,12.81,0.05,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 20260917.3978 12.81CV 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 09 17.3978 2461300.8978 12.65 04:58:03.17 +34:04:34.7
170.00757 -5.42379 galactic Aur Second-epoch detections are separated by 3.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:03.17 +34:04:34.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.580+/-0.023 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:03.17 +34:04:34.7: 14.00 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:03.17 +34:04:34.7: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461300.8978,12.65,0.05,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 20260917.3978 12.65CV 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 09 17.3978 2461300.8978 13.07 04:54:23.13 +35:55:04.1
168.09078 -4.86648 galactic Aur Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.5948+35.9182 | 04:54:23.13 +35:55:04.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.071+/-0.035 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:23.13 +35:55:04.1: 14.00 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:23.13 +35:55:04.1: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 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
ATO J073.5948+35.9182,2461300.8978,13.07,0.05,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 J073.5948+35.9182 20260917.3978 13.07CV 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 09 17.3978 2461300.8978 12.88 04:57:15.52 +33:30:19.1
170.35637 -5.90627 galactic Aur Second-epoch detections are separated by 1.6" and 7.5 pix
The object was found in VSX17" Gaia DR3 160947164911016960
Type: ROT
# Max. Min./Amp. JD0 Period
17.510 G 17.550 G 0.393632000000 F
ATTENTION: measured mag 12.88 is 4.6 mag brighter than the VSX record maximum brightness 17.51 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:15.52 +33:30:19.1: 13.99 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:15.52 +33:30:19.1: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 160947164911016960,2461300.8978,12.88,0.05,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 160947164911016960 20260917.3978 12.88CV 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 09 17.3978 2461300.8978 12.80 04:59:41.99 +36:09:44.3
168.56788 -3.87271 galactic Aur Second-epoch detections are separated by 2.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:41.99 +36:09:44.3 (user input) | T | P | (position from user input) J-Ks=0.378+/-0.032 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:41.99 +36:09:44.3: 14.00 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:41.99 +36:09:44.3: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 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,2461300.8978,12.80,0.05,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 20260917.3978 12.80CV 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 09 17.3978 2461300.8978 12.89 04:54:06.75 +35:13:44.2
168.59478 -5.34146 galactic Aur Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:06.75 +35:13:44.2 (user input) | T | P | (position from user input) J-Ks=1.276+/-0.025 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:06.75 +35:13:44.2: 13.98 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:06.75 +35:13:44.2: 13.99 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 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,2461300.8978,12.89,0.05,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 20260917.3978 12.89CV 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 09 17.3978 2461300.8978 12.82 04:59:57.92 +36:30:38.9
168.32558 -3.61609 galactic Aur Second-epoch detections are separated by 1.0" and 6.8 pix
The object was found in VSX23" ZTF J045958.51+363100.3
Type: EW:
# Max. Min./Amp. JD0 Period
18.969 r Y 0.206 r 2458362.93860 0.562378400000
ATTENTION: measured mag 12.82 is 5.9 mag brighter than the VSX record maximum brightness 18.76 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:57.92 +36:30:38.9: 14.00 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:57.92 +36:30:38.9: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.00 +/- 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
ZTF J045958.51+363100.3,2461300.8978,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J045958.51+363100.3 20260917.3978 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.89 04:56:11.07 +34:22:11.3
169.53578 -5.54524 galactic Aur Second-epoch detections are separated by 1.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:11.07 +34:22:11.3 (user input) | T | P | (position from user input) J-Ks=0.916+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:11.07 +34:22:11.3: 13.98 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:11.07 +34:22:11.3: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.97 +/- 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,2461300.8978,12.89,0.05,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 20260917.3978 12.89CV 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 09 17.3978 2461300.8978 12.84 04:55:03.48 +35:28:38.7
168.52132 -5.03559 galactic Aur Second-epoch detections are separated by 1.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:03.48 +35:28:38.7 (user input) | T | P | (position from user input) J-Ks=0.972+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:03.48 +35:28:38.7: 13.98 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:03.48 +35:28:38.7: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.99 +/- 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,2461300.8978,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.88 04:56:20.92 +36:00:20.6
168.27089 -4.50135 galactic Aur Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:20.92 +36:00:20.6 (user input) | T | P | (position from user input) J-Ks=1.008+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:20.92 +36:00:20.6: 13.95 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:20.92 +36:00:20.6: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 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,2461300.8978,12.88,0.05,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 20260917.3978 12.88CV 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 09 17.3978 2461300.8978 12.92 04:55:29.65 +35:39:50.3
168.43068 -4.84981 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.8754+35.6724 | 04:55:29.65 +35:39:50.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.970+/-0.025 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:29.65 +35:39:50.3: 13.99 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:29.65 +35:39:50.3: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 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
ATO J073.8754+35.6724,2461300.8978,12.92,0.05,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 J073.8754+35.6724 20260917.3978 12.92CV 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 09 17.3978 2461300.8978 12.77 04:58:01.58 +35:00:44.2
169.26515 -4.84992 galactic Aur Second-epoch detections are separated by 2.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:01.58 +35:00:44.2 (user input) | T | P | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.394+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:01.58 +35:00:44.2: 13.96 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:01.58 +35:00:44.2: 13.94 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 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,2461300.8978,12.77,0.05,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 20260917.3978 12.77CV 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 09 17.3978 2461300.8978 12.86 04:59:46.05 +36:36:46.7
168.22040 -3.58452 galactic Aur Second-epoch detections are separated by 2.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:46.05 +36:36:46.7 (user input) | T | P | (position from user input) J-Ks=0.862+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:46.05 +36:36:46.7: 13.95 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:46.05 +36:36:46.7: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 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,2461300.8978,12.86,0.05,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 20260917.3978 12.86CV 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 09 17.3978 2461300.8978 12.78 04:57:04.49 +34:46:04.7
169.33649 -5.15440 galactic Aur Second-epoch detections are separated by 0.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:04.49 +34:46:04.7 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:04.49 +34:46:04.7: 13.96 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:04.49 +34:46:04.7: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461300.8978,12.78,0.05,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 20260917.3978 12.78CV 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 09 17.3978 2461300.8978 12.74 04:58:08.36 +35:53:38.0
168.58442 -4.28661 galactic Aur Second-epoch detections are separated by 2.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:08.36 +35:53:38.0 (user input) | T | P | (position from user input) J-Ks=0.627+/-0.034 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:08.36 +35:53:38.0: 13.94 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:08.36 +35:53:38.0: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.97 +/- 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,2461300.8978,12.74,0.05,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 20260917.3978 12.74CV 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 09 17.3978 2461300.8978 12.82 04:58:37.61 +34:55:40.6
169.40796 -4.80524 galactic Aur Second-epoch detections are separated by 2.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:37.61 +34:55:40.6 (user input) | T | P | (position from user input) J-Ks=0.514+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:37.61 +34:55:40.6: 13.92 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:37.61 +34:55:40.6: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 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,2461300.8978,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.84 04:55:53.87 +34:56:42.3
169.04651 -5.23356 galactic Aur Second-epoch detections are separated by 1.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:53.87 +34:56:42.3 (user input) | T | P | (position from user input) J-Ks=1.020+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:53.87 +34:56:42.3: 13.93 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:53.87 +34:56:42.3: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.95 +/- 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,2461300.8978,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.80 04:57:53.36 +35:00:42.0
169.24823 -4.87235 galactic Aur Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:53.36 +35:00:42.0 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:53.36 +35:00:42.0: 13.93 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:53.36 +35:00:42.0: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.80,0.05,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 20260917.3978 12.80CV 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 09 17.3978 2461300.8978 12.91 04:55:10.12 +34:33:20.7
169.25860 -5.59333 galactic Aur Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:10.12 +34:33:20.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.860+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:10.12 +34:33:20.7: 13.96 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:10.12 +34:33:20.7: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.91CV 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 09 17.3978 2461300.8978 12.97 04:53:38.69 +35:55:19.6
167.99296 -4.98053 galactic Aur Second-epoch detections are separated by 1.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:53:38.69 +35:55:19.6 (user input) | T | P | (position from user input) J-Ks=1.384+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:38.69 +35:55:19.6: 13.90 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:38.69 +35:55:19.6: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 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,2461300.8978,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.97CV 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 09 17.3978 2461300.8978 12.96 04:56:41.97 +36:02:13.9
168.29045 -4.42624 galactic Aur Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:41.97 +36:02:13.9 (user input) | T | P | (position from user input) J-Ks=0.553+/-0.037 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:41.97 +36:02:13.9: 13.95 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:41.97 +36:02:13.9: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.96,0.05,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
target 20260917.3978 12.96CV 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 09 17.3978 2461300.8978 12.69 04:58:40.35 +34:54:34.0
169.42837 -4.80928 galactic Aur Second-epoch detections are separated by 2.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.6701+34.9068 | 04:58:40.35 +34:54:34.0 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.763+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:40.35 +34:54:34.0: 13.91 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:40.35 +34:54:34.0: 13.88 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.90 +/- 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
ATO J074.6701+34.9068,2461300.8978,12.69,0.05,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 J074.6701+34.9068 20260917.3978 12.69CV 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 09 17.3978 2461300.8978 12.89 04:56:00.89 +35:05:59.7
168.93982 -5.11842 galactic Aur Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:00.89 +35:05:59.7 (user input) | T | P | (position from user input) J-Ks=0.698+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:00.89 +35:05:59.7: 13.93 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:00.89 +35:05:59.7: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 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,2461300.8978,12.89,0.05,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 20260917.3978 12.89CV 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 09 17.3978 2461300.8978 12.87 04:56:49.64 +34:58:30.4
169.14176 -5.06572 galactic Aur Second-epoch detections are separated by 2.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:49.64 +34:58:30.4 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.527+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:49.64 +34:58:30.4: 13.93 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:49.64 +34:58:30.4: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.95 +/- 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,2461300.8978,12.87,0.05,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 20260917.3978 12.87CV 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 09 17.3978 2461300.8978 12.85 04:55:00.96 +35:00:48.9
168.87961 -5.33206 galactic Aur Second-epoch detections are separated by 4.7" and 6.9 pix
The object was found in VSX24" Gaia DR3 162037124529404288
Type: ROT
# Max. Min./Amp. JD0 Period
14.580 G 14.620 G G
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:00.96 +35:00:48.9: 13.92 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:00.96 +35:00:48.9: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 162037124529404288,2461300.8978,12.85,0.05,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 162037124529404288 20260917.3978 12.85CV 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 09 17.3978 2461300.8978 12.88 04:54:56.40 +34:53:50.2
168.96107 -5.41686 galactic Aur Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:56.40 +34:53:50.2 (user input) | T | P | (position from user input) J-Ks=0.910+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:56.40 +34:53:50.2: 13.88 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:56.40 +34:53:50.2: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 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,2461300.8978,12.88,0.05,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 20260917.3978 12.88CV 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 09 17.3978 2461300.8978 12.72 04:56:31.07 +34:17:26.7
169.64097 -5.54040 galactic Aur Second-epoch detections are separated by 1.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1254+34.2924 | 04:56:31.07 +34:17:26.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:31.07 +34:17:26.7: 13.89 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:31.07 +34:17:26.7: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.93 +/- 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
ATO J074.1254+34.2924,2461300.8978,12.72,0.05,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 J074.1254+34.2924 20260917.3978 12.72CV 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 09 17.3978 2461300.8978 12.73 04:58:12.18 +34:08:43.8
169.97214 -5.35663 galactic Aur Second-epoch detections are separated by 1.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5494+34.1475 | 04:58:12.18 +34:08:43.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.567+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:12.18 +34:08:43.8: 13.93 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:12.18 +34:08:43.8: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 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
ATO J074.5494+34.1475,2461300.8978,12.73,0.05,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 J074.5494+34.1475 20260917.3978 12.73CV 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 09 17.3978 2461300.8978 12.81 04:59:23.87 +36:14:56.5
168.46180 -3.86729 galactic Aur Second-epoch detections are separated by 3.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:23.87 +36:14:56.5 (user input) | T | P | (position from user input) J-Ks=0.590+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:23.87 +36:14:56.5: 13.89 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:23.87 +36:14:56.5: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.82 +/- 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,2461300.8978,12.81,0.05,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 20260917.3978 12.81CV 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 09 17.3978 2461300.8978 12.62 04:57:52.66 +34:33:18.9
169.60685 -5.15642 galactic Aur Second-epoch detections are separated by 1.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:52.66 +34:33:18.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.524+/-0.042 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:52.66 +34:33:18.9: 13.90 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:52.66 +34:33:18.9: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.87 +/- 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,2461300.8978,12.62,0.05,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 20260917.3978 12.62CV 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 09 17.3978 2461300.8978 12.62 04:56:50.93 +34:40:36.5
169.37939 -5.24737 galactic Aur Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.2113+34.6672 | 04:56:50.93 +34:40:36.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.500+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:50.93 +34:40:36.5: 13.85 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:50.93 +34:40:36.5: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.2113+34.6672,2461300.8978,12.62,0.05,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 J074.2113+34.6672 20260917.3978 12.62CV 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 09 17.3978 2461300.8978 12.82 04:56:48.30 +35:10:14.4
168.98502 -4.94791 galactic Aur Second-epoch detections are separated by 2.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:48.30 +35:10:14.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.549+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:48.30 +35:10:14.4: 13.85 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:48.30 +35:10:14.4: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461300.8978,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.74 04:55:59.31 +34:32:40.2
169.37308 -5.46828 galactic Aur Second-epoch detections are separated by 1.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:59.31 +34:32:40.2 (user input) | T | P | (position from user input) J-Ks=0.948+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:59.31 +34:32:40.2: 13.90 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:59.31 +34:32:40.2: 13.93 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 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,2461300.8978,12.74,0.05,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 20260917.3978 12.74CV 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 09 17.3978 2461300.8978 12.98 04:56:08.90 +36:05:01.6
168.18433 -4.48442 galactic Aur Second-epoch detections are separated by 2.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:08.90 +36:05:01.6 (user input) | T | P | (position from user input) J-Ks=0.487+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:08.90 +36:05:01.6: 13.88 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:08.90 +36:05:01.6: 13.98 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.98,0.05,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 20260917.3978 12.98CV 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 09 17.3978 2461300.8978 12.89 04:56:00.53 +36:01:23.1
168.21432 -4.54429 galactic Aur Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:00.53 +36:01:23.1 (user input) | T | P | (position from user input) J-Ks=0.499+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:00.53 +36:01:23.1: 13.84 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:00.53 +36:01:23.1: 13.97 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.89 +/- 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,2461300.8978,12.89,0.05,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 20260917.3978 12.89CV 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 09 17.3978 2461300.8978 12.62 04:59:39.38 +36:03:58.9
168.63825 -3.93869 galactic Aur Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:39.38 +36:03:58.9 (user input) | T | P | (position from user input) J-Ks=0.958+/-0.030 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:39.38 +36:03:58.9: 13.85 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:39.38 +36:03:58.9: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 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,2461300.8978,12.62,0.05,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 20260917.3978 12.62CV 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 09 17.3978 2461300.8978 12.95 04:55:35.07 +36:01:42.8
168.15634 -4.60793 galactic Aur Second-epoch detections are separated by 1.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:35.07 +36:01:42.8 (user input) | T | P | (position from user input) J-Ks=0.837+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:35.07 +36:01:42.8: 13.85 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:35.07 +36:01:42.8: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 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,2461300.8978,12.95,0.05,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 20260917.3978 12.95CV 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 09 17.3978 2461300.8978 12.56 04:58:27.65 +34:53:52.1
169.41069 -4.85061 galactic Aur Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:27.65 +34:53:52.1 (user input) | T | P | (position from user input) J-Ks=0.934+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:27.65 +34:53:52.1: 13.84 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:27.65 +34:53:52.1: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.87 +/- 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,2461300.8978,12.56,0.05,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 20260917.3978 12.56CV 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 09 17.3978 2461300.8978 12.93 04:53:59.36 +36:13:31.3
167.80003 -4.73589 galactic Aur Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:53:59.36 +36:13:31.3 (user input) | T | P | (position from user input) J-Ks=0.925+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:59.36 +36:13:31.3: 13.84 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:59.36 +36:13:31.3: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 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,2461300.8978,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.74 04:59:30.66 +36:23:25.4
168.36429 -3.76223 galactic Aur Second-epoch detections are separated by 1.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:30.66 +36:23:25.4 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:30.66 +36:23:25.4: 13.84 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:30.66 +36:23:25.4: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.74,0.05,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 20260917.3978 12.74CV 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 09 17.3978 2461300.8978 12.63 04:57:12.91 +34:32:01.4
169.53907 -5.27691 galactic Aur Second-epoch detections are separated by 1.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:12.91 +34:32:01.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.521+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:12.91 +34:32:01.4: 13.81 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:12.91 +34:32:01.4: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.63,0.05,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 20260917.3978 12.63CV 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 09 17.3978 2461300.8978 12.71 04:58:36.02 +36:01:14.0
168.54243 -4.13498 galactic Aur Second-epoch detections are separated by 0.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:36.02 +36:01:14.0 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.031 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:36.02 +36:01:14.0: 13.81 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:36.02 +36:01:14.0: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461300.8978,12.71,0.05,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 20260917.3978 12.71CV 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 09 17.3978 2461300.8978 12.54 04:58:23.79 +34:50:58.5
169.44059 -4.89076 galactic Aur Second-epoch detections are separated by 1.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:23.79 +34:50:58.5 (user input) | T | P | (position from user input) J-Ks=0.920+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:23.79 +34:50:58.5: 13.81 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:23.79 +34:50:58.5: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461300.8978,12.54,0.05,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 20260917.3978 12.54CV 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 09 17.3978 2461300.8978 12.89 04:55:43.97 +35:47:46.9
168.35718 -4.72936 galactic Aur Second-epoch detections are separated by 1.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:43.97 +35:47:46.9 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:43.97 +35:47:46.9: 13.82 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:43.97 +35:47:46.9: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 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,2461300.8978,12.89,0.05,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 20260917.3978 12.89CV 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 09 17.3978 2461300.8978 12.85 04:55:03.49 +34:43:30.6
169.11134 -5.50538 galactic Aur Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:03.49 +34:43:30.6 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:03.49 +34:43:30.6: 13.82 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:03.49 +34:43:30.6: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 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,2461300.8978,12.85,0.05,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 20260917.3978 12.85CV 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 09 17.3978 2461300.8978 12.88 04:57:20.42 +36:07:57.4
168.29613 -4.26550 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:20.42 +36:07:57.4 (user input) | T | P | (position from user input) J-Ks=0.858+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:20.42 +36:07:57.4: 13.81 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:20.42 +36:07:57.4: 13.81 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461300.8978,12.88,0.05,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 20260917.3978 12.88CV 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 09 17.3978 2461300.8978 12.67 04:59:08.68 +35:56:45.7
168.66936 -4.09433 galactic Aur Second-epoch detections are separated by 1.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.7848+35.9431 | 04:59:08.68 +35:56:45.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.250+/-0.033 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:08.68 +35:56:45.7: 13.82 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:08.68 +35:56:45.7: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.84 +/- 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
ATO J074.7848+35.9431,2461300.8978,12.67,0.05,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 J074.7848+35.9431 20260917.3978 12.67CV 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 09 17.3978 2461300.8978 12.52 04:57:56.28 +34:40:07.4
169.52499 -5.07653 galactic Aur Second-epoch detections are separated by 2.3" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4718+34.6730 | 04:57:56.28 +34:40:07.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.851+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:56.28 +34:40:07.4: 13.81 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:56.28 +34:40:07.4: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.4718+34.6730,2461300.8978,12.52,0.05,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 J074.4718+34.6730 20260917.3978 12.52CV 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 09 17.3978 2461300.8978 12.88 04:59:39.48 +36:48:51.1
168.04803 -3.47787 galactic Aur Second-epoch detections are separated by 2.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.9178+36.8122 | 04:59:39.48 +36:48:51.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.295+/-0.031 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:39.48 +36:48:51.1: 13.82 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:39.48 +36:48:51.1: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 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 J074.9178+36.8122,2461300.8978,12.88,0.05,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
ATO J074.9178+36.8122 20260917.3978 12.88CV 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 09 17.3978 2461300.8978 12.62 04:58:11.05 +35:44:39.2
168.70799 -4.37205 galactic Aur Second-epoch detections are separated by 1.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:11.05 +35:44:39.2 (user input) | T | P | (position from user input) J-Ks=0.988+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:11.05 +35:44:39.2: 13.79 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:11.05 +35:44:39.2: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 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,2461300.8978,12.62,0.05,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 20260917.3978 12.62CV 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 09 17.3978 2461300.8978 12.84 04:55:00.82 +35:49:28.9
168.24360 -4.82553 galactic Aur Second-epoch detections are separated by 1.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:00.82 +35:49:28.9 (user input) | T | P | (position from user input) J-Ks=0.478+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:00.82 +35:49:28.9: 13.79 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:00.82 +35:49:28.9: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461300.8978,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.51 04:56:34.51 +34:31:49.4
169.45960 -5.38238 galactic Aur Second-epoch detections are separated by 1.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1381+34.5228 | 04:56:34.51 +34:31:49.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.478+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:34.51 +34:31:49.4: 13.81 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:34.51 +34:31:49.4: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 J074.1381+34.5228,2461300.8978,12.51,0.05,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 J074.1381+34.5228 20260917.3978 12.51CV 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 09 17.3978 2461300.8978 12.61 04:55:27.86 +34:49:38.2
169.08343 -5.37650 galactic Aur Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:27.86 +34:49:38.2 (user input) | T | P | (position from user input) J-Ks=1.056+/-0.023 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:27.86 +34:49:38.2: 13.78 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:27.86 +34:49:38.2: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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,2461300.8978,12.61,0.05,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 20260917.3978 12.61CV 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 09 17.3978 2461300.8978 12.60 04:56:09.32 +34:39:17.3
169.30776 -5.37279 galactic Aur Second-epoch detections are separated by 1.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.0436+34.6610 | 04:56:09.32 +34:39:17.3 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.828+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:09.32 +34:39:17.3: 13.79 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:09.32 +34:39:17.3: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 J074.0436+34.6610,2461300.8978,12.60,0.05,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
ATO J074.0436+34.6610 20260917.3978 12.60CV 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 09 17.3978 2461300.8978 12.57 04:57:21.74 +34:50:09.4
169.31965 -5.06596 galactic Aur Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:21.74 +34:50:09.4 (user input) | T | P | (position from user input) J-Ks=0.493+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:21.74 +34:50:09.4: 13.77 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:21.74 +34:50:09.4: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 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,2461300.8978,12.57,0.05,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 20260917.3978 12.57CV 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 09 17.3978 2461300.8978 12.59 04:55:44.12 +34:52:37.8
169.07904 -5.30192 galactic Aur Second-epoch detections are separated by 2.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:44.12 +34:52:37.8 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.024 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:44.12 +34:52:37.8: 13.78 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:44.12 +34:52:37.8: 13.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 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,2461300.8978,12.59,0.05,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 20260917.3978 12.59CV 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 09 17.3978 2461300.8978 12.61 04:55:20.28 +34:27:58.8
169.35070 -5.62181 galactic Aur Second-epoch detections are separated by 2.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:20.28 +34:27:58.8 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:20.28 +34:27:58.8: 13.80 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:20.28 +34:27:58.8: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.61,0.05,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 20260917.3978 12.61CV 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 09 17.3978 2461300.8978 12.89 04:59:30.11 +36:39:02.4
168.15775 -3.60329 galactic Aur Second-epoch detections are separated by 0.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:30.11 +36:39:02.4 (user input) | T | P | (position from user input) J-Ks=0.300+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:30.11 +36:39:02.4: 13.76 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:30.11 +36:39:02.4: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 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,2461300.8978,12.89,0.05,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 20260917.3978 12.89CV 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 09 17.3978 2461300.8978 12.78 04:55:51.69 +35:35:59.8
168.52762 -4.83141 galactic Aur Second-epoch detections are separated by 1.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:51.69 +35:35:59.8 (user input) | T | P | (position from user input) J-Ks=0.872+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:51.69 +35:35:59.8: 13.76 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:51.69 +35:35:59.8: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 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,2461300.8978,12.78,0.05,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 20260917.3978 12.78CV 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 09 17.3978 2461300.8978 12.52 04:54:51.25 +35:23:45.5
168.55909 -5.11891 galactic Aur Second-epoch detections are separated by 1.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:51.25 +35:23:45.5 (user input) | T | P | (position from user input) J-Ks=0.691+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:51.25 +35:23:45.5: 13.75 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:51.25 +35:23:45.5: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 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,2461300.8978,12.52,0.05,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 20260917.3978 12.52CV 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 09 17.3978 2461300.8978 12.53 04:59:28.82 +35:49:28.8
168.80719 -4.11557 galactic Aur Second-epoch detections are separated by 3.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.8679+35.8214 | 04:59:28.82 +35:49:28.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.819+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:28.82 +35:49:28.8: 13.76 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:28.82 +35:49:28.8: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 J074.8679+35.8214,2461300.8978,12.53,0.05,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
ATO J074.8679+35.8214 20260917.3978 12.53CV 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 09 17.3978 2461300.8978 12.59 04:59:46.18 +36:28:31.9
168.32919 -3.66880 galactic Aur Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:46.18 +36:28:31.9 (user input) | T | P | (position from user input) J-Ks=0.833+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:46.18 +36:28:31.9: 13.74 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:46.18 +36:28:31.9: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 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,2461300.8978,12.59,0.05,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 20260917.3978 12.59CV 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 09 17.3978 2461300.8978 12.57 04:57:29.99 +33:51:53.0
170.10359 -5.64464 galactic Aur Second-epoch detections are separated by 1.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 160989740921830656 | 04:57:26.43 +33:52:07.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2V 1928MeUpp..37....1S BD+33 930 J-Ks=1.167+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:29.99 +33:51:53.0: 13.75 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:29.99 +33:51:53.0: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 160989740921830656,2461300.8978,12.57,0.05,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 160989740921830656 20260917.3978 12.57CV 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 09 17.3978 2461300.8978 12.75 04:55:01.84 +34:56:55.5
168.93235 -5.37020 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:01.84 +34:56:55.5 (user input) | T | P | (position from user input) J-Ks=0.846+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:01.84 +34:56:55.5: 13.74 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:01.84 +34:56:55.5: 13.74 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461300.8978,12.75,0.05,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
target 20260917.3978 12.75CV 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 09 17.3978 2461300.8978 12.57 04:58:43.18 +34:55:20.4
169.42417 -4.79372 galactic Aur Second-epoch detections are separated by 2.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:43.18 +34:55:20.4 (user input) | T | P | (position from user input) J-Ks=0.860+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:43.18 +34:55:20.4: 13.76 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:43.18 +34:55:20.4: 13.65 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.57,0.05,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 20260917.3978 12.57CV 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 09 17.3978 2461300.8978 12.57 04:55:43.15 +34:41:35.6
169.22151 -5.41909 galactic Aur Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:43.15 +34:41:35.6 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.697+/-0.023 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:43.15 +34:41:35.6: 13.78 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:43.15 +34:41:35.6: 13.77 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 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,2461300.8978,12.57,0.05,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 20260917.3978 12.57CV 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 09 17.3978 2461300.8978 12.62 04:58:23.55 +35:36:55.0
168.83588 -4.41851 galactic Aur Second-epoch detections are separated by 2.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5952+35.6269 | 04:58:23.55 +35:36:55.0 (user input) | DBH (ATLAS) | (ATLAS) | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.408+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:23.55 +35:36:55.0: 13.76 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:23.55 +35:36:55.0: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 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 J074.5952+35.6269,2461300.8978,12.62,0.05,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 J074.5952+35.6269 20260917.3978 12.62CV 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 09 17.3978 2461300.8978 12.82 04:57:06.75 +35:43:50.4
168.58351 -4.55114 galactic Aur Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.2752+35.7268 | 04:57:06.75 +35:43:50.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.879+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:06.75 +35:43:50.4: 13.80 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:06.75 +35:43:50.4: 13.83 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 J074.2752+35.7268,2461300.8978,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.2752+35.7268 20260917.3978 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.66 04:59:31.17 +36:40:42.8
168.13793 -3.58331 galactic Aur Second-epoch detections are separated by 1.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:31.17 +36:40:42.8 (user input) | T | P | (position from user input) J-Ks=0.964+/-0.029 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:31.17 +36:40:42.8: 13.77 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:31.17 +36:40:42.8: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 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,2461300.8978,12.66,0.05,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 20260917.3978 12.66CV 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 09 17.3978 2461300.8978 12.68 04:57:55.69 +35:48:54.1
168.61999 -4.36903 galactic Aur Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4821+35.8151 | 04:57:55.69 +35:48:54.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.985+/-0.025 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:55.69 +35:48:54.1: 13.74 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:55.69 +35:48:54.1: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 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 J074.4821+35.8151,2461300.8978,12.68,0.05,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 J074.4821+35.8151 20260917.3978 12.68CV 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 09 17.3978 2461300.8978 12.79 04:56:31.61 +35:29:59.0
168.69088 -4.78790 galactic Aur Second-epoch detections are separated by 3.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1315+35.4994 | 04:56:31.61 +35:29:59.0 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.751+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:31.61 +35:29:59.0: 13.73 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:31.61 +35:29:59.0: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.1315+35.4994,2461300.8978,12.79,0.05,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
ATO J074.1315+35.4994 20260917.3978 12.79CV 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 09 17.3978 2461300.8978 12.71 04:54:49.37 +35:41:49.6
168.31921 -4.93554 galactic Aur Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:49.37 +35:41:49.6 (user input) | T | P | (position from user input) J-Ks=0.984+/-0.025 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:49.37 +35:41:49.6: 13.74 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:49.37 +35:41:49.6: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461300.8978,12.71,0.05,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 20260917.3978 12.71CV 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 09 17.3978 2461300.8978 12.71 04:57:07.10 +35:53:26.4
168.45842 -4.45089 galactic Aur Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:07.10 +35:53:26.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:07.10 +35:53:26.4: 13.72 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:07.10 +35:53:26.4: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 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,2461300.8978,12.71,0.05,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 20260917.3978 12.71CV 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 09 17.3978 2461300.8978 12.64 04:58:06.38 +36:05:09.4
168.42900 -4.17301 galactic Aur Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:06.38 +36:05:09.4 (user input) | T | P | (position from user input) J-Ks=0.602+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:06.38 +36:05:09.4: 13.76 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:06.38 +36:05:09.4: 13.80 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.64,0.05,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 20260917.3978 12.64CV 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 09 17.3978 2461300.8978 12.59 05:00:00.83 +36:39:09.2
168.21961 -3.52121 galactic Aur Second-epoch detections are separated by 1.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:00:00.83 +36:39:09.2 (user input) | T | P | (position from user input) J-Ks=1.089+/-0.029 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 05:00:00.83 +36:39:09.2: 13.72 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 05:00:00.83 +36:39:09.2: 13.76 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 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,2461300.8978,12.59,0.05,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 20260917.3978 12.59CV 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 09 17.3978 2461300.8978 12.50 04:56:52.51 +34:42:13.6
169.36152 -5.22639 galactic Aur Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.2147+34.7026 | 04:56:52.51 +34:42:13.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:52.51 +34:42:13.6: 13.72 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:52.51 +34:42:13.6: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.2147+34.7026,2461300.8978,12.50,0.05,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 J074.2147+34.7026 20260917.3978 12.50CV 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 09 17.3978 2461300.8978 12.63 04:57:30.28 +35:36:07.8
168.73418 -4.56837 galactic Aur Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:30.28 +35:36:07.8 (user input) | T | P | (position from user input) J-Ks=0.547+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:30.28 +35:36:07.8: 13.71 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:30.28 +35:36:07.8: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.72 +/- 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,2461300.8978,12.63,0.05,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 20260917.3978 12.63CV 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 09 17.3978 2461300.8978 12.51 04:58:18.55 +35:01:59.7
169.28451 -4.79144 galactic Aur Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5778+35.0456 | 04:58:18.55 +35:01:59.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.493+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:18.55 +35:01:59.7: 13.71 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:18.55 +35:01:59.7: 13.78 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 J074.5778+35.0456,2461300.8978,12.51,0.05,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 J074.5778+35.0456 20260917.3978 12.51CV 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 09 17.3978 2461300.8978 12.53 04:59:49.14 +36:27:55.8
168.34322 -3.66716 galactic Aur Second-epoch detections are separated by 2.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:49.14 +36:27:55.8 (user input) | T | P | (position from user input) J-Ks=0.767+/-0.026 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:49.14 +36:27:55.8: 13.73 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:49.14 +36:27:55.8: 13.89 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.80 +/- 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,2461300.8978,12.53,0.05,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 20260917.3978 12.53CV 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 09 17.3978 2461300.8978 12.52 04:58:35.68 +35:42:13.6
168.79152 -4.33155 galactic Aur Second-epoch detections are separated by 1.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.6460+35.6921 | 04:58:35.68 +35:42:13.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A2V (LAMOST DR5) J-Ks=0.304+/-0.030 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:35.68 +35:42:13.6: 13.70 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:35.68 +35:42:13.6: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 J074.6460+35.6921,2461300.8978,12.52,0.05,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 J074.6460+35.6921 20260917.3978 12.52CV 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 09 17.3978 2461300.8978 12.55 04:56:00.30 +34:40:38.1
169.27080 -5.38304 galactic Aur Second-epoch detections are separated by 1.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:00.30 +34:40:38.1 (user input) | T | P | (position from user input) J-Ks=1.013+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:00.30 +34:40:38.1: 13.70 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:00.30 +34:40:38.1: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461300.8978,12.55,0.05,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 20260917.3978 12.55CV 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 09 17.3978 2461300.8978 12.54 04:59:45.63 +36:13:49.6
168.52161 -3.82112 galactic Aur Second-epoch detections are separated by 1.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:45.63 +36:13:49.6 (user input) | T | P | (position from user input) J-Ks=0.521+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:45.63 +36:13:49.6: 13.68 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:45.63 +36:13:49.6: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461300.8978,12.54,0.05,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 20260917.3978 12.54CV 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 09 17.3978 2461300.8978 12.57 04:55:36.58 +34:54:06.6
169.04354 -5.30671 galactic Aur Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.9036+34.8983 | 04:55:36.58 +34:54:06.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.271+/-0.026 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:36.58 +34:54:06.6: 13.70 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:36.58 +34:54:06.6: 13.69 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 J073.9036+34.8983,2461300.8978,12.57,0.05,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 J073.9036+34.8983 20260917.3978 12.57CV 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 09 17.3978 2461300.8978 12.55 04:58:38.90 +36:18:32.6
168.32102 -3.94910 galactic Aur Second-epoch detections are separated by 2.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:38.90 +36:18:32.6 (user input) | T | P | (position from user input) J-Ks=0.710+/-0.034 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:38.90 +36:18:32.6: 13.72 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:38.90 +36:18:32.6: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.55,0.05,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 20260917.3978 12.55CV 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 09 17.3978 2461300.8978 12.54 04:58:48.44 +35:59:26.7
168.59185 -4.12046 galactic Aur Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 186206249829815936 | 04:58:48.44 +35:59:26.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.754+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:48.44 +35:59:26.7: 13.69 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:48.44 +35:59:26.7: 13.72 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 186206249829815936,2461300.8978,12.54,0.05,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
Large-amplitude variable Gaia DR2 186206249829815936 20260917.3978 12.54CV 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 09 17.3978 2461300.8978 12.58 04:59:56.53 +36:32:22.2
168.30004 -3.60211 galactic Aur Second-epoch detections are separated by 1.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:56.53 +36:32:22.2 (user input) | T | P | (position from user input) J-Ks=0.248+/-0.030 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:56.53 +36:32:22.2: 13.67 +/- 0.05 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:56.53 +36:32:22.2: 13.69 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.58,0.05,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 20260917.3978 12.58CV 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 09 17.3978 2461300.8978 12.51 04:56:36.18 +34:14:49.7
169.68630 -5.55367 galactic Aur Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1527+34.2443 | 04:56:36.18 +34:14:49.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.569+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:36.18 +34:14:49.7: 13.66 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:36.18 +34:14:49.7: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.1527+34.2443,2461300.8978,12.51,0.05,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 J074.1527+34.2443 20260917.3978 12.51CV 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 09 17.3978 2461300.8978 12.67 04:56:25.77 +36:02:30.7
168.25273 -4.46606 galactic Aur Second-epoch detections are separated by 0.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:25.77 +36:02:30.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:25.77 +36:02:30.7: 13.59 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:25.77 +36:02:30.7: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.67,0.05,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 20260917.3978 12.67CV 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 09 17.3978 2461300.8978 12.40 04:57:52.32 +34:40:22.1
169.51335 -5.08467 galactic Aur Second-epoch detections are separated by 2.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4718+34.6730 | 04:57:52.32 +34:40:22.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.440+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:52.32 +34:40:22.1: 13.67 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:52.32 +34:40:22.1: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.4718+34.6730,2461300.8978,12.40,0.05,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
ATO J074.4718+34.6730 20260917.3978 12.40CV 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 09 17.3978 2461300.8978 12.60 04:55:10.41 +35:07:49.0
168.80828 -5.23402 galactic Aur Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:10.41 +35:07:49.0 (user input) | T | P | (position from user input) J-Ks=1.057+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:10.41 +35:07:49.0: 13.67 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:10.41 +35:07:49.0: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461300.8978,12.60,0.05,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 20260917.3978 12.60CV 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 09 17.3978 2461300.8978 12.42 04:56:47.46 +34:20:59.5
169.62955 -5.45949 galactic Aur Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:47.46 +34:20:59.5 (user input) | T | P | (position from user input) J-Ks=0.610+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:47.46 +34:20:59.5: 13.67 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:47.46 +34:20:59.5: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.42,0.05,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 20260917.3978 12.42CV 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 09 17.3978 2461300.8978 12.63 04:55:11.47 +35:17:57.3
168.67802 -5.12570 galactic Aur Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 186075407948027264 | 04:55:08.13 +35:18:11.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.435+/-0.029 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:11.47 +35:17:57.3: 13.66 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:11.47 +35:17:57.3: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 186075407948027264,2461300.8978,12.63,0.05,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
Large-amplitude variable Gaia DR2 186075407948027264 20260917.3978 12.63CV 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 09 17.3978 2461300.8978 12.63 04:59:22.70 +36:14:15.1
168.46845 -3.87747 galactic Aur Second-epoch detections are separated by 0.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:22.70 +36:14:15.1 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.029 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:22.70 +36:14:15.1: 13.67 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:22.70 +36:14:15.1: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.63,0.05,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 20260917.3978 12.63CV 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 09 17.3978 2461300.8978 12.49 04:58:48.76 +35:02:26.4
169.34247 -4.70576 galactic Aur Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:48.76 +35:02:26.4 (user input) | T | P | (position from user input) J-Ks=0.897+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:48.76 +35:02:26.4: 13.67 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:48.76 +35:02:26.4: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.49CV 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 09 17.3978 2461300.8978 12.54 04:57:08.29 +34:48:33.7
169.31198 -5.11854 galactic Aur Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:08.29 +34:48:33.7 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.463+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:08.29 +34:48:33.7: 13.63 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:08.29 +34:48:33.7: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.54,0.05,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 20260917.3978 12.54CV 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 09 17.3978 2461300.8978 12.57 04:55:39.53 +35:33:03.5
168.54026 -4.89416 galactic Aur Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:39.53 +35:33:03.5 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.025 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:39.53 +35:33:03.5: 13.64 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:39.53 +35:33:03.5: 13.67 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.57,0.05,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 20260917.3978 12.57CV 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 09 17.3978 2461300.8978 12.60 04:58:26.89 +36:05:19.3
168.46966 -4.11705 galactic Aur Second-epoch detections are separated by 1.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:26.89 +36:05:19.3 (user input) | T | P | (position from user input) J-Ks=0.521+/-0.031 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:26.89 +36:05:19.3: 13.65 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:26.89 +36:05:19.3: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461300.8978,12.60,0.05,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 20260917.3978 12.60CV 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 09 17.3978 2461300.8978 12.63 04:54:52.60 +35:31:05.5
168.46621 -5.03891 galactic Aur Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:52.60 +35:31:05.5 (user input) | T | P | (position from user input) J-Ks=0.435+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:52.60 +35:31:05.5: 13.66 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:52.60 +35:31:05.5: 13.73 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.69 +/- 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,2461300.8978,12.63,0.05,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 20260917.3978 12.63CV 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 09 17.3978 2461300.8978 12.68 04:55:30.08 +35:45:57.8
168.35155 -4.78496 galactic Aur Second-epoch detections are separated by 1.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:30.08 +35:45:57.8 (user input) | T | P | (position from user input) J-Ks=0.317+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:30.08 +35:45:57.8: 13.63 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:30.08 +35:45:57.8: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.68,0.05,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 20260917.3978 12.68CV 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 09 17.3978 2461300.8978 12.71 04:54:13.04 +35:56:20.8
168.05270 -4.87964 galactic Aur Second-epoch detections are separated by 1.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.5570+35.9405 | 04:54:13.04 +35:56:20.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.294+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:13.04 +35:56:20.8: 13.65 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:13.04 +35:56:20.8: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.5570+35.9405,2461300.8978,12.71,0.05,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 J073.5570+35.9405 20260917.3978 12.71CV 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 09 17.3978 2461300.8978 12.29 04:58:30.07 +35:54:10.0
168.62285 -4.22353 galactic Aur Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:30.07 +35:54:10.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:30.07 +35:54:10.0: 13.57 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:30.07 +35:54:10.0: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.29,0.05,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 20260917.3978 12.29CV 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 09 17.3978 2461300.8978 12.34 04:56:34.68 +34:34:43.8
169.42182 -5.35185 galactic Aur Second-epoch detections are separated by 1.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:34.68 +34:34:43.8 (user input) | T | P | (position from user input) J-Ks=0.543+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:34.68 +34:34:43.8: 13.63 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:34.68 +34:34:43.8: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.34CV 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 09 17.3978 2461300.8978 12.34 04:57:07.09 +34:38:12.1
169.44548 -5.22878 galactic Aur Second-epoch detections are separated by 1.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:07.09 +34:38:12.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:07.09 +34:38:12.1: 13.62 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:07.09 +34:38:12.1: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.34CV 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 09 17.3978 2461300.8978 12.46 04:59:37.46 +36:33:04.6
168.25136 -3.64516 galactic Aur Second-epoch detections are separated by 2.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:37.46 +36:33:04.6 (user input) | T | P | (position from user input) J-Ks=0.313+/-0.029 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:37.46 +36:33:04.6: 13.62 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:37.46 +36:33:04.6: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.46,0.05,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 20260917.3978 12.46CV 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 09 17.3978 2461300.8978 12.56 04:58:42.00 +36:00:43.4
168.56161 -4.12438 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:42.00 +36:00:43.4 (user input) | T | P | (position from user input) J-Ks=0.338+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:42.00 +36:00:43.4: 13.62 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:42.00 +36:00:43.4: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.56,0.05,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 20260917.3978 12.56CV 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 09 17.3978 2461300.8978 12.36 04:57:46.58 +34:27:43.2
169.66750 -5.23047 galactic Aur Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4376+34.4703 | 04:57:46.58 +34:27:43.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.042+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:46.58 +34:27:43.2: 13.58 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:46.58 +34:27:43.2: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 J074.4376+34.4703,2461300.8978,12.36,0.05,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
ATO J074.4376+34.4703 20260917.3978 12.36CV 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 09 17.3978 2461300.8978 12.58 04:54:30.72 +35:46:11.8
168.22257 -4.93914 galactic Aur Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:30.72 +35:46:11.8 (user input) | T | P | (position from user input) J-Ks=0.848+/-0.025 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:30.72 +35:46:11.8: 13.62 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:30.72 +35:46:11.8: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.58,0.05,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 20260917.3978 12.58CV 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 09 17.3978 2461300.8978 12.61 04:54:37.32 +35:44:05.6
168.26403 -4.94369 galactic Aur Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:37.32 +35:44:05.6 (user input) | T | P | (position from user input) J-Ks=0.304+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:37.32 +35:44:05.6: 13.62 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:37.32 +35:44:05.6: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.61,0.05,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 20260917.3978 12.61CV 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 09 17.3978 2461300.8978 12.48 04:56:19.08 +34:57:43.7
169.08689 -5.15555 galactic Aur Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:19.08 +34:57:43.7 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.586+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:19.08 +34:57:43.7: 13.61 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:19.08 +34:57:43.7: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 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,2461300.8978,12.48,0.05,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 20260917.3978 12.48CV 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 09 17.3978 2461300.8978 12.59 04:55:09.86 +34:57:31.4
168.94170 -5.34258 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:09.86 +34:57:31.4 (user input) | T | P | (position from user input) J-Ks=0.862+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:09.86 +34:57:31.4: 13.62 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:09.86 +34:57:31.4: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.59,0.05,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 20260917.3978 12.59CV 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 09 17.3978 2461300.8978 12.50 04:57:15.90 +35:06:34.4
169.09168 -4.91206 galactic Aur Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:15.90 +35:06:34.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.087+/-0.023 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:15.90 +35:06:34.4: 13.61 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:15.90 +35:06:34.4: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.50,0.05,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 20260917.3978 12.50CV 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 09 17.3978 2461300.8978 12.39 04:56:39.34 +34:36:30.2
169.40851 -5.32097 galactic Aur Second-epoch detections are separated by 0.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:39.34 +34:36:30.2 (user input) | T | P | (position from user input) J-Ks=1.203+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:39.34 +34:36:30.2: 13.62 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:39.34 +34:36:30.2: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 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,2461300.8978,12.39,0.05,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 20260917.3978 12.39CV 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 09 17.3978 2461300.8978 12.39 04:57:54.08 +33:58:12.0
170.07211 -5.51411 galactic Aur Second-epoch detections are separated by 1.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:54.08 +33:58:12.0 (user input) | T | P | (position from user input) J-Ks=0.460+/-0.024 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:54.08 +33:58:12.0: 13.59 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:54.08 +33:58:12.0: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.39,0.05,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 20260917.3978 12.39CV 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 09 17.3978 2461300.8978 12.35 04:57:10.51 +34:49:23.5
169.30581 -5.10400 galactic Aur Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:10.51 +34:49:23.5 (user input) | T | P | (position from user input) J-Ks=0.620+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:10.51 +34:49:23.5: 13.61 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:10.51 +34:49:23.5: 13.59 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.35,0.05,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 20260917.3978 12.35CV 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 09 17.3978 2461300.8978 12.34 04:57:50.81 +33:51:47.6
170.14949 -5.58893 galactic Aur Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:50.81 +33:51:47.6 (user input) | T | P | (position from user input) J-Ks=0.938+/-0.023 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:50.81 +33:51:47.6: 13.58 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:50.81 +33:51:47.6: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.54 +/- 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,2461300.8978,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.34CV 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 09 17.3978 2461300.8978 12.42 04:56:49.87 +34:43:14.4
169.34258 -5.22300 galactic Aur Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:49.87 +34:43:14.4 (user input) | T | P | (position from user input) J-Ks=0.831+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:49.87 +34:43:14.4: 13.59 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:49.87 +34:43:14.4: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.42,0.05,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 20260917.3978 12.42CV 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 09 17.3978 2461300.8978 12.48 04:57:31.22 +33:55:16.2
170.06165 -5.60641 galactic Aur Second-epoch detections are separated by 1.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.3757+33.9209 | 04:57:31.22 +33:55:16.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.394+/-0.025 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:31.22 +33:55:16.2: 13.57 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:31.22 +33:55:16.2: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.3757+33.9209,2461300.8978,12.48,0.05,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 J074.3757+33.9209 20260917.3978 12.48CV 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 09 17.3978 2461300.8978 12.70 04:57:16.08 +34:07:16.1
169.87128 -5.52380 galactic Aur Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:16.08 +34:07:16.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.990+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:16.08 +34:07:16.1: 13.58 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:16.08 +34:07:16.1: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 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,2461300.8978,12.70,0.05,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 20260917.3978 12.70CV 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 09 17.3978 2461300.8978 12.47 04:57:55.89 +35:59:50.2
168.47688 -4.25566 galactic Aur Second-epoch detections are separated by 1.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4794+35.9977 | 04:57:55.89 +35:59:50.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:55.89 +35:59:50.2: 13.60 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:55.89 +35:59:50.2: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.4794+35.9977,2461300.8978,12.47,0.05,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
ATO J074.4794+35.9977 20260917.3978 12.47CV 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 09 17.3978 2461300.8978 12.52 04:55:32.90 +35:07:55.2
168.85495 -5.17306 galactic Aur Second-epoch detections are separated by 1.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.8858+35.1289 | 04:55:32.90 +35:07:55.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.272+/-0.025 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:32.90 +35:07:55.2: 13.58 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:32.90 +35:07:55.2: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.8858+35.1289,2461300.8978,12.52,0.05,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 J073.8858+35.1289 20260917.3978 12.52CV 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 09 17.3978 2461300.8978 12.52 04:55:35.37 +34:28:01.8
169.38249 -5.58075 galactic Aur Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:35.37 +34:28:01.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:35.37 +34:28:01.8: 13.58 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:35.37 +34:28:01.8: 13.44 +/- 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,2461300.8978,12.52,0.05,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 20260917.3978 12.52CV 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 09 17.3978 2461300.8978 12.60 04:55:27.00 +34:38:44.2
169.22428 -5.49204 galactic Aur Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:27.00 +34:38:44.2 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.346+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:27.00 +34:38:44.2: 13.57 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:27.00 +34:38:44.2: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.60,0.05,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 20260917.3978 12.60CV 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 09 17.3978 2461300.8978 12.43 04:59:07.94 +36:20:51.9
168.35084 -3.84853 galactic Aur Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.7759+36.3569 | 04:59:06.23 +36:21:24.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.567+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:07.94 +36:20:51.9: 13.56 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:07.94 +36:20:51.9: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.7759+36.3569,2461300.8978,12.43,0.05,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 J074.7759+36.3569 20260917.3978 12.43CV 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 09 17.3978 2461300.8978 12.48 04:55:10.34 +35:42:58.9
168.34865 -4.86813 galactic Aur Second-epoch detections are separated by 1.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:10.34 +35:42:58.9 (user input) | T | P | (position from user input) J-Ks=1.071+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:10.34 +35:42:58.9: 13.56 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:10.34 +35:42:58.9: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.48,0.05,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 20260917.3978 12.48CV 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 09 17.3978 2461300.8978 12.28 04:57:38.46 +34:53:57.8
169.30517 -4.98179 galactic Aur Second-epoch detections are separated by 1.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:38.46 +34:53:57.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.910+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:38.46 +34:53:57.8: 13.56 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:38.46 +34:53:57.8: 13.47 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.28CV 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 09 17.3978 2461300.8978 12.57 04:58:06.24 +35:11:20.8
169.13552 -4.72812 galactic Aur Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5269+35.1919 | 04:58:06.24 +35:11:20.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.496+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:06.24 +35:11:20.8: 13.56 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:06.24 +35:11:20.8: 13.65 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.5269+35.1919,2461300.8978,12.57,0.05,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 J074.5269+35.1919 20260917.3978 12.57CV 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 09 17.3978 2461300.8978 12.56 04:56:27.99 +35:18:57.9
168.82755 -4.91171 galactic Aur Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:27.99 +35:18:57.9 (user input) | T | P | (position from user input) J-Ks=1.547+/-0.029 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:27.99 +35:18:57.9: 13.55 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:27.99 +35:18:57.9: 13.51 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 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
target,2461300.8978,12.56,0.05,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 20260917.3978 12.56CV 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 09 17.3978 2461300.8978 13.25 04:59:05.05 +35:42:49.0
168.84525 -4.24729 galactic Aur Second-epoch detections are separated by 1.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:05.05 +35:42:49.0 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.610+/-0.036 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:05.05 +35:42:49.0: 14.73 +/- 0.11 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:05.05 +35:42:49.0: 14.59 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.65 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.25CV 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 09 17.3978 2461300.8978 12.37 04:55:12.08 +35:35:10.4
168.45433 -4.94484 galactic Aur Second-epoch detections are separated by 1.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.7954+35.5818 | 04:55:12.08 +35:35:10.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.378+/-0.029 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:12.08 +35:35:10.4: 13.54 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:12.08 +35:35:10.4: 13.61 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.7954+35.5818,2461300.8978,12.37,0.05,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 J073.7954+35.5818 20260917.3978 12.37CV 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 09 17.3978 2461300.8978 12.31 04:57:18.50 +34:33:47.5
169.52776 -5.24359 galactic Aur Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:18.50 +34:33:47.5 (user input) | T | P | (position from user input) J-Ks=1.198+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:18.50 +34:33:47.5: 13.54 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:18.50 +34:33:47.5: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.31CV 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 09 17.3978 2461300.8978 12.35 04:58:28.93 +34:53:04.8
169.42377 -4.85528 galactic Aur Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:28.93 +34:53:04.8 (user input) | T | P | (position from user input) J-Ks=1.357+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:28.93 +34:53:04.8: 13.54 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:28.93 +34:53:04.8: 13.52 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.35,0.05,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 20260917.3978 12.35CV 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 09 17.3978 2461300.8978 12.32 04:59:21.24 +36:01:09.2
168.63775 -4.01587 galactic Aur Second-epoch detections are separated by 0.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:21.24 +36:01:09.2 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.031 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:21.24 +36:01:09.2: 13.50 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:21.24 +36:01:09.2: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.32,0.05,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 20260917.3978 12.32CV 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 09 17.3978 2461300.8978 13.22 04:59:09.44 +35:50:49.1
168.74914 -4.15339 galactic Aur Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:09.44 +35:50:49.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.872+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:09.44 +35:50:49.1: 14.68 +/- 0.11 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:09.44 +35:50:49.1: 14.58 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.22CV 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 09 17.3978 2461300.8978 12.54 04:54:00.64 +35:57:52.7
168.00642 -4.89620 galactic Aur Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.5042+35.9632 | 04:54:00.64 +35:57:52.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:00.64 +35:57:52.7: 13.49 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:00.64 +35:57:52.7: 13.50 +/- 0.04 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
ATO J073.5042+35.9632,2461300.8978,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J073.5042+35.9632 20260917.3978 12.54CV 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 09 17.3978 2461300.8978 12.36 04:58:10.15 +34:13:47.0
169.90124 -5.31016 galactic Aur Second-epoch detections are separated by 1.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:10.15 +34:13:47.0 (user input) | T | P | (position from user input) J-Ks=0.359+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:10.15 +34:13:47.0: 13.49 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:10.15 +34:13:47.0: 13.51 +/- 0.04 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,2461300.8978,12.36,0.05,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 20260917.3978 12.36CV 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 09 17.3978 2461300.8978 12.38 04:58:49.38 +35:27:00.8
169.02034 -4.45152 galactic Aur Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:49.38 +35:27:00.8 (user input) | T | P | (position from user input) J-Ks=0.223+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:49.38 +35:27:00.8: 13.47 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:49.38 +35:27:00.8: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.38,0.05,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 20260917.3978 12.38CV 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 09 17.3978 2461300.8978 12.50 04:54:04.22 +35:48:39.6
168.13410 -4.98319 galactic Aur Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.5329+35.8108 | 04:54:04.22 +35:48:39.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.330+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:04.22 +35:48:39.6: 13.49 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:04.22 +35:48:39.6: 13.41 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.5329+35.8108,2461300.8978,12.50,0.05,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 J073.5329+35.8108 20260917.3978 12.50CV 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 09 17.3978 2461300.8978 12.39 04:55:33.75 +34:58:44.7
168.97682 -5.26612 galactic Aur Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:33.75 +34:58:44.7 (user input) | T | P | (position from user input) J-Ks=0.940+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:33.75 +34:58:44.7: 13.46 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:33.75 +34:58:44.7: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.39,0.05,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 20260917.3978 12.39CV 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 09 17.3978 2461300.8978 12.25 04:56:38.36 +34:38:28.4
169.38057 -5.30323 galactic Aur Second-epoch detections are separated by 1.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185844269987467904 | 04:56:41.59 +34:38:40.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3 1949AnHar.112....1C HD 280266 J-Ks=0.882+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:38.36 +34:38:28.4: 13.47 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:38.36 +34:38:28.4: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.48 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185844269987467904,2461300.8978,12.25,0.05,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 185844269987467904 20260917.3978 12.25CV 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 09 17.3978 2461300.8978 12.26 04:57:08.10 +34:47:46.0
169.32202 -5.12726 galactic Aur Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:08.10 +34:47:46.0 (user input) | T | P | (position from user input) J-Ks=0.671+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:08.10 +34:47:46.0: 13.43 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:08.10 +34:47:46.0: 13.45 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.26CV 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 09 17.3978 2461300.8978 12.25 04:57:13.54 +34:52:29.0
169.27166 -5.06394 galactic Aur Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.3034+34.8710 | 04:57:13.54 +34:52:29.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.341+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:13.54 +34:52:29.0: 13.42 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:13.54 +34:52:29.0: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J074.3034+34.8710,2461300.8978,12.25,0.05,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 J074.3034+34.8710 20260917.3978 12.25CV 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 09 17.3978 2461300.8978 13.29 04:58:36.01 +36:07:09.7
168.46452 -4.07396 galactic Aur Second-epoch detections are separated by 2.8" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:36.01 +36:07:09.7 (user input) | T | P | (position from user input) J-Ks=0.586+/-0.033 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:36.01 +36:07:09.7: 14.68 +/- 0.10 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:36.01 +36:07:09.7: 14.59 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.29,0.05,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 20260917.3978 13.29CV 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 09 17.3978 2461300.8978 12.27 04:57:59.51 +35:52:27.6
168.58129 -4.32218 galactic Aur Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:59.51 +35:52:27.6 (user input) | T | P | (position from user input) J-Ks=0.937+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:59.51 +35:52:27.6: 13.43 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:59.51 +35:52:27.6: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.27CV 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 09 17.3978 2461300.8978 12.18 04:57:45.79 +34:28:02.7
169.66154 -5.22925 galactic Aur Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4376+34.4703 | 04:57:45.79 +34:28:02.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.485+/-0.025 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:45.79 +34:28:02.7: 13.43 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:45.79 +34:28:02.7: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J074.4376+34.4703,2461300.8978,12.18,0.05,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
ATO J074.4376+34.4703 20260917.3978 12.18CV 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 09 17.3978 2461300.8978 12.45 04:56:36.96 +35:36:36.6
168.61540 -4.70502 galactic Aur Second-epoch detections are separated by 2.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1560+35.6137 | 04:56:34.20 +35:36:57.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:36.96 +35:36:36.6: 13.43 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:36.96 +35:36:36.6: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J074.1560+35.6137,2461300.8978,12.45,0.05,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 J074.1560+35.6137 20260917.3978 12.45CV 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 09 17.3978 2461300.8978 12.34 04:58:52.58 +35:32:46.9
168.95117 -4.38367 galactic Aur Second-epoch detections are separated by 1.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:52.58 +35:32:46.9 (user input) | T | P | (position from user input) SpType: A3IV (LAMOST DR5) J-Ks=0.352+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:52.58 +35:32:46.9: 13.43 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:52.58 +35:32:46.9: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.34CV 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 09 17.3978 2461300.8978 12.36 04:55:19.25 +35:34:22.5
168.48000 -4.93418 galactic Aur Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:19.25 +35:34:22.5 (user input) | T | P | (position from user input) J-Ks=0.440+/-0.025 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:19.25 +35:34:22.5: 13.42 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:19.25 +35:34:22.5: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.36,0.05,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 20260917.3978 12.36CV 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 09 17.3978 2461300.8978 12.12 04:56:00.39 +34:26:27.8
169.45678 -5.52971 galactic Aur Second-epoch detections are separated by 2.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:00.39 +34:26:27.8 (user input) | T | P | (position from user input) J-Ks=0.903+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:00.39 +34:26:27.8: 13.42 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:00.39 +34:26:27.8: 13.35 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.12CV 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 09 17.3978 2461300.8978 12.30 04:58:04.62 +35:46:23.9
168.67159 -4.37114 galactic Aur Second-epoch detections are separated by 0.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:04.62 +35:46:23.9 (user input) | T | P | (position from user input) J-Ks=1.126+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:04.62 +35:46:23.9: 13.40 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:04.62 +35:46:23.9: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 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
target,2461300.8978,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.30CV 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 09 17.3978 2461300.8978 12.15 04:58:55.59 +35:58:34.9
168.61812 -4.11037 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:55.59 +35:58:34.9 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.033 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:55.59 +35:58:34.9: 13.40 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:55.59 +35:58:34.9: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.15,0.05,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 20260917.3978 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 09 17.3978 2461300.8978 12.24 04:55:19.66 +35:26:33.7
168.58297 -5.01440 galactic Aur Second-epoch detections are separated by 1.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:19.66 +35:26:33.7 (user input) | T | P | (position from user input) J-Ks=1.197+/-0.026 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:19.66 +35:26:33.7: 13.41 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:19.66 +35:26:33.7: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.24,0.05,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 20260917.3978 12.24CV 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 09 17.3978 2461300.8978 12.15 04:56:36.85 +34:37:33.4
169.38937 -5.31677 galactic Aur Second-epoch detections are separated by 3.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:36.85 +34:37:33.4 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.029 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:36.85 +34:37:33.4: 13.34 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:36.85 +34:37:33.4: 13.35 +/- 0.04 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,2461300.8978,12.15,0.05,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 20260917.3978 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 09 17.3978 2461300.8978 12.39 04:55:40.63 +35:36:40.5
168.49531 -4.85365 galactic Aur Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.9196+35.6113 | 04:55:40.63 +35:36:40.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.550+/-0.025 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:40.63 +35:36:40.5: 13.41 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:40.63 +35:36:40.5: 13.44 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J073.9196+35.6113,2461300.8978,12.39,0.05,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
ATO J073.9196+35.6113 20260917.3978 12.39CV 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 09 17.3978 2461300.8978 12.27 04:58:36.85 +35:06:13.1
169.26760 -4.69889 galactic Aur Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:36.85 +35:06:13.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.958+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:36.85 +35:06:13.1: 13.38 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:36.85 +35:06:13.1: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.27CV 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 09 17.3978 2461300.8978 12.43 04:59:58.79 +36:49:24.1
168.08053 -3.42148 galactic Aur Second-epoch detections are separated by 1.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:58.79 +36:49:24.1 (user input) | T | P | (position from user input) J-Ks=1.364+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:58.79 +36:49:24.1: 13.42 +/- 0.04 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:58.79 +36:49:24.1: 13.36 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.43CV 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 09 17.3978 2461300.8978 12.25 04:58:41.28 +35:28:39.6
168.98167 -4.45622 galactic Aur Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:41.28 +35:28:39.6 (user input) | T | P | (position from user input) J-Ks=0.909+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:41.28 +35:28:39.6: 13.39 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:41.28 +35:28:39.6: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.25CV 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 09 17.3978 2461300.8978 12.51 04:53:51.72 +35:56:38.2
168.00363 -4.93261 galactic Aur Second-epoch detections are separated by 0.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:53:51.72 +35:56:38.2 (user input) | T | P | (position from user input) J-Ks=0.321+/-0.033 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:51.72 +35:56:38.2: 13.39 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:51.72 +35:56:38.2: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.51,0.05,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 20260917.3978 12.51CV 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 09 17.3978 2461300.8978 12.33 04:57:34.14 +34:07:14.4
169.91037 -5.47515 galactic Aur Second-epoch detections are separated by 1.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:34.14 +34:07:14.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.909+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:34.14 +34:07:14.4: 13.39 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:34.14 +34:07:14.4: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.33CV 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 09 17.3978 2461300.8978 12.15 04:55:54.39 +34:34:17.7
169.34123 -5.46464 galactic Aur Second-epoch detections are separated by 0.4" and 7.5 pix
The object was found in VSX 1" ASASSN-V J045554.50+343417.5
Type: SRS
# Max. Min./Amp. JD0 Period
13.920 V 14.040 V 2457458.78400 26.558000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:54.39 +34:34:17.7: 13.40 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:54.39 +34:34:17.7: 13.43 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045554.50+343417.5,2461300.8978,12.15,0.05,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
ASASSN-V J045554.50+343417.5 20260917.3978 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 09 17.3978 2461300.8978 12.26 04:59:46.38 +36:11:18.9
168.55623 -3.84490 galactic Aur Second-epoch detections are separated by 1.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:46.38 +36:11:18.9 (user input) | T | P | (position from user input) J-Ks=1.091+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:46.38 +36:11:18.9: 13.37 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:46.38 +36:11:18.9: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.26CV 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 09 17.3978 2461300.8978 12.27 04:55:43.91 +35:28:49.5
168.60492 -4.92655 galactic Aur Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:43.91 +35:28:49.5 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.025 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:43.91 +35:28:49.5: 13.38 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:43.91 +35:28:49.5: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.27CV 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 09 17.3978 2461300.8978 12.44 04:54:46.79 +35:55:01.9
168.14144 -4.80462 galactic Aur Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.6951+35.9171 | 04:54:46.79 +35:55:01.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.104+/-0.032 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:46.79 +35:55:01.9: 13.36 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:46.79 +35:55:01.9: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.6951+35.9171,2461300.8978,12.44,0.05,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
ATO J073.6951+35.9171 20260917.3978 12.44CV 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 09 17.3978 2461300.8978 12.14 04:57:18.11 +34:50:37.6
169.30576 -5.07085 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:18.11 +34:50:37.6 (user input) | T | P | (position from user input) J-Ks=1.180+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:18.11 +34:50:37.6: 13.36 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:18.11 +34:50:37.6: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.14CV 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 09 17.3978 2461300.8978 12.36 04:59:41.14 +36:39:34.0
168.17358 -3.56884 galactic Aur Second-epoch detections are separated by 0.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:41.14 +36:39:34.0 (user input) | T | P | (position from user input) J-Ks=0.792+/-0.024 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:41.14 +36:39:34.0: 13.36 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:41.14 +36:39:34.0: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.36,0.05,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 20260917.3978 12.36CV 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 09 17.3978 2461300.8978 12.23 04:58:02.42 +33:58:36.8
170.08454 -5.48718 galactic Aur Second-epoch detections are separated by 0.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:02.42 +33:58:36.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.378+/-0.024 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:02.42 +33:58:36.8: 13.36 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:02.42 +33:58:36.8: 13.34 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.23CV 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 09 17.3978 2461300.8978 12.14 04:56:39.49 +34:38:58.2
169.37646 -5.29505 galactic Aur Second-epoch detections are separated by 1.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185844269987467904 | 04:56:41.59 +34:38:40.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3 1949AnHar.112....1C HD 280266
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:39.49 +34:38:58.2: 13.28 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:39.49 +34:38:58.2: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185844269987467904,2461300.8978,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 185844269987467904 20260917.3978 12.14CV 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 09 17.3978 2461300.8978 12.09 04:59:01.15 +35:40:04.6
168.87314 -4.28584 galactic Aur Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:01.15 +35:40:04.6 (user input) | T | P | (position from user input) J-Ks=0.875+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:01.15 +35:40:04.6: 13.33 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:01.15 +35:40:04.6: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.09CV 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 09 17.3978 2461300.8978 12.06 04:58:35.08 +34:51:36.0
169.45627 -4.85395 galactic Aur Second-epoch detections are separated by 0.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.6477+34.8583 | 04:58:35.08 +34:51:36.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.250+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:35.08 +34:51:36.0: 13.34 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:35.08 +34:51:36.0: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.6477+34.8583,2461300.8978,12.06,0.05,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 J074.6477+34.8583 20260917.3978 12.06CV 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 09 17.3978 2461300.8978 12.44 04:56:36.99 +36:02:52.3
168.27161 -4.43274 galactic Aur Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:36.99 +36:02:52.3 (user input) | T | P | (position from user input) J-Ks=0.398+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:36.99 +36:02:52.3: 13.34 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:36.99 +36:02:52.3: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.44CV 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 09 17.3978 2461300.8978 12.32 04:54:35.18 +35:49:45.9
168.18551 -4.89014 galactic Aur Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:35.18 +35:49:45.9 (user input) | T | P | (position from user input) J-Ks=0.954+/-0.025 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:35.18 +35:49:45.9: 13.32 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:35.18 +35:49:45.9: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.32,0.05,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 20260917.3978 12.32CV 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 09 17.3978 2461300.8978 12.03 04:55:24.29 +35:22:43.0
168.64308 -5.04211 galactic Aur Second-epoch detections are separated by 0.7" and 7.2 pix
The object was found in VSX 1" ZTF J045524.36+352242.2
Type: SR
# Max. Min./Amp. JD0 Period
12.786 r Y 0.180 r 2458379.27570 236.556845300000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:24.29 +35:22:43.0: 13.33 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:24.29 +35:22:43.0: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J045524.36+352242.2,2461300.8978,12.03,0.05,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
ZTF J045524.36+352242.2 20260917.3978 12.03CV 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 09 17.3978 2461300.8978 12.29 04:54:36.91 +35:31:50.7
168.42296 -5.07256 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.6540+35.5304 | 04:54:36.91 +35:31:50.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.972+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:36.91 +35:31:50.7: 13.31 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:36.91 +35:31:50.7: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.6540+35.5304,2461300.8978,12.29,0.05,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 J073.6540+35.5304 20260917.3978 12.29CV 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 09 17.3978 2461300.8978 12.37 04:54:55.75 +35:07:55.2
168.77560 -5.27196 galactic Aur Second-epoch detections are separated by 1.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.7323+35.1322 | 04:54:55.75 +35:07:55.2 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.315+/-0.029 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:55.75 +35:07:55.2: 13.34 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:55.75 +35:07:55.2: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.7323+35.1322,2461300.8978,12.37,0.05,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 J073.7323+35.1322 20260917.3978 12.37CV 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 09 17.3978 2461300.8978 12.28 04:55:19.62 +35:02:58.0
168.89139 -5.25994 galactic Aur Second-epoch detections are separated by 1.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:19.62 +35:02:58.0 (user input) | T | P | (position from user input) J-Ks=1.269+/-0.025 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:19.62 +35:02:58.0: 13.31 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:19.62 +35:02:58.0: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.28CV 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 09 17.3978 2461300.8978 12.31 04:59:57.62 +36:45:31.5
168.12914 -3.46432 galactic Aur Second-epoch detections are separated by 0.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:57.62 +36:45:31.5 (user input) | T | P | (position from user input) J-Ks=0.530+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:57.62 +36:45:31.5: 13.34 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:57.62 +36:45:31.5: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.31CV 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 09 17.3978 2461300.8978 12.18 04:58:41.68 +35:50:02.3
168.70139 -4.23520 galactic Aur Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.6727+35.8357 | 04:58:41.68 +35:50:02.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.324+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:41.68 +35:50:02.3: 13.32 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:41.68 +35:50:02.3: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.6727+35.8357,2461300.8978,12.18,0.05,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
ATO J074.6727+35.8357 20260917.3978 12.18CV 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 09 17.3978 2461300.8978 12.22 04:55:40.91 +34:30:10.4
169.36632 -5.54361 galactic Aur Second-epoch detections are separated by 0.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:40.91 +34:30:10.4 (user input) | T | P | (position from user input) J-Ks=0.325+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:40.91 +34:30:10.4: 13.32 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:40.91 +34:30:10.4: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.22CV 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 09 17.3978 2461300.8978 12.25 04:56:15.01 +34:50:49.3
169.16873 -5.23802 galactic Aur Second-epoch detections are separated by 1.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:15.01 +34:50:49.3 (user input) | T | P | (position from user input) J-Ks=1.060+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:15.01 +34:50:49.3: 13.31 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:15.01 +34:50:49.3: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.25CV 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 09 17.3978 2461300.8978 12.41 04:57:28.08 +35:51:45.0
168.52466 -4.41282 galactic Aur Second-epoch detections are separated by 1.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:28.08 +35:51:45.0 (user input) | T | P | (position from user input) J-Ks=0.846+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:28.08 +35:51:45.0: 13.30 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:28.08 +35:51:45.0: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.41,0.05,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 20260917.3978 12.41CV 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 09 17.3978 2461300.8978 12.21 04:59:31.44 +36:35:39.8
168.20490 -3.63447 galactic Aur Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:31.44 +36:35:39.8 (user input) | T | P | (position from user input) J-Ks=0.846+/-0.031 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:31.44 +36:35:39.8: 13.31 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:31.44 +36:35:39.8: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.21CV 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 09 17.3978 2461300.8978 12.19 04:58:31.29 +36:18:32.2
168.30528 -3.96926 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:31.29 +36:18:32.2 (user input) | T | P | (position from user input) J-Ks=0.346+/-0.032 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:31.29 +36:18:32.2: 13.30 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:31.29 +36:18:32.2: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.19CV 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 09 17.3978 2461300.8978 12.14 04:58:41.26 +34:53:59.2
169.43793 -4.81279 galactic Aur Second-epoch detections are separated by 0.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185827880393322112 | 04:58:38.71 +34:53:45.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1949AnHar.112....1C HD 280328 J-Ks=0.895+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:41.26 +34:53:59.2: 13.26 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:41.26 +34:53:59.2: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185827880393322112,2461300.8978,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 185827880393322112 20260917.3978 12.14CV 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 09 17.3978 2461300.8978 12.16 04:56:46.06 +34:16:33.7
169.68474 -5.50906 galactic Aur Second-epoch detections are separated by 1.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:46.06 +34:16:33.7 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:46.06 +34:16:33.7: 13.30 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:46.06 +34:16:33.7: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.16,0.05,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 20260917.3978 12.16CV 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 09 17.3978 2461300.8978 12.07 04:58:00.39 +34:52:51.4
169.36625 -4.93430 galactic Aur Second-epoch detections are separated by 2.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:00.39 +34:52:51.4 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.601+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:00.39 +34:52:51.4: 13.28 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:00.39 +34:52:51.4: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.07,0.05,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 20260917.3978 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 09 17.3978 2461300.8978 12.29 04:57:58.94 +36:13:02.9
168.30990 -4.11124 galactic Aur Second-epoch detections are separated by 0.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4958+36.2167 | 04:57:58.94 +36:13:02.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:58.94 +36:13:02.9: 13.27 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:58.94 +36:13:02.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.4958+36.2167,2461300.8978,12.29,0.05,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 J074.4958+36.2167 20260917.3978 12.29CV 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 09 17.3978 2461300.8978 12.14 04:58:51.51 +36:01:23.2
168.57273 -4.09234 galactic Aur Second-epoch detections are separated by 0.5" and 7.3 pix
The object was found in VSX 0" Gaia DR3 186206589132015232
Type: ROT
# Max. Min./Amp. JD0 Period
12.970 G 13.000 G G
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:51.51 +36:01:23.2: 13.27 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:51.51 +36:01:23.2: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186206589132015232,2461300.8978,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 186206589132015232 20260917.3978 12.14CV 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 09 17.3978 2461300.8978 12.05 04:59:13.20 +35:54:16.3
168.71154 -4.10791 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.8055+35.9041 | 04:59:13.20 +35:54:16.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.165+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:13.20 +35:54:16.3: 13.25 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:13.20 +35:54:16.3: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.8055+35.9041,2461300.8978,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.8055+35.9041 20260917.3978 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.06 04:56:45.91 +34:15:07.6
169.70327 -5.52430 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:45.91 +34:15:07.6 (user input) | T | P | (position from user input) J-Ks=0.986+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:45.91 +34:15:07.6: 13.24 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:45.91 +34:15:07.6: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.06,0.05,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
target 20260917.3978 12.06CV 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 09 17.3978 2461300.8978 12.22 04:54:52.89 +35:40:11.5
168.34803 -4.94329 galactic Aur Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:52.89 +35:40:11.5 (user input) | T | P | (position from user input) J-Ks=0.309+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:52.89 +35:40:11.5: 13.26 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:52.89 +35:40:11.5: 13.32 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.22CV 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 09 17.3978 2461300.8978 12.07 04:58:21.94 +34:26:26.1
169.75975 -5.14814 galactic Aur Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.852 Wladilena -566 122 579 14.5 -0 0
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:21.94 +34:26:26.1: 13.22 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:21.94 +34:26:26.1: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461300.8978,12.07,0.05,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
VARIABLE_NAME 20260917.3978 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 09 17.3978 2461300.8978 12.29 04:56:50.77 +35:50:18.3
168.46514 -4.52656 galactic Aur Second-epoch detections are separated by 0.6" and 7.1 pix
The object was found in VSX 1" Gaia DR3 186119903809124352
Type: ROT
# Max. Min./Amp. JD0 Period
12.920 G 12.940 G G
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:50.77 +35:50:18.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:50.77 +35:50:18.3: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186119903809124352,2461300.8978,12.29,0.05,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 186119903809124352 20260917.3978 12.29CV 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 09 17.3978 2461300.8978 12.02 04:56:44.17 +34:39:21.3
169.38141 -5.27849 galactic Aur Second-epoch detections are separated by 1.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:44.17 +34:39:21.3 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:44.17 +34:39:21.3: 13.26 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:44.17 +34:39:21.3: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.02CV 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 09 17.3978 2461300.8978 12.27 04:55:10.48 +34:43:43.6
169.12351 -5.48442 galactic Aur Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:10.48 +34:43:43.6 (user input) | T | P | (position from user input) J-Ks=0.439+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:10.48 +34:43:43.6: 13.20 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:10.48 +34:43:43.6: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.27CV 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 09 17.3978 2461300.8978 12.15 04:59:42.67 +36:26:04.0
168.35437 -3.70337 galactic Aur Second-epoch detections are separated by 1.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:42.67 +36:26:04.0 (user input) | T | P | (position from user input) J-Ks=0.363+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:42.67 +36:26:04.0: 13.19 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:42.67 +36:26:04.0: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.15,0.05,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 20260917.3978 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 09 17.3978 2461300.8978 12.11 04:58:13.85 +34:34:58.5
169.63009 -5.08215 galactic Aur Second-epoch detections are separated by 0.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:13.85 +34:34:58.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.505+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:13.85 +34:34:58.5: 13.19 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:13.85 +34:34:58.5: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.11CV 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 09 17.3978 2461300.8978 12.00 04:55:57.06 +35:00:06.9
169.00866 -5.18966 galactic Aur Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185868351867772288 | 04:55:57.11 +35:00:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.173+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:57.06 +35:00:06.9: 13.18 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:57.06 +35:00:06.9: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.18 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185868351867772288,2461300.8978,12.00,0.05,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
Gaia DR3 185868351867772288 20260917.3978 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 09 17.3978 2461300.8978 11.98 04:59:07.74 +35:58:56.1
168.63881 -4.07449 galactic Aur Second-epoch detections are separated by 0.2" and 7.3 pix
The object was found in VSX24" ZTF J045906.84+355834.7
Type: HADS
# Max. Min./Amp. JD0 Period
17.744 r Y 0.517 r 2458366.98340 0.088965100000
ATTENTION: measured mag 11.98 is 5.2 mag brighter than the VSX record maximum brightness 17.23 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:07.74 +35:58:56.1: 13.17 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:07.74 +35:58:56.1: 13.21 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J045906.84+355834.7,2461300.8978,11.98,0.05,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
ZTF J045906.84+355834.7 20260917.3978 11.98CV 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 09 17.3978 2461300.8978 11.96 04:58:34.83 +34:52:58.4
169.43767 -4.84051 galactic Aur Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:34.83 +34:52:58.4 (user input) | T | P | (position from user input) J-Ks=0.488+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:34.83 +34:52:58.4: 13.17 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:34.83 +34:52:58.4: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,11.96,0.05,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
target 20260917.3978 11.96CV 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 09 17.3978 2461300.8978 12.05 04:56:46.52 +33:23:05.7
170.38875 -6.05996 galactic Aur Second-epoch detections are separated by 1.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1967+33.3831 | 04:56:49.55 +33:23:12.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.434+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:46.52 +33:23:05.7: 13.11 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:46.52 +33:23:05.7: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.1967+33.3831,2461300.8978,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.1967+33.3831 20260917.3978 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.04 04:56:59.61 +34:28:47.8
169.55304 -5.34608 galactic Aur Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 161773280393713024 | 04:56:59.61 +34:28:47.8 (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: A5V (LAMOST DR5) J-Ks=0.357+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:59.61 +34:28:47.8: 13.17 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:59.61 +34:28:47.8: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 161773280393713024,2461300.8978,12.04,0.05,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
Large-amplitude variable Gaia DR2 161773280393713024 20260917.3978 12.04CV 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 09 17.3978 2461300.8978 12.17 04:59:51.47 +36:45:37.2
168.11523 -3.47952 galactic Aur Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.9646+36.7604 | 04:59:51.47 +36:45:37.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.081+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:51.47 +36:45:37.2: 13.16 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:51.47 +36:45:37.2: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.9646+36.7604,2461300.8978,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.9646+36.7604 20260917.3978 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.12 04:53:49.10 +35:26:42.2
168.38794 -5.25267 galactic Aur Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.4550+35.4447 | 04:53:49.21 +35:26:41.1 (Gaia DR3) | IRR (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.542+/-0.030 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:49.10 +35:26:42.2: 13.14 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:49.10 +35:26:42.2: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.4550+35.4447,2461300.8978,12.12,0.05,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
ATO J073.4550+35.4447 20260917.3978 12.12CV 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 09 17.3978 2461300.8978 11.99 04:58:47.09 +35:47:40.9
168.74369 -4.24507 galactic Aur Second-epoch detections are separated by 1.7" and 7.2 pix
The object was found in VSX 1" Gaia DR3 186010498106765952
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.970 G 13.000 G B
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:47.09 +35:47:40.9: 13.14 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:47.09 +35:47:40.9: 13.11 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186010498106765952,2461300.8978,11.99,0.05,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 186010498106765952 20260917.3978 11.99CV 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 09 17.3978 2461300.8978 12.17 04:56:59.98 +34:13:07.7
169.75971 -5.50691 galactic Aur Second-epoch detections are separated by 1.1" and 7.4 pix
The object was found in VSX 0" TSVSC1 TN-N301120011-15-82-2
Type: VAR
# Max. Min./Amp. JD0 Period
12.620 R 0.812600000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:59.98 +34:13:07.7: 13.13 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:59.98 +34:13:07.7: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TSVSC1 TN-N301120011-15-82-2,2461300.8978,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TSVSC1 TN-N301120011-15-82-2 20260917.3978 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.23 04:56:22.74 +36:02:39.8
168.24437 -4.47248 galactic Aur Second-epoch detections are separated by 0.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:22.74 +36:02:39.8 (user input) | T | P | (position from user input) J-Ks=0.639+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:22.74 +36:02:39.8: 13.10 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:22.74 +36:02:39.8: 13.05 +/- 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,2461300.8978,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.23CV 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 09 17.3978 2461300.8978 11.82 04:59:16.11 +35:41:23.0
168.88724 -4.23254 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:16.11 +35:41:23.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.997+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:16.11 +35:41:23.0: 13.11 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:16.11 +35:41:23.0: 13.09 +/- 0.03 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,2461300.8978,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 11.87 04:57:48.25 +34:18:44.0
169.78930 -5.31853 galactic Aur Second-epoch detections are separated by 0.5" and 7.3 pix
The object was found in VSX11" Gaia DR3 161755718272891776
Type: E
# Max. Min./Amp. JD0 Period
18.370 G 18.910 G 1.180790000000
ATTENTION: measured mag 11.87 is 6.5 mag brighter than the VSX record maximum brightness 18.37 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:48.25 +34:18:44.0: 13.10 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:48.25 +34:18:44.0: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 161755718272891776,2461300.8978,11.87,0.05,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 161755718272891776 20260917.3978 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 09 17.3978 2461300.8978 11.84 04:59:13.58 +35:50:02.2
168.76806 -4.15040 galactic Aur Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186015617707782144 | 04:59:13.69 +35:50:00.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.260+/-0.027 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:13.58 +35:50:02.2: 13.08 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:13.58 +35:50:02.2: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186015617707782144,2461300.8978,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 186015617707782144 20260917.3978 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.15 04:54:09.02 +35:39:48.7
168.25963 -5.06303 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:09.02 +35:39:48.7 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.026 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:09.02 +35:39:48.7: 13.06 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:09.02 +35:39:48.7: 13.08 +/- 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,2461300.8978,12.15,0.05,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 20260917.3978 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 09 17.3978 2461300.8978 13.27 04:56:22.90 +34:54:46.8
169.13368 -5.17588 galactic Aur Second-epoch detections are separated by 1.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.0972+34.9148 | 04:56:22.90 +34:54:46.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.153+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:22.90 +34:54:46.8: 14.49 +/- 0.09 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:22.90 +34:54:46.8: 14.50 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.50 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.0972+34.9148,2461300.8978,13.27,0.05,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
ATO J074.0972+34.9148 20260917.3978 13.27CV 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 09 17.3978 2461300.8978 11.96 04:55:05.07 +35:20:34.4
168.63016 -5.11543 galactic Aur Second-epoch detections are separated by 0.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:05.07 +35:20:34.4 (user input) | T | P | (position from user input) J-Ks=0.415+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:05.07 +35:20:34.4: 13.06 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:05.07 +35:20:34.4: 13.10 +/- 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,2461300.8978,11.96,0.05,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
target 20260917.3978 11.96CV 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 09 17.3978 2461300.8978 11.91 04:59:14.39 +36:12:09.7
168.47868 -3.92094 galactic Aur Second-epoch detections are separated by 1.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.8099+36.2032 | 04:59:14.39 +36:12:09.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.043+/-0.034 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:14.39 +36:12:09.7: 13.05 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:14.39 +36:12:09.7: 13.00 +/- 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
ATO J074.8099+36.2032,2461300.8978,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.8099+36.2032 20260917.3978 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.00 04:54:23.69 +35:30:36.6
168.41089 -5.12041 galactic Aur Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.6120+35.5066 | 04:54:23.69 +35:30:36.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.504+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:23.69 +35:30:36.6: 13.06 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:23.69 +35:30:36.6: 13.08 +/- 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
ATO J073.6120+35.5066,2461300.8978,12.00,0.05,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
ATO J073.6120+35.5066 20260917.3978 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 09 17.3978 2461300.8978 12.14 04:54:25.89 +35:48:20.8
168.18427 -4.92942 galactic Aur Second-epoch detections are separated by 1.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186142336421450624 | 04:54:25.91 +35:48:20.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.959+/-0.025 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:25.89 +35:48:20.8: 13.05 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:25.89 +35:48:20.8: 13.06 +/- 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
Gaia DR3 186142336421450624,2461300.8978,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 186142336421450624 20260917.3978 12.14CV 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 09 17.3978 2461300.8978 11.96 04:58:38.49 +35:30:34.3
168.95067 -4.44400 galactic Aur Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185908591417363840 | 04:58:38.53 +35:30:33.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.021+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:38.49 +35:30:34.3: 13.04 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:38.49 +35:30:34.3: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185908591417363840,2461300.8978,11.96,0.05,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 185908591417363840 20260917.3978 11.96CV 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 09 17.3978 2461300.8978 12.11 04:56:06.35 +35:12:24.2
168.86752 -5.03738 galactic Aur Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:06.35 +35:12:24.2 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.569+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:06.35 +35:12:24.2: 13.04 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:06.35 +35:12:24.2: 13.14 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.11CV 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 09 17.3978 2461300.8978 12.10 04:54:33.72 +35:43:02.0
168.27020 -4.96425 galactic Aur Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.6406+35.7173 | 04:54:33.72 +35:43:02.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.526+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:33.72 +35:43:02.0: 13.02 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:33.72 +35:43:02.0: 13.07 +/- 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 J073.6406+35.7173,2461300.8978,12.10,0.05,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
ATO J073.6406+35.7173 20260917.3978 12.10CV 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 09 17.3978 2461300.8978 12.06 04:55:45.94 +35:21:31.0
168.70483 -4.99709 galactic Aur Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186069940451681536 | 04:55:46.07 +35:21:30.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.491+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:45.94 +35:21:31.0: 13.01 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:45.94 +35:21:31.0: 12.97 +/- 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
Gaia DR3 186069940451681536,2461300.8978,12.06,0.05,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 186069940451681536 20260917.3978 12.06CV 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 09 17.3978 2461300.8978 11.96 04:55:45.27 +35:38:07.6
168.48616 -4.82628 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:45.27 +35:38:07.6 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.025 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:45.27 +35:38:07.6: 13.02 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:45.27 +35:38:07.6: 13.04 +/- 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,2461300.8978,11.96,0.05,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
target 20260917.3978 11.96CV 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 09 17.3978 2461300.8978 12.08 04:59:57.26 +36:48:09.3
168.09379 -3.43829 galactic Aur Second-epoch detections are separated by 0.4" and 7.2 pix
The object was found in VSX15" Gaia DR3 186640831803065344
Type: ROT
# Max. Min./Amp. JD0 Period
15.220 G 15.250 G K
ATTENTION: measured mag 12.08 is 3.1 mag brighter than the VSX record maximum brightness 15.22 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:57.26 +36:48:09.3: 13.01 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:57.26 +36:48:09.3: 12.98 +/- 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 186640831803065344,2461300.8978,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 186640831803065344 20260917.3978 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 11.93 04:58:12.43 +34:18:27.4
169.84456 -5.25592 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5521+34.3049 | 04:58:12.43 +34:18:27.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.918+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:12.43 +34:18:27.4: 13.02 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:12.43 +34:18:27.4: 12.99 +/- 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
ATO J074.5521+34.3049,2461300.8978,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.5521+34.3049 20260917.3978 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 11.77 04:59:05.82 +35:49:46.8
168.75524 -4.17368 galactic Aur Second-epoch detections are separated by 0.5" and 7.2 pix
The object was found in VSX16" ZTF J045905.72+354931.1
Type: EW
# Max. Min./Amp. JD0 Period
17.302 r Y 0.205 r 2458437.84280 0.352619600000
ATTENTION: measured mag 11.77 is 5.3 mag brighter than the VSX record maximum brightness 17.10 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:05.82 +35:49:46.8: 13.01 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:05.82 +35:49:46.8: 13.00 +/- 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
ZTF J045905.72+354931.1,2461300.8978,11.77,0.05,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
ZTF J045905.72+354931.1 20260917.3978 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 09 17.3978 2461300.8978 11.88 04:56:42.84 +34:43:41.3
169.32170 -5.23724 galactic Aur Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1832+34.7180 | 04:56:42.84 +34:43:41.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.476+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:42.84 +34:43:41.3: 13.01 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:42.84 +34:43:41.3: 12.99 +/- 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
ATO J074.1832+34.7180,2461300.8978,11.88,0.05,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
ATO J074.1832+34.7180 20260917.3978 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 09 17.3978 2461300.8978 11.80 04:58:52.51 +35:50:15.2
168.72121 -4.20420 galactic Aur Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.7057+35.8442 | 04:58:52.51 +35:50:15.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.870+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:52.51 +35:50:15.2: 13.01 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:52.51 +35:50:15.2: 12.98 +/- 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
ATO J074.7057+35.8442,2461300.8978,11.80,0.05,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
ATO J074.7057+35.8442 20260917.3978 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 09 17.3978 2461300.8978 11.98 04:59:31.01 +36:43:25.3
168.10198 -3.55591 galactic Aur Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186265550442204544 | 04:59:33.87 +36:43:34.4 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE J-Ks=0.952+/-0.029 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:31.01 +36:43:25.3: 13.00 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:31.01 +36:43:25.3: 12.98 +/- 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
Gaia DR3 186265550442204544,2461300.8978,11.98,0.05,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 186265550442204544 20260917.3978 11.98CV 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 09 17.3978 2461300.8978 11.85 04:56:44.50 +34:40:03.7
169.37284 -5.27030 galactic Aur Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:44.50 +34:40:03.7 (user input) | T | P | (position from user input) J-Ks=0.279+/-0.030 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:44.50 +34:40:03.7: 13.00 +/- 0.03 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:44.50 +34:40:03.7: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,11.85,0.05,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 20260917.3978 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 09 17.3978 2461300.8978 11.88 04:56:33.27 +34:50:46.7
169.20827 -5.18954 galactic Aur Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:33.27 +34:50:46.7 (user input) | T | P | (position from user input) J-Ks=0.385+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:33.27 +34:50:46.7: 12.99 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:33.27 +34:50:46.7: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,11.88,0.05,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 20260917.3978 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 09 17.3978 2461300.8978 11.82 04:57:31.76 +34:31:51.0
169.58157 -5.22789 galactic Aur Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:31.76 +34:31:51.0 (user input) | T | P | (position from user input) J-Ks=0.404+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:31.76 +34:31:51.0: 12.97 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:31.76 +34:31:51.0: 12.94 +/- 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,2461300.8978,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 13.13 04:58:03.95 +34:31:19.4
169.65709 -5.14646 galactic Aur Second-epoch detections are separated by 2.7" and 7.0 pix
The object was found in VSX 2" Gaia DR3 185781803983215616
Type: ROT
# Max. Min./Amp. JD0 Period
14.070 G 14.100 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:03.95 +34:31:19.4: 14.47 +/- 0.09 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:03.95 +34:31:19.4: 14.36 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185781803983215616,2461300.8978,13.13,0.05,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 185781803983215616 20260917.3978 13.13CV 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 09 17.3978 2461300.8978 12.02 04:54:12.16 +35:39:33.6
168.26960 -5.05738 galactic Aur Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:12.16 +35:39:33.6 (user input) | T | P | (position from user input) J-Ks=0.604+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:12.16 +35:39:33.6: 12.95 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:12.16 +35:39:33.6: 12.92 +/- 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,2461300.8978,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.02CV 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 09 17.3978 2461300.8978 13.19 04:57:24.04 +35:06:27.5
169.11045 -4.89148 galactic Aur Second-epoch detections are separated by 4.6" and 7.9 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 | 04:57:24.04 +35:06:27.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:24.04 +35:06:27.5: 14.48 +/- 0.09 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:24.04 +35:06:27.5: 14.44 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.19CV 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 09 17.3978 2461300.8978 11.94 04:58:12.03 +36:04:51.6
168.44470 -4.16113 galactic Aur Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186222222812969984 | 04:58:12.10 +36:04:51.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.118+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:12.03 +36:04:51.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:12.03 +36:04:51.6: 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
Gaia DR3 186222222812969984,2461300.8978,11.94,0.05,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 186222222812969984 20260917.3978 11.94CV 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 09 17.3978 2461300.8978 11.81 04:57:03.17 +34:12:16.6
169.77774 -5.50707 galactic Aur Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 161756233668295168 | 04:57:03.21 +34:12:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=1.219+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:03.17 +34:12:16.6: 12.91 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:03.17 +34:12:16.6: 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 161756233668295168,2461300.8978,11.81,0.05,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 161756233668295168 20260917.3978 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 09 17.3978 2461300.8978 11.86 04:59:13.89 +36:17:30.8
168.40726 -3.86726 galactic Aur Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186237134938590208 | 04:59:13.90 +36:17:30.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.939+/-0.031 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:13.89 +36:17:30.8: 12.90 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:13.89 +36:17:30.8: 12.88 +/- 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
Gaia DR3 186237134938590208,2461300.8978,11.86,0.05,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
Gaia DR3 186237134938590208 20260917.3978 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 09 17.3978 2461300.8978 13.31 04:57:05.50 +34:31:10.6
169.53437 -5.30562 galactic Aur Second-epoch detections are separated by 1.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:05.50 +34:31:10.6 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5) J-Ks=0.500+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:05.50 +34:31:10.6: 14.46 +/- 0.09 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:05.50 +34:31:10.6: 14.50 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.31CV 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 09 17.3978 2461300.8978 11.88 04:55:39.53 +35:29:44.2
168.58370 -4.92869 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX 0" Gaia DR3 186084062304147200
Type: ROT
# Max. Min./Amp. JD0 Period
12.460 G 12.480 G G
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:39.53 +35:29:44.2: 12.88 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:39.53 +35:29:44.2: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 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 186084062304147200,2461300.8978,11.88,0.05,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
Gaia DR3 186084062304147200 20260917.3978 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 09 17.3978 2461300.8978 11.92 04:59:44.38 +36:43:21.0
168.13049 -3.52147 galactic Aur Second-epoch detections are separated by 0.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:44.38 +36:43:21.0 (user input) | T | P | (position from user input) J-Ks=0.558+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:44.38 +36:43:21.0: 12.86 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:44.38 +36:43:21.0: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 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
target,2461300.8978,11.92,0.05,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
target 20260917.3978 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 09 17.3978 2461300.8978 11.88 04:57:46.65 +35:41:59.3
168.69175 -4.46437 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:46.65 +35:41:59.3 (user input) | T | P | (position from user input) J-Ks=0.575+/-0.025 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:46.65 +35:41:59.3: 12.86 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:46.65 +35:41:59.3: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.85 +/- 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
target,2461300.8978,11.88,0.05,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 20260917.3978 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 09 17.3978 2461300.8978 11.73 04:58:22.94 +35:42:33.7
168.76041 -4.36200 galactic Aur Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5999+35.7102 | 04:58:22.94 +35:42:33.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.472+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:22.94 +35:42:33.7: 12.85 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:22.94 +35:42:33.7: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 J074.5999+35.7102,2461300.8978,11.73,0.05,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 J074.5999+35.7102 20260917.3978 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 09 17.3978 2461300.8978 11.78 04:59:35.36 +36:12:54.4
168.51242 -3.85776 galactic Aur Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186232977410250240 | 04:59:35.37 +36:12:54.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.907+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:35.36 +36:12:54.4: 12.84 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:35.36 +36:12:54.4: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186232977410250240,2461300.8978,11.78,0.05,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 186232977410250240 20260917.3978 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 09 17.3978 2461300.8978 11.71 04:59:20.58 +36:07:23.9
168.55420 -3.95348 galactic Aur Second-epoch detections are separated by 1.1" and 7.1 pix
The object was found in VSX 1" Gaia DR3 186232049697316096
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.500 G 12.590 G 0.156900600000 A
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:20.58 +36:07:23.9: 12.83 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:20.58 +36:07:23.9: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186232049697316096,2461300.8978,11.71,0.05,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
Gaia DR3 186232049697316096 20260917.3978 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 09 17.3978 2461300.8978 11.65 04:57:12.09 +34:38:24.6
169.45341 -5.21318 galactic Aur Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.3028+34.6388 | 04:57:12.09 +34:38:24.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1V (LAMOST DR5) J-Ks=0.602+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:12.09 +34:38:24.6: 12.81 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:12.09 +34:38:24.6: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 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 J074.3028+34.6388,2461300.8978,11.65,0.05,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 J074.3028+34.6388 20260917.3978 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 09 17.3978 2461300.8978 11.72 04:56:30.86 +34:15:42.8
169.66326 -5.55888 galactic Aur Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1293+34.2619 | 04:56:31.04 +34:15:43.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:30.86 +34:15:42.8: 12.81 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:30.86 +34:15:42.8: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.1293+34.2619,2461300.8978,11.72,0.05,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
ATO J074.1293+34.2619 20260917.3978 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 09 17.3978 2461300.8978 11.68 04:57:43.77 +34:22:45.1
169.72686 -5.28925 galactic Aur Second-epoch detections are separated by 1.5" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4359+34.3780 | 04:57:43.74 +34:22:45.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2V (LAMOST DR5) J-Ks=0.940+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:43.77 +34:22:45.1: 12.78 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:43.77 +34:22:45.1: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.4359+34.3780,2461300.8978,11.68,0.05,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
ATO J074.4359+34.3780 20260917.3978 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 09 17.3978 2461300.8978 13.05 04:58:15.65 +34:48:44.1
169.45282 -4.93571 galactic Aur Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:15.65 +34:48:44.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.881+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:15.65 +34:48:44.1: 14.42 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:15.65 +34:48:44.1: 14.40 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.05CV 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 09 17.3978 2461300.8978 11.70 04:54:43.46 +35:19:47.5
168.59427 -5.18091 galactic Aur Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186076228283803648 | 04:54:43.50 +35:19:47.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.403+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:43.46 +35:19:47.5: 12.77 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:43.46 +35:19:47.5: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186076228283803648,2461300.8978,11.70,0.05,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 186076228283803648 20260917.3978 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 09 17.3978 2461300.8978 13.14 04:54:41.92 +35:36:08.3
168.37760 -5.01454 galactic Aur Second-epoch detections are separated by 1.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:41.92 +35:36:08.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:41.92 +35:36:08.3: 14.34 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:41.92 +35:36:08.3: 14.44 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.39 +/- 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,2461300.8978,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.14CV 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 09 17.3978 2461300.8978 13.29 04:56:46.38 +35:45:30.6
168.51870 -4.58784 galactic Aur Second-epoch detections are separated by 2.2" and 7.0 pix
The object was found in VSX 1" Gaia DR3 186116983231373696
Type: L
# Max. Min./Amp. JD0 Period
13.850 G 14.010 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:46.38 +35:45:30.6: 14.41 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:46.38 +35:45:30.6: 14.33 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186116983231373696,2461300.8978,13.29,0.05,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 186116983231373696 20260917.3978 13.29CV 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 09 17.3978 2461300.8978 11.60 04:57:05.84 +34:40:59.3
169.40621 -5.20336 galactic Aur Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185799121291231616 | 04:57:05.78 +34:40:59.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=0.455+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:05.84 +34:40:59.3: 12.75 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:05.84 +34:40:59.3: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185799121291231616,2461300.8978,11.60,0.05,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
Gaia DR3 185799121291231616 20260917.3978 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 09 17.3978 2461300.8978 12.96 04:59:32.31 +36:05:05.4
168.60897 -3.94608 galactic Aur Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:32.31 +36:05:05.4 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.032 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:32.31 +36:05:05.4: 14.39 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:32.31 +36:05:05.4: 14.24 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.96,0.05,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
target 20260917.3978 12.96CV 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 09 17.3978 2461300.8978 13.05 04:57:15.18 +34:40:32.4
169.43201 -5.18287 galactic Aur Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:15.18 +34:40:32.4 (user input) | T | P | (position from user input) J-Ks=0.994+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:15.18 +34:40:32.4: 14.39 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:15.18 +34:40:32.4: 14.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.32 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.05CV 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 09 17.3978 2461300.8978 11.79 04:57:30.14 +35:06:36.5
169.12141 -4.87360 galactic Aur Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185861140618741248 | 04:57:30.16 +35:06:36.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.688+/-0.023 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:30.14 +35:06:36.5: 12.73 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:30.14 +35:06:36.5: 12.74 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185861140618741248,2461300.8978,11.79,0.05,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 185861140618741248 20260917.3978 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 09 17.3978 2461300.8978 12.96 04:58:35.64 +35:04:19.8
169.28990 -4.72155 galactic Aur Second-epoch detections are separated by 2.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:35.64 +35:04:19.8 (user input) | T | P | (position from user input) J-Ks=0.354+/-0.031 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:35.64 +35:04:19.8: 14.43 +/- 0.09 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:35.64 +35:04:19.8: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.96,0.05,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
target 20260917.3978 12.96CV 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 09 17.3978 2461300.8978 11.46 04:59:28.13 +35:54:04.1
168.74535 -4.07031 galactic Aur Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.8675+35.9009 | 04:59:28.21 +35:54:03.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.256+/-0.035 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:28.13 +35:54:04.1: 12.71 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:28.13 +35:54:04.1: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.8675+35.9009,2461300.8978,11.46,0.05,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 J074.8675+35.9009 20260917.3978 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 09 17.3978 2461300.8978 13.29 04:53:46.43 +35:39:21.7
168.21732 -5.12729 galactic Aur Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.4439+35.6553 | 04:53:46.43 +35:39:21.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:46.43 +35:39:21.7: 14.41 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:46.43 +35:39:21.7: 14.42 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J073.4439+35.6553,2461300.8978,13.29,0.05,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 J073.4439+35.6553 20260917.3978 13.29CV 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 09 17.3978 2461300.8978 13.18 04:55:06.80 +35:27:13.8
168.54687 -5.04153 galactic Aur Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:06.80 +35:27:13.8 (user input) | T | P | (position from user input) J-Ks=1.504+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:06.80 +35:27:13.8: 14.37 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:06.80 +35:27:13.8: 14.33 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.36 +/- 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,2461300.8978,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.18CV 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 09 17.3978 2461300.8978 11.54 04:57:34.38 +34:34:55.8
169.54666 -5.18906 galactic Aur Second-epoch detections are separated by 1.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185794478429347200 | 04:57:34.38 +34:34:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5) J-Ks=1.026+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:34.38 +34:34:55.8: 12.69 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:34.38 +34:34:55.8: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185794478429347200,2461300.8978,11.54,0.05,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 185794478429347200 20260917.3978 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 09 17.3978 2461300.8978 11.77 04:57:50.71 +36:07:24.9
168.36662 -4.19113 galactic Aur Second-epoch detections are separated by 0.4" and 7.2 pix
The object was found in VSX 9" Gaia DR3 186217584248287872
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.490 G 14.540 G A
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:50.71 +36:07:24.9: 12.70 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:50.71 +36:07:24.9: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186217584248287872,2461300.8978,11.77,0.05,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
Gaia DR3 186217584248287872 20260917.3978 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 09 17.3978 2461300.8978 11.61 04:59:20.57 +36:06:20.0
168.56820 -3.96445 galactic Aur Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186231980977839616 | 04:59:20.61 +36:06:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.923+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:20.57 +36:06:20.0: 12.69 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:20.57 +36:06:20.0: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186231980977839616,2461300.8978,11.61,0.05,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 186231980977839616 20260917.3978 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 09 17.3978 2461300.8978 13.18 04:59:06.78 +35:44:46.4
168.82312 -4.22258 galactic Aur Second-epoch detections are separated by 1.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:06.78 +35:44:46.4 (user input) | T | P | (position from user input) J-Ks=0.372+/-0.032 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:06.78 +35:44:46.4: 14.40 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:06.78 +35:44:46.4: 14.43 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.18CV 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 09 17.3978 2461300.8978 13.17 04:59:46.13 +36:24:20.8
168.38417 -3.71187 galactic Aur Second-epoch detections are separated by 2.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.9428+36.4148 | 04:59:46.13 +36:24:20.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.549+/-0.030 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:46.13 +36:24:20.8: 14.38 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:46.13 +36:24:20.8: 14.51 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.9428+36.4148,2461300.8978,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.9428+36.4148 20260917.3978 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 13.18 04:55:34.81 +34:51:24.4
169.07514 -5.33952 galactic Aur Second-epoch detections are separated by 2.0" and 7.4 pix
The object was found in VSX 1" Gaia DR3 161846604077106688
Type: ROT
# Max. Min./Amp. JD0 Period
14.000 G 14.020 G G
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:34.81 +34:51:24.4: 14.40 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:34.81 +34:51:24.4: 14.28 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.34 +/- 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
Gaia DR3 161846604077106688,2461300.8978,13.18,0.05,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 161846604077106688 20260917.3978 13.18CV 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 09 17.3978 2461300.8978 12.87 04:57:43.34 +34:47:36.3
169.39910 -5.03425 galactic Aur Second-epoch detections are separated by 1.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:43.34 +34:47:36.3 (user input) | T | P | (position from user input) SpType: G9 (LAMOST DR5) J-Ks=0.675+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:43.34 +34:47:36.3: 14.37 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:43.34 +34:47:36.3: 14.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 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,2461300.8978,12.87,0.05,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 20260917.3978 12.87CV 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 09 17.3978 2461300.8978 11.53 04:57:30.07 +33:28:54.9
170.40626 -5.88098 galactic Aur Second-epoch detections are separated by 1.4" and 7.2 pix
The object was found in VSX 7" ZTF J045730.47+332850.6
Type: SR
# Max. Min./Amp. JD0 Period
15.232 g Y 0.855 g 2458378.96010 111.641292900000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:30.07 +33:28:54.9: 12.65 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:30.07 +33:28:54.9: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J045730.47+332850.6,2461300.8978,11.53,0.05,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
ZTF J045730.47+332850.6 20260917.3978 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 09 17.3978 2461300.8978 11.64 04:57:42.03 +35:01:06.6
169.21883 -4.89850 galactic Aur Second-epoch detections are separated by 0.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185856983090574464 | 04:57:42.07 +35:01:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.331+/-0.026 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:42.03 +35:01:06.6: 12.66 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:42.03 +35:01:06.6: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185856983090574464,2461300.8978,11.64,0.05,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 185856983090574464 20260917.3978 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 09 17.3978 2461300.8978 13.17 04:59:18.31 +36:31:03.5
168.23831 -3.71638 galactic Aur Second-epoch detections are separated by 0.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:18.31 +36:31:03.5 (user input) | T | P | (position from user input) J-Ks=0.574+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:18.31 +36:31:03.5: 14.43 +/- 0.09 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:18.31 +36:31:03.5: 14.43 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 11.69 04:55:20.74 +34:56:06.4
168.98352 -5.32828 galactic Aur Second-epoch detections are separated by 0.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 161848008530713856 | 04:55:20.79 +34:56:06.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.798+/-0.024 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:20.74 +34:56:06.4: 12.64 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:20.74 +34:56:06.4: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 161848008530713856,2461300.8978,11.69,0.05,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
Gaia DR3 161848008530713856 20260917.3978 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 09 17.3978 2461300.8978 13.09 04:57:53.23 +34:09:17.3
169.92427 -5.40229 galactic Aur Second-epoch detections are separated by 1.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:53.23 +34:09:17.3 (user input) | T | P | (position from user input) J-Ks=1.034+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:53.23 +34:09:17.3: 14.33 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:53.23 +34:09:17.3: 14.41 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.09CV 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 09 17.3978 2461300.8978 11.65 04:57:35.39 +35:47:09.8
168.60018 -4.44083 galactic Aur Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186106499214339200 | 04:57:35.40 +35:47:09.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.547+/-0.024 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:35.39 +35:47:09.8: 12.61 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:35.39 +35:47:09.8: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186106499214339200,2461300.8978,11.65,0.05,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
Gaia DR3 186106499214339200 20260917.3978 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 09 17.3978 2461300.8978 13.21 04:57:17.61 +34:43:50.7
169.39377 -5.14221 galactic Aur Second-epoch detections are separated by 2.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:17.61 +34:43:50.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.561+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:17.61 +34:43:50.7: 14.37 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:17.61 +34:43:50.7: 14.55 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.21CV 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 09 17.3978 2461300.8978 11.48 04:57:29.75 +35:45:08.3
168.61489 -4.47671 galactic Aur Second-epoch detections are separated by 1.4" and 7.4 pix
The object was found in VSX 1" ASASSN-V J045729.80+354507.7
Type: SR
# Max. Min./Amp. JD0 Period
13.040 V 13.130 V 2458034.00000 340.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:29.75 +35:45:08.3: 12.56 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:29.75 +35:45:08.3: 12.48 +/- 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
ASASSN-V J045729.80+354507.7,2461300.8978,11.48,0.05,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
ASASSN-V J045729.80+354507.7 20260917.3978 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 09 17.3978 2461300.8978 11.40 04:58:24.81 +35:40:53.4
168.78630 -4.37424 galactic Aur Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186007856701995904 | 04:58:25.11 +35:40:53.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:24.81 +35:40:53.4: 12.57 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:24.81 +35:40:53.4: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186007856701995904,2461300.8978,11.40,0.05,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 186007856701995904 20260917.3978 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 09 17.3978 2461300.8978 11.40 04:57:32.91 +34:40:35.3
169.46915 -5.13466 galactic Aur Second-epoch detections are separated by 1.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185798537175668608 | 04:57:32.89 +34:40:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5) J-Ks=0.772+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:32.91 +34:40:35.3: 12.56 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:32.91 +34:40:35.3: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185798537175668608,2461300.8978,11.40,0.05,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 185798537175668608 20260917.3978 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 09 17.3978 2461300.8978 13.26 04:58:09.65 +35:59:09.5
168.51458 -4.22622 galactic Aur Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5377+35.9820 | 04:58:09.65 +35:59:09.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.757+/-0.031 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:09.65 +35:59:09.5: 14.43 +/- 0.09 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:09.65 +35:59:09.5: 14.50 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J074.5377+35.9820,2461300.8978,13.26,0.05,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 J074.5377+35.9820 20260917.3978 13.26CV 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 09 17.3978 2461300.8978 11.56 04:59:55.05 +36:43:36.0
168.14918 -3.49083 galactic Aur Second-epoch detections are separated by 0.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186639938449879296 | 04:59:55.06 +36:43:35.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.933+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:55.05 +36:43:36.0: 12.52 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:55.05 +36:43:36.0: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186639938449879296,2461300.8978,11.56,0.05,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
Gaia DR3 186639938449879296 20260917.3978 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 09 17.3978 2461300.8978 11.49 04:56:41.50 +35:03:22.8
169.06053 -5.03707 galactic Aur Second-epoch detections are separated by 1.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185871890920823296 | 04:56:41.61 +35:03:21.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.027+/-9.995 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:41.50 +35:03:22.8: 12.47 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:41.50 +35:03:22.8: 12.48 +/- 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 185871890920823296,2461300.8978,11.49,0.05,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 185871890920823296 20260917.3978 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 09 17.3978 2461300.8978 13.05 04:58:48.76 +35:53:36.5
168.66925 -4.17966 galactic Aur Second-epoch detections are separated by 4.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:48.76 +35:53:36.5 (user input) | T | P | (position from user input) J-Ks=0.366+/-0.031 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:48.76 +35:53:36.5: 14.33 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:48.76 +35:53:36.5: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.25 +/- 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,2461300.8978,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.05CV 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 09 17.3978 2461300.8978 11.29 04:58:41.94 +35:56:13.9
168.62052 -4.17077 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX24" ZTF J045840.90+355634.3
Type: EA
# Max. Min./Amp. JD0 Period
15.907 r Y 0.474 r 2458377.98500 1.474726600000
ATTENTION: measured mag 11.29 is 4.1 mag brighter than the VSX record maximum brightness 15.43 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:41.94 +35:56:13.9: 12.45 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:41.94 +35:56:13.9: 12.42 +/- 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
ZTF J045840.90+355634.3,2461300.8978,11.29,0.05,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
ZTF J045840.90+355634.3 20260917.3978 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 09 17.3978 2461300.8978 11.35 04:58:05.29 +34:50:50.8
169.40307 -4.94183 galactic Aur Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5181+34.8483 | 04:58:05.34 +34:50:49.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.859+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:05.29 +34:50:50.8: 12.45 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:05.29 +34:50:50.8: 12.42 +/- 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 J074.5181+34.8483,2461300.8978,11.35,0.05,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
ATO J074.5181+34.8483 20260917.3978 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 09 17.3978 2461300.8978 11.53 04:57:53.92 +35:54:26.8
168.54349 -4.31650 galactic Aur Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 186201920503792640 | 04:57:53.91 +35:54:27.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.465+/-0.024 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:53.92 +35:54:26.8: 12.44 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:53.92 +35:54:26.8: 12.41 +/- 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
Large-amplitude variable Gaia DR2 186201920503792640,2461300.8978,11.53,0.05,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
Large-amplitude variable Gaia DR2 186201920503792640 20260917.3978 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 09 17.3978 2461300.8978 12.89 04:57:59.16 +34:57:13.6
169.30618 -4.89258 galactic Aur Second-epoch detections are separated by 1.7" and 7.1 pix
The object was found in VSX 1" Gaia DR3 185855608701043968
Type: ROT
# Max. Min./Amp. JD0 Period
13.840 G 13.870 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:59.16 +34:57:13.6: 14.32 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:59.16 +34:57:13.6: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 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
Gaia DR3 185855608701043968,2461300.8978,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 185855608701043968 20260917.3978 12.89CV 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 09 17.3978 2461300.8978 11.41 04:58:25.35 +35:05:03.1
169.25867 -4.74174 galactic Aur Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185881546007325824 | 04:58:25.37 +35:05:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.445+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:25.35 +35:05:03.1: 12.40 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:25.35 +35:05:03.1: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185881546007325824,2461300.8978,11.41,0.05,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
Gaia DR3 185881546007325824 20260917.3978 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 09 17.3978 2461300.8978 13.27 04:53:58.43 +35:39:18.3
168.24366 -5.09625 galactic Aur Second-epoch detections are separated by 3.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:53:58.43 +35:39:18.3 (user input) | T | P | (position from user input) J-Ks=0.361+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:53:58.43 +35:39:18.3: 14.31 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:53:58.43 +35:39:18.3: 14.37 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.34 +/- 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,2461300.8978,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.27CV 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 09 17.3978 2461300.8978 11.29 04:57:01.86 +34:15:03.6
169.73835 -5.48188 galactic Aur Second-epoch detections are separated by 0.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 161757470618875648 | 04:57:01.81 +34:15:04.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.319+/-0.024 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:01.86 +34:15:03.6: 12.38 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:01.86 +34:15:03.6: 12.34 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 161757470618875648,2461300.8978,11.29,0.05,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 161757470618875648 20260917.3978 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 09 17.3978 2461300.8978 12.89 04:59:21.45 +36:03:35.9
168.60601 -3.99020 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:21.45 +36:03:35.9 (user input) | T | P | (position from user input) J-Ks=0.272+/-0.035 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:21.45 +36:03:35.9: 14.30 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:21.45 +36:03:35.9: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.18 +/- 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,2461300.8978,12.89,0.05,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 20260917.3978 12.89CV 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 09 17.3978 2461300.8978 11.47 04:56:25.70 +35:11:37.0
168.91897 -4.99396 galactic Aur Second-epoch detections are separated by 0.3" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.1078+35.1890 | 04:56:25.80 +35:11:36.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.239+/-0.029 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:25.70 +35:11:37.0: 12.37 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:25.70 +35:11:37.0: 12.42 +/- 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
ATO J074.1078+35.1890,2461300.8978,11.47,0.05,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
ATO J074.1078+35.1890 20260917.3978 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 09 17.3978 2461300.8978 11.43 04:55:46.37 +35:28:08.5
168.61908 -4.92712 galactic Aur Second-epoch detections are separated by 0.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186083787426241024 | 04:55:46.39 +35:28:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.304+/-0.025 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:46.37 +35:28:08.5: 12.36 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:46.37 +35:28:08.5: 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 186083787426241024,2461300.8978,11.43,0.05,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 186083787426241024 20260917.3978 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 09 17.3978 2461300.8978 11.41 04:58:04.65 +36:03:52.7
168.44216 -4.19077 galactic Aur Second-epoch detections are separated by 0.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186216278578233216 | 04:58:04.68 +36:03:52.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.858+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:04.65 +36:03:52.7: 12.34 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:04.65 +36:03:52.7: 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
Gaia DR3 186216278578233216,2461300.8978,11.41,0.05,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
Gaia DR3 186216278578233216 20260917.3978 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 09 17.3978 2461300.8978 13.05 04:57:54.53 +34:55:31.7
169.31869 -4.92251 galactic Aur Second-epoch detections are separated by 2.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:54.53 +34:55:31.7 (user input) | T | P | (position from user input) J-Ks=0.692+/-0.027 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:54.53 +34:55:31.7: 14.34 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:54.53 +34:55:31.7: 14.36 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.05CV 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 09 17.3978 2461300.8978 11.39 04:56:00.46 +35:37:56.2
168.52082 -4.78803 galactic Aur Second-epoch detections are separated by 0.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186109488511575936 | 04:56:00.46 +35:37:56.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.823+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:00.46 +35:37:56.2: 12.33 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:00.46 +35:37:56.2: 12.32 +/- 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 186109488511575936,2461300.8978,11.39,0.05,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 186109488511575936 20260917.3978 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 09 17.3978 2461300.8978 12.91 04:58:12.45 +35:01:09.6
169.28259 -4.81640 galactic Aur Second-epoch detections are separated by 3.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:12.45 +35:01:09.6 (user input) | T | P | (position from user input) J-Ks=1.152+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:12.45 +35:01:09.6: 14.27 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:12.45 +35:01:09.6: 14.25 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.26 +/- 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,2461300.8978,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.91CV 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 09 17.3978 2461300.8978 11.35 04:56:01.70 +35:32:16.7
168.59748 -4.84349 galactic Aur Second-epoch detections are separated by 0.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.0072+35.5379 | 04:56:01.74 +35:32:16.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.883+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:01.70 +35:32:16.7: 12.27 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:01.70 +35:32:16.7: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J074.0072+35.5379,2461300.8978,11.35,0.05,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
ATO J074.0072+35.5379 20260917.3978 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 09 17.3978 2461300.8978 13.16 04:55:50.80 +35:27:50.9
168.63232 -4.91841 galactic Aur Second-epoch detections are separated by 1.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:50.80 +35:27:50.9 (user input) | T | P | (position from user input) J-Ks=0.550+/-0.025 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:50.80 +35:27:50.9: 14.30 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:50.80 +35:27:50.9: 14.23 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.26 +/- 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,2461300.8978,13.16,0.05,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 20260917.3978 13.16CV 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 09 17.3978 2461300.8978 13.20 04:54:32.77 +35:55:15.5
168.10876 -4.83914 galactic Aur Second-epoch detections are separated by 1.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.6396+35.9206 | 04:54:32.77 +35:55:15.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.091+/-0.025 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:32.77 +35:55:15.5: 14.29 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:32.77 +35:55:15.5: 14.43 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.35 +/- 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
ATO J073.6396+35.9206,2461300.8978,13.20,0.05,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
ATO J073.6396+35.9206 20260917.3978 13.20CV 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 09 17.3978 2461300.8978 11.29 04:55:08.13 +35:18:10.8
168.66796 -5.13223 galactic Aur Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 186075407948027264 | 04:55:08.13 +35:18:11.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.504+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:08.13 +35:18:10.8: 12.26 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:08.13 +35:18:10.8: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 186075407948027264,2461300.8978,11.29,0.05,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
Large-amplitude variable Gaia DR2 186075407948027264 20260917.3978 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 09 17.3978 2461300.8978 13.01 04:59:35.13 +36:30:25.6
168.28141 -3.67851 galactic Aur Second-epoch detections are separated by 1.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.8952+36.5173 | 04:59:35.13 +36:30:25.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.346+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:35.13 +36:30:25.6: 14.26 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:35.13 +36:30:25.6: 14.12 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.18 +/- 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
ATO J074.8952+36.5173,2461300.8978,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.8952+36.5173 20260917.3978 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 13.01 04:59:15.21 +36:29:56.6
168.24656 -3.73601 galactic Aur Second-epoch detections are separated by 2.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:15.21 +36:29:56.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:15.21 +36:29:56.6: 14.29 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:15.21 +36:29:56.6: 14.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.20 +/- 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,2461300.8978,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 13.10 04:56:50.38 +34:54:16.3
169.19890 -5.10755 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:50.38 +34:54:16.3 (user input) | T | P | (position from user input) J-Ks=0.568+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:50.38 +34:54:16.3: 14.25 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:50.38 +34:54:16.3: 14.30 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.27 +/- 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,2461300.8978,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.10CV 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 09 17.3978 2461300.8978 12.98 04:58:53.10 +35:38:34.8
168.87597 -4.32267 galactic Aur Second-epoch detections are separated by 1.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:53.10 +35:38:34.8 (user input) | T | P | (position from user input) J-Ks=0.503+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:53.10 +35:38:34.8: 14.30 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:53.10 +35:38:34.8: 14.30 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,12.98,0.05,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 20260917.3978 12.98CV 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 09 17.3978 2461300.8978 12.98 04:58:36.28 +35:02:35.6
169.31410 -4.73769 galactic Aur Second-epoch detections are separated by 3.7" and 6.7 pix
The object was found in VSX 1" Gaia DR3 185834271303477120
Type: ROT
# Max. Min./Amp. JD0 Period
13.990 G 14.030 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:36.28 +35:02:35.6: 14.29 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:36.28 +35:02:35.6: 14.40 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185834271303477120,2461300.8978,12.98,0.05,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 185834271303477120 20260917.3978 12.98CV 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 09 17.3978 2461300.8978 11.33 04:54:45.24 +35:10:04.2
168.72503 -5.27751 galactic Aur Second-epoch detections are separated by 0.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 186060976857992960 | 04:54:45.26 +35:10:04.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: OB 1965LS....C05....0H LS V +35 4 J-Ks=0.257+/-0.028 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:45.24 +35:10:04.2: 12.21 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:45.24 +35:10:04.2: 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 186060976857992960,2461300.8978,11.33,0.05,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 186060976857992960 20260917.3978 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 09 17.3978 2461300.8978 13.02 04:58:26.12 +36:10:02.4
168.40609 -4.07047 galactic Aur Second-epoch detections are separated by 1.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.6092+36.1670 | 04:58:26.12 +36:10:02.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.810+/-0.037 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:26.12 +36:10:02.4: 14.27 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:26.12 +36:10:02.4: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.21 +/- 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
ATO J074.6092+36.1670,2461300.8978,13.02,0.05,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
ATO J074.6092+36.1670 20260917.3978 13.02CV 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 09 17.3978 2461300.8978 12.79 04:57:34.34 +34:26:45.5
169.65403 -5.27343 galactic Aur Second-epoch detections are separated by 0.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.3935+34.4461 | 04:57:34.34 +34:26:45.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.411+/-0.024 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:34.34 +34:26:45.5: 14.25 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:34.34 +34:26:45.5: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.21 +/- 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
ATO J074.3935+34.4461,2461300.8978,12.79,0.05,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
ATO J074.3935+34.4461 20260917.3978 12.79CV 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 09 17.3978 2461300.8978 13.09 04:57:07.20 +34:32:54.8
169.51518 -5.28310 galactic Aur Second-epoch detections are separated by 1.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:07.20 +34:32:54.8 (user input) | T | P | (position from user input) J-Ks=0.557+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:07.20 +34:32:54.8: 14.24 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:07.20 +34:32:54.8: 14.33 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.28 +/- 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,2461300.8978,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.09CV 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 09 17.3978 2461300.8978 13.12 04:54:57.53 +35:15:05.5
168.68569 -5.19254 galactic Aur Second-epoch detections are separated by 2.2" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J073.7435+35.2522 | 04:54:57.53 +35:15:05.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.044+/-0.029 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:57.53 +35:15:05.5: 14.31 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:57.53 +35:15:05.5: 14.43 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.36 +/- 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
ATO J073.7435+35.2522,2461300.8978,13.12,0.05,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
ATO J073.7435+35.2522 20260917.3978 13.12CV 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 09 17.3978 2461300.8978 13.04 04:57:59.96 +35:58:33.2
168.50225 -4.25812 galactic Aur Second-epoch detections are separated by 2.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:59.96 +35:58:33.2 (user input) | T | P | (position from user input) J-Ks=0.965+/-0.025 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:59.96 +35:58:33.2: 14.23 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:59.96 +35:58:33.2: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 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,2461300.8978,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.04CV 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 09 17.3978 2461300.8978 13.06 04:56:22.74 +34:41:46.3
169.30391 -5.31104 galactic Aur Second-epoch detections are separated by 0.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.0915+34.6972 | 04:56:22.74 +34:41:46.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.899+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:22.74 +34:41:46.3: 14.28 +/- 0.08 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:22.74 +34:41:46.3: 14.23 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.26 +/- 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
ATO J074.0915+34.6972,2461300.8978,13.06,0.05,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 J074.0915+34.6972 20260917.3978 13.06CV 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 09 17.3978 2461300.8978 10.95 04:56:55.83 +34:45:46.0
169.32213 -5.18087 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185847289349477376 | 04:56:57.61 +34:45:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1949AnHar.112....1C HD 280265 J-Ks=0.392+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:55.83 +34:45:46.0: 11.91 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:55.83 +34:45:46.0: 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
Gaia DR3 185847289349477376,2461300.8978,10.95,0.05,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 185847289349477376 20260917.3978 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 09 17.3978 2461300.8978 13.12 04:58:26.66 +36:04:18.8
168.48243 -4.12804 galactic Aur Second-epoch detections are separated by 1.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:26.66 +36:04:18.8 (user input) | T | P | (position from user input) J-Ks=0.383+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:26.66 +36:04:18.8: 14.23 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:26.66 +36:04:18.8: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 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,2461300.8978,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.12CV 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 09 17.3978 2461300.8978 12.96 04:57:58.94 +33:53:26.0
170.14533 -5.54993 galactic Aur Second-epoch detections are separated by 4.6" and 6.9 pix
The object was found in VSX 2" Gaia DR3 160989294245410816
Type: ROT
# Max. Min./Amp. JD0 Period
13.810 G 13.830 G 24.862000000000 K
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:58.94 +33:53:26.0: 14.20 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:58.94 +33:53:26.0: 14.15 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.18 +/- 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
Gaia DR3 160989294245410816,2461300.8978,12.96,0.05,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 160989294245410816 20260917.3978 12.96CV 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 09 17.3978 2461300.8978 13.11 04:55:48.47 +35:35:06.6
168.53240 -4.84915 galactic Aur Second-epoch detections are separated by 0.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:48.47 +35:35:06.6 (user input) | T | P | (position from user input) J-Ks=0.396+/-0.026 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:48.47 +35:35:06.6: 14.24 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:48.47 +35:35:06.6: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 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,2461300.8978,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.11CV 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 09 17.3978 2461300.8978 12.96 04:56:16.48 +34:47:05.1
169.22086 -5.27280 galactic Aur Second-epoch detections are separated by 2.1" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:16.48 +34:47:05.1 (user input) | T | P | (position from user input) J-Ks=0.628+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:16.48 +34:47:05.1: 14.23 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:16.48 +34:47:05.1: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.18 +/- 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,2461300.8978,12.96,0.05,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
target 20260917.3978 12.96CV 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 09 17.3978 2461300.8978 12.87 04:58:44.79 +35:47:22.9
168.74282 -4.25427 galactic Aur Second-epoch detections are separated by 1.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.6967+35.7878 | 04:58:44.79 +35:47:22.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.462+/-0.029 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:44.79 +35:47:22.9: 14.20 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:44.79 +35:47:22.9: 14.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 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
ATO J074.6967+35.7878,2461300.8978,12.87,0.05,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
ATO J074.6967+35.7878 20260917.3978 12.87CV 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 09 17.3978 2461300.8978 12.93 04:57:17.88 +34:56:19.3
169.23048 -5.01265 galactic Aur Second-epoch detections are separated by 1.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:17.88 +34:56:19.3 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:17.88 +34:56:19.3: 14.26 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:17.88 +34:56:19.3: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.21 +/- 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,2461300.8978,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 13.00 04:55:54.19 +34:39:16.3
169.27558 -5.41357 galactic Aur Second-epoch detections are separated by 2.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:54.19 +34:39:16.3 (user input) | T | P | (position from user input) J-Ks=0.565+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:54.19 +34:39:16.3: 14.21 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:54.19 +34:39:16.3: 14.26 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.23 +/- 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,2461300.8978,13.00,0.05,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 20260917.3978 13.00CV 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 09 17.3978 2461300.8978 12.84 04:58:01.38 +34:19:30.6
169.80711 -5.27500 galactic Aur Second-epoch detections are separated by 1.4" and 7.5 pix
The object was found in VSX19" Gaia DR3 185774824659030016
Type: S
# Max. Min./Amp. JD0 Period
17.120 G 17.570 G F
ATTENTION: measured mag 12.84 is 4.3 mag brighter than the VSX record maximum brightness 17.12 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:01.38 +34:19:30.6: 14.22 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:01.38 +34:19:30.6: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.12 +/- 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
Gaia DR3 185774824659030016,2461300.8978,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 185774824659030016 20260917.3978 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 10.67 04:57:17.39 +35:46:24.8
168.57217 -4.49632 galactic Aur Second-epoch detections are separated by 1.1" and 7.2 pix
The object was found in VSX 2" ASASSN-V J045717.50+354623.7
Type: SR
# Max. Min./Amp. JD0 Period
13.280 g Y 0.190 g 2459207.87800 127.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:17.39 +35:46:24.8: 11.69 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:17.39 +35:46:24.8: 11.53 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 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
ASASSN-V J045717.50+354623.7,2461300.8978,10.67,0.05,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
ASASSN-V J045717.50+354623.7 20260917.3978 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 09 17.3978 2461300.8978 13.15 04:54:51.01 +35:49:18.9
168.22497 -4.85313 galactic Aur Second-epoch detections are separated by 2.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:54:51.01 +35:49:18.9 (user input) | T | P | (position from user input) J-Ks=0.392+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:51.01 +35:49:18.9: 14.20 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:51.01 +35:49:18.9: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.19 +/- 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,2461300.8978,13.15,0.05,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 20260917.3978 13.15CV 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 09 17.3978 2461300.8978 12.95 04:59:10.94 +35:39:11.1
168.90536 -4.26890 galactic Aur Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:10.94 +35:39:11.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:10.94 +35:39:11.1: 14.21 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:10.94 +35:39:11.1: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 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,2461300.8978,12.95,0.05,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 20260917.3978 12.95CV 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 09 17.3978 2461300.8978 12.74 04:59:10.79 +35:33:35.7
168.97863 -4.32671 galactic Aur Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:10.79 +35:33:35.7 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:10.79 +35:33:35.7: 14.17 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:10.79 +35:33:35.7: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 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,2461300.8978,12.74,0.05,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 20260917.3978 12.74CV 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 09 17.3978 2461300.8978 12.97 04:57:46.97 +34:06:30.6
169.94745 -5.44787 galactic Aur Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:46.97 +34:06:30.6 (user input) | T | P | (position from user input) J-Ks=0.412+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:46.97 +34:06:30.6: 14.16 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:46.97 +34:06:30.6: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.14 +/- 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,2461300.8978,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.97CV 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 09 17.3978 2461300.8978 12.95 04:59:49.17 +36:17:23.7
168.48197 -3.77514 galactic Aur Second-epoch detections are separated by 3.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.9593+36.2903 | 04:59:49.17 +36:17:23.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.165+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:49.17 +36:17:23.7: 14.15 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:49.17 +36:17:23.7: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.08 +/- 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
ATO J074.9593+36.2903,2461300.8978,12.95,0.05,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 J074.9593+36.2903 20260917.3978 12.95CV 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 09 17.3978 2461300.8978 13.29 04:58:07.87 +34:46:44.9
169.46246 -4.97709 galactic Aur Second-epoch detections are separated by 1.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:07.87 +34:46:44.9 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.359+/-0.033 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:07.87 +34:46:44.9: 14.99 +/- 0.14 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:07.87 +34:46:44.9: 14.75 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461300.8978,13.29,0.05,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 20260917.3978 13.29CV 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 09 17.3978 2461300.8978 12.88 04:58:51.62 +35:36:38.1
168.89846 -4.34662 galactic Aur Second-epoch detections are separated by 2.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:51.62 +35:36:38.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:51.62 +35:36:38.1: 14.07 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:51.62 +35:36:38.1: 14.17 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.11 +/- 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,2461300.8978,12.88,0.05,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 20260917.3978 12.88CV 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 09 17.3978 2461300.8978 12.81 04:56:03.80 +34:41:12.0
169.27089 -5.36779 galactic Aur Second-epoch detections are separated by 2.7" and 6.9 pix
The object was found in VSX 2" Gaia DR3 161829218049616512
Type: VAR
# Max. Min./Amp. JD0 Period
13.260 G 13.300 G 0.084681600000 M
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:03.80 +34:41:12.0: 14.16 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:03.80 +34:41:12.0: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 161829218049616512,2461300.8978,12.81,0.05,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 161829218049616512 20260917.3978 12.81CV 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 09 17.3978 2461300.8978 12.91 04:58:02.68 +34:18:39.4
169.82112 -5.28026 galactic Aur Second-epoch detections are separated by 2.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5026+34.3204 | 04:58:02.68 +34:18:39.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.530+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:02.68 +34:18:39.4: 14.12 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:02.68 +34:18:39.4: 14.14 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.13 +/- 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
ATO J074.5026+34.3204,2461300.8978,12.91,0.05,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 J074.5026+34.3204 20260917.3978 12.91CV 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 09 17.3978 2461300.8978 13.04 04:56:28.11 +34:29:52.7
169.47143 -5.41974 galactic Aur Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:28.11 +34:29:52.7 (user input) | T | P | (position from user input) J-Ks=0.840+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:28.11 +34:29:52.7: 14.13 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:28.11 +34:29:52.7: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.17 +/- 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,2461300.8978,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.04CV 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 09 17.3978 2461300.8978 12.89 04:59:10.11 +35:30:11.3
169.02205 -4.36352 galactic Aur Second-epoch detections are separated by 3.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:10.11 +35:30:11.3 (user input) | T | P | (position from user input) J-Ks=1.021+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:10.11 +35:30:11.3: 14.11 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:10.11 +35:30:11.3: 14.13 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 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,2461300.8978,12.89,0.05,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 20260917.3978 12.89CV 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 09 17.3978 2461300.8978 12.73 04:59:24.25 +35:47:28.1
168.82414 -4.14838 galactic Aur Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:59:24.25 +35:47:28.1 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.029 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:24.25 +35:47:28.1: 14.11 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:24.25 +35:47:28.1: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461300.8978,12.73,0.05,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 20260917.3978 12.73CV 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 09 17.3978 2461300.8978 12.96 04:55:33.55 +35:04:37.6
168.89942 -5.20555 galactic Aur Second-epoch detections are separated by 0.9" and 7.3 pix
The object was found in VSX10" Gaia DR3 186057433506960512
Type: E
# Max. Min./Amp. JD0 Period
18.940 G 19.830 G 1.519080000000
ATTENTION: measured mag 12.96 is 6.0 mag brighter than the VSX record maximum brightness 18.94 - possible unusual activity of a known variable! (Alternatively, this may be a new object that coincides with the known variable's position just by chance.)
The object was not found in astcheck.
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:33.55 +35:04:37.6: 14.08 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:33.55 +35:04:37.6: 14.12 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 186057433506960512,2461300.8978,12.96,0.05,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 186057433506960512 20260917.3978 12.96CV 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 09 17.3978 2461300.8978 12.88 04:56:29.26 +34:43:41.0
169.29277 -5.27375 galactic Aur Second-epoch detections are separated by 2.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:29.26 +34:43:41.0 (user input) | T | P | (position from user input) J-Ks=0.547+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:29.26 +34:43:41.0: 14.11 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:29.26 +34:43:41.0: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.13 +/- 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,2461300.8978,12.88,0.05,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 20260917.3978 12.88CV 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 09 17.3978 2461300.8978 12.95 04:56:57.19 +34:40:37.0
169.39264 -5.23045 galactic Aur Second-epoch detections are separated by 2.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:57.19 +34:40:37.0 (user input) | T | P | (position from user input) J-Ks=0.942+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:57.19 +34:40:37.0: 14.10 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:57.19 +34:40:37.0: 14.09 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461300.8978,12.95,0.05,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 20260917.3978 12.95CV 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 09 17.3978 2461300.8978 12.80 04:58:56.28 +35:38:34.5
168.88270 -4.31425 galactic Aur Second-epoch detections are separated by 3.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:56.28 +35:38:34.5 (user input) | T | P | (position from user input) J-Ks=0.339+/-0.028 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:56.28 +35:38:34.5: 14.11 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:56.28 +35:38:34.5: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.10 +/- 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,2461300.8978,12.80,0.05,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 20260917.3978 12.80CV 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 09 17.3978 2461300.8978 9.89 04:56:57.64 +34:45:37.5
169.32785 -5.17748 galactic Aur Second-epoch detections are separated by 0.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 185847289349477376 | 04:56:57.61 +34:45:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1949AnHar.112....1C HD 280265 J-Ks=0.455+/-0.027 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:57.64 +34:45:37.5: 10.83 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:57.64 +34:45:37.5: 10.83 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 185847289349477376,2461300.8978,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 185847289349477376 20260917.3978 9.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.93 04:55:25.15 +35:20:41.9
168.67130 -5.06082 galactic Aur Second-epoch detections are separated by 1.3" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:25.15 +35:20:41.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:25.15 +35:20:41.9: 14.09 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:25.15 +35:20:41.9: 14.24 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 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,2461300.8978,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.79 04:58:20.26 +34:19:17.1
169.85034 -5.22620 galactic Aur Second-epoch detections are separated by 0.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:20.26 +34:19:17.1 (user input) | T | P | (position from user input) J-Ks=1.047+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:20.26 +34:19:17.1: 14.09 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:20.26 +34:19:17.1: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 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,2461300.8978,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.79CV 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 09 17.3978 2461300.8978 12.84 04:59:08.12 +35:48:34.2
168.77596 -4.18000 galactic Aur Second-epoch detections are separated by 1.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.7912+35.8091 | 04:59:08.12 +35:48:34.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.548+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:08.12 +35:48:34.2: 14.11 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:08.12 +35:48:34.2: 14.16 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.13 +/- 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
ATO J074.7912+35.8091,2461300.8978,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.7912+35.8091 20260917.3978 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.91 04:59:20.30 +36:04:48.7
168.58765 -3.98079 galactic Aur Second-epoch detections are separated by 2.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.8350+36.0794 | 04:59:20.30 +36:04:48.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:20.30 +36:04:48.7: 14.06 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:20.30 +36:04:48.7: 14.02 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.04 +/- 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
ATO J074.8350+36.0794,2461300.8978,12.91,0.05,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 J074.8350+36.0794 20260917.3978 12.91CV 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 09 17.3978 2461300.8978 13.00 04:58:14.24 +35:02:38.9
169.26680 -4.79627 galactic Aur Second-epoch detections are separated by 2.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:14.24 +35:02:38.9 (user input) | T | P | (position from user input) J-Ks=0.607+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:14.24 +35:02:38.9: 14.09 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:14.24 +35:02:38.9: 14.22 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.15 +/- 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,2461300.8978,13.00,0.05,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 20260917.3978 13.00CV 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 09 17.3978 2461300.8978 13.09 04:56:28.41 +35:07:17.7
168.98137 -5.03150 galactic Aur Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:28.41 +35:07:17.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.988+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:28.41 +35:07:17.7: 14.09 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:28.41 +35:07:17.7: 13.97 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461300.8978,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.09CV 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 09 17.3978 2461300.8978 12.69 04:56:35.72 +34:25:06.8
169.55027 -5.44854 galactic Aur Second-epoch detections are separated by 1.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:35.72 +34:25:06.8 (user input) | T | P | (position from user input) J-Ks=0.443+/-0.030 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:35.72 +34:25:06.8: 14.08 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:35.72 +34:25:06.8: 13.98 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.03 +/- 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,2461300.8978,12.69,0.05,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 20260917.3978 12.69CV 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 09 17.3978 2461300.8978 12.88 04:57:49.42 +34:50:18.2
169.37654 -4.99009 galactic Aur Second-epoch detections are separated by 2.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:49.42 +34:50:18.2 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.601+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:49.42 +34:50:18.2: 14.10 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:49.42 +34:50:18.2: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461300.8978,12.88,0.05,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 20260917.3978 12.88CV 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 09 17.3978 2461300.8978 13.05 04:56:43.88 +35:47:20.5
168.48944 -4.57549 galactic Aur Second-epoch detections are separated by 1.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:43.88 +35:47:20.5 (user input) | T | P | (position from user input) J-Ks=0.791+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:43.88 +35:47:20.5: 14.10 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:43.88 +35:47:20.5: 14.08 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461300.8978,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.05CV 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 09 17.3978 2461300.8978 12.87 04:57:01.70 +34:52:25.2
169.24730 -5.09635 galactic Aur Second-epoch detections are separated by 2.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:01.70 +34:52:25.2 (user input) | T | P | (position from user input) J-Ks=0.627+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:01.70 +34:52:25.2: 14.08 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:01.70 +34:52:25.2: 14.14 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.11 +/- 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,2461300.8978,12.87,0.05,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 20260917.3978 12.87CV 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 09 17.3978 2461300.8978 12.93 04:55:13.47 +34:22:15.8
169.41090 -5.69951 galactic Aur Second-epoch detections are separated by 1.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:13.47 +34:22:15.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.958+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:13.47 +34:22:15.8: 14.07 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:13.47 +34:22:15.8: 13.96 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 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,2461300.8978,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.84 04:58:17.63 +35:48:36.9
168.66975 -4.31374 galactic Aur Second-epoch detections are separated by 3.0" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.5712+35.8087 | 04:58:17.63 +35:48:36.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.908+/-0.028 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:17.63 +35:48:36.9: 14.09 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:17.63 +35:48:36.9: 14.20 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.14 +/- 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
ATO J074.5712+35.8087,2461300.8978,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J074.5712+35.8087 20260917.3978 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.82 04:57:40.64 +34:11:36.4
169.86682 -5.41254 galactic Aur Second-epoch detections are separated by 1.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:40.64 +34:11:36.4 (user input) | T | P | (position from user input) J-Ks=0.666+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:40.64 +34:11:36.4: 14.07 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:40.64 +34:11:36.4: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461300.8978,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 17.3978 2461300.8978 12.94 04:58:43.17 +36:14:43.8
168.38000 -3.97709 galactic Aur Second-epoch detections are separated by 2.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:43.17 +36:14:43.8 (user input) | T | P | (position from user input) J-Ks=0.483+/-0.040 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:43.17 +36:14:43.8: 14.05 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:43.17 +36:14:43.8: 14.00 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461300.8978,12.94,0.05,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
target 20260917.3978 12.94CV 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 09 17.3978 2461300.8978 12.70 04:57:34.95 +34:26:05.7
169.66405 -5.27862 galactic Aur Second-epoch detections are separated by 0.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.3935+34.4461 | 04:57:34.95 +34:26:05.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.061+/-0.024 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:34.95 +34:26:05.7: 14.05 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:34.95 +34:26:05.7: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.04 +/- 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
ATO J074.3935+34.4461,2461300.8978,12.70,0.05,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
ATO J074.3935+34.4461 20260917.3978 12.70CV 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 09 17.3978 2461300.8978 13.10 04:57:25.37 +36:05:47.2
168.33494 -4.27488 galactic Aur Second-epoch detections are separated by 1.7" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:25.37 +36:05:47.2 (user input) | T | P | (position from user input) J-Ks=0.534+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:25.37 +36:05:47.2: 14.08 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:25.37 +36:05:47.2: 14.10 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461300.8978,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.10CV 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 09 17.3978 2461300.8978 12.96 04:58:19.56 +35:58:28.6
168.54426 -4.20699 galactic Aur Second-epoch detections are separated by 0.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:19.56 +35:58:28.6 (user input) | T | P | (position from user input) J-Ks=0.317+/-0.032 (F)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:19.56 +35:58:28.6: 14.08 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:19.56 +35:58:28.6: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 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,2461300.8978,12.96,0.05,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
target 20260917.3978 12.96CV 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 09 17.3978 2461300.8978 13.02 04:58:53.54 +35:27:58.5
169.01642 -4.43052 galactic Aur Second-epoch detections are separated by 1.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:53.54 +35:27:58.5 (user input) | T | P | (position from user input) J-Ks=0.646+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:53.54 +35:27:58.5: 14.07 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:53.54 +35:27:58.5: 14.19 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.12 +/- 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,2461300.8978,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.02CV 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 09 17.3978 2461300.8978 12.76 04:56:43.07 +34:47:46.1
169.26865 -5.19442 galactic Aur Second-epoch detections are separated by 1.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:43.07 +34:47:46.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.488+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:43.07 +34:47:46.1: 14.07 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:43.07 +34:47:46.1: 13.91 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.98 +/- 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,2461300.8978,12.76,0.05,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 20260917.3978 12.76CV 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 09 17.3978 2461300.8978 12.89 04:57:46.45 +34:10:12.4
169.89768 -5.41122 galactic Aur Second-epoch detections are separated by 1.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:46.45 +34:10:12.4 (user input) | T | P | (position from user input) J-Ks=0.567+/-0.028 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:46.45 +34:10:12.4: 14.09 +/- 0.07 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:46.45 +34:10:12.4: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461300.8978,12.89,0.05,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 20260917.3978 12.89CV 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 09 17.3978 2461300.8978 12.72 04:56:21.50 +34:22:02.4
169.56012 -5.51867 galactic Aur Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:21.50 +34:22:02.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.048+/-0.027 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:21.50 +34:22:02.4: 14.04 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:21.50 +34:22:02.4: 14.01 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461300.8978,12.72,0.05,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 20260917.3978 12.72CV 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 09 17.3978 2461300.8978 13.06 04:56:16.82 +35:02:58.3
169.01336 -5.10725 galactic Aur Second-epoch detections are separated by 2.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:16.82 +35:02:58.3 (user input) | T | P | (position from user input) J-Ks=1.263+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:16.82 +35:02:58.3: 14.09 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:16.82 +35:02:58.3: 14.05 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.07 +/- 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,2461300.8978,13.06,0.05,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
target 20260917.3978 13.06CV 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 09 17.3978 2461300.8978 12.77 04:57:54.76 +34:01:54.5
170.02473 -5.47410 galactic Aur Second-epoch detections are separated by 1.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:54.76 +34:01:54.5 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.826+/-0.023 (M)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:54.76 +34:01:54.5: 14.05 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:54.76 +34:01:54.5: 13.99 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461300.8978,12.77,0.05,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 20260917.3978 12.77CV 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 09 17.3978 2461300.8978 13.05 04:58:18.10 +36:10:23.3
168.38479 -4.08807 galactic Aur Second-epoch detections are separated by 3.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:58:18.10 +36:10:23.3 (user input) | T | P | (position from user input) J-Ks=0.334+/-0.035 (G)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:18.10 +36:10:23.3: 14.05 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:18.10 +36:10:23.3: 14.14 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.09 +/- 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,2461300.8978,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.05CV 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 09 17.3978 2461300.8978 13.02 04:55:13.19 +34:28:21.3
169.33053 -5.63696 galactic Aur Second-epoch detections are separated by 0.6" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:13.19 +34:28:21.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.504+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:13.19 +34:28:21.3: 14.06 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:13.19 +34:28:21.3: 13.96 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.01 +/- 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,2461300.8978,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 13.02CV 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 09 17.3978 2461300.8978 12.97 04:55:27.31 +35:42:06.6
168.39603 -4.83237 galactic Aur Second-epoch detections are separated by 1.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:27.31 +35:42:06.6 (user input) | T | P | (position from user input) J-Ks=0.700+/-0.025 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:27.31 +35:42:06.6: 14.01 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:27.31 +35:42:06.6: 14.02 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 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,2461300.8978,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260917.3978 12.97CV 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 09 17.3978 2461300.8978 12.94 04:57:43.42 +34:14:28.1
169.83511 -5.37553 galactic Aur Second-epoch detections are separated by 1.0" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J074.4310+34.2436 | 04:57:43.42 +34:14:28.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.633+/-0.029 (K)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:43.42 +34:14:28.1: 14.04 +/- 0.06 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:43.42 +34:14:28.1: 14.14 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.08 +/- 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
ATO J074.4310+34.2436,2461300.8978,12.94,0.05,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 J074.4310+34.2436 20260917.3978 12.94CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
First image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Last image: 2461300.89812478 17.09.2026 09:33:07.981 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 88
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
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: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 16647
Objects passed selection criteria: 16594
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 12866.2
Average stars matched: 12227.5 (95.0355 %)
Memory usage VmPeak: 242664 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 17 04:35:58 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
First image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Last image: 2461300.89812478 17.09.2026 09:33:07.981 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 792
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 77 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 122531
Objects passed selection criteria: 122292
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 96569.8
Average stars matched: 90708.8 (93.9308 %)
Memory usage VmPeak: 520504 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 17 04:38:48 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
SExtractor catalog cache: saved Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461300.89739203
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits exists and is non-empty
wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits exists and is non-empty
wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits exists and is non-empty
wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (1st reference image)
verification OK: wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:49.059 +37:59:50.85 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits (1st new image)
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:50.406 +37:59:16.58 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:21:49.059 +37:59:50.85
Second-epoch image center 04:21:50.406 +37:59:16.58
Angular distance between the image centers 0.0105 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits (2nd new image)
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
Image size: 941.2'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:47.811 +37:59:48.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:21:49.059 +37:59:50.85
Second-epoch image center 04:21:47.811 +37:59:48.39
Angular distance between the image centers 0.0042 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:21:50.406 +37:59:16.58
Second-epoch second image center 04:21:47.811 +37:59:48.39
Angular distance between the image centers 0.01228 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits &> /tmp/tmp.6pHFvieefN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits &> /tmp/tmp.ftOIRkjk9Q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits &> /tmp/tmp.qc0jf3M7IZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits &> /tmp/tmp.0owOCANBB5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
Found non-empty wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
The reference image (wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits) and catalog (wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat) found
'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat' -> 'wcsmag.cat'
Read 18677 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9661 to 76.3326 deg, Dec +32.1948 to +43.3141 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 54.9661 to 76.3326 deg, Dec 32.1948 to 43.3141 deg
Loaded 9192 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6385 out of 7127 total matches.
Matched with Tycho-2 7127 out of 18677 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.973500
a=0.000000 b=1.000000 c=22.973500
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.51
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.51
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 18677 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9661 to 76.3326 deg, Dec +32.1948 to +43.3141 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 54.9661 to 76.3326 deg, Dec 32.1948 to 43.3141 deg
Loaded 9192 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6385 out of 7127 total matches.
Matched with Tycho-2 7127 out of 18677 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Forced-photometry filter: calibrated wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -> calib.txt_param_ref_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (aperture=6.0)
Read 18569 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.4956 to 75.7898 deg, Dec +32.0248 to +43.3806 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 54.4956 to 75.7898 deg, Dec 32.0248 to 43.3806 deg
Loaded 9219 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6462 out of 7192 total matches.
Matched with Tycho-2 7192 out of 18569 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Forced-photometry filter: calibrated wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits -> calib.txt_param_ref_wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
2.1 pix Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
2.5 pix fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
2.5 pix fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
Limiting magnitude estimates:
15.5 mag. Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
15.5 mag. Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
14.1 mag. fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
14.4 mag. fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.6pHFvieefN (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1808, bad_region=0, passed=18677
Got 18677 stars (including 16842 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat
util/solve_plate_with_UCAC5 got 18677 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 4856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 18677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 18677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4856 matched stars entering correct_measured_positions(), 18677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4856 stars left (next iteration limit 5341)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits N_match=4856 sigma_overall_arcsec=0.308 sigma_q1_arcsec=0.418 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.271 sigma_q4_arcsec=0.245 n_q1=1609 n_q2=1204 n_q3=763 n_q4=1280 worst_quadrant_to_overall_ratio=1.356
The image catalog is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -region wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ftOIRkjk9Q (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits' -> 'wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat corresponding to the image wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat corresponding to the image wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1757, bad_region=0, passed=18569
Got 18569 stars (including 16779 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat
util/solve_plate_with_UCAC5 got 18569 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 4857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 18569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 18569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 18569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4857 stars left (next iteration limit 5342)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits N_match=4857 sigma_overall_arcsec=0.390 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.394 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.351 n_q1=1197 n_q2=768 n_q3=1133 n_q4=1759 worst_quadrant_to_overall_ratio=1.371
The image catalog is written to wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits -region wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.qc0jf3M7IZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits.wcscat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits.wcscat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=367, bad_region=0, passed=6901
Got 6901 stars (including 6520 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits.wcscat
util/solve_plate_with_UCAC5 got 6901 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 6901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 6901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 6901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4863 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4863 robust_rms=9.191 arcsec worst_quadrant_rms=51.618 arcsec
SIP_REFIT: SIP order 3 trial: matched=4863 robust_rms=0.429 arcsec worst_quadrant_rms=0.505 arcsec
SIP_REFIT: SIP order 5 trial: matched=4863 robust_rms=0.297 arcsec worst_quadrant_rms=0.377 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4863 robust_rms_before=1.010 arcsec robust_rms_before_corrected=0.333 arcsec robust_rms_after=0.297 arcsec worst_quadrant_rms_before=0.451 worst_quadrant_rms_after=0.377
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:50.435 +37:59:15.66 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 6901 stars ###
'wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/correct_sextractor_wcs_catalog_usingxy2sky1648412.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.010 -> 0.297 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4863 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4720 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4720 pairs (4863 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4720 robust_rms=8.488 arcsec worst_quadrant_rms=59.368 arcsec
SIP_REFIT: SIP order 3 trial: matched=4720 robust_rms=0.426 arcsec worst_quadrant_rms=0.504 arcsec
SIP_REFIT: SIP order 5 trial: matched=4720 robust_rms=0.295 arcsec worst_quadrant_rms=0.387 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4720 robust_rms_before=0.295 arcsec robust_rms_before_corrected=0.295 arcsec robust_rms_after=0.295 arcsec worst_quadrant_rms_before=0.381 worst_quadrant_rms_after=0.387
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.387 vs 0.381 arcsec) - keeping the current solution
SIP_REFIT: the second refit on the re-matched pairs was not applied - keeping the first refit solution
Accuracy estimation diagnostic: 4720 matched stars entering correct_measured_positions(), 6901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4720 matched stars entering correct_measured_positions(), 6901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
WCS_QUALITY_DIAG: file=fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits N_match=4720 sigma_overall_arcsec=0.321 sigma_q1_arcsec=0.299 sigma_q2_arcsec=0.453 sigma_q3_arcsec=0.292 sigma_q4_arcsec=0.355 n_q1=1422 n_q2=553 n_q3=1761 n_q4=984 worst_quadrant_to_overall_ratio=1.412
The image catalog is written to wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits -region wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.0owOCANBB5 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits.wcscat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits.wcscat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=415, bad_region=1, passed=7732
Got 7732 stars (including 7299 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits.wcscat
util/solve_plate_with_UCAC5 got 7732 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 4859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 7730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 7730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 7730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4861 stars left (next iteration limit 5346)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4861 robust_rms=7.095 arcsec worst_quadrant_rms=86.089 arcsec
SIP_REFIT: SIP order 3 trial: matched=4861 robust_rms=0.428 arcsec worst_quadrant_rms=0.502 arcsec
SIP_REFIT: SIP order 5 trial: matched=4861 robust_rms=0.288 arcsec worst_quadrant_rms=0.371 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4861 robust_rms_before=1.030 arcsec robust_rms_before_corrected=0.324 arcsec robust_rms_after=0.288 arcsec worst_quadrant_rms_before=0.478 worst_quadrant_rms_after=0.371
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
verification OK: wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:21:47.841 +37:59:47.46 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 7732 stars ###
'wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/correct_sextractor_wcs_catalog_usingxy2sky1648895.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.030 -> 0.288 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4861 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4708 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4708 pairs (4861 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4708 robust_rms=6.946 arcsec worst_quadrant_rms=86.358 arcsec
SIP_REFIT: SIP order 3 trial: matched=4708 robust_rms=0.424 arcsec worst_quadrant_rms=0.500 arcsec
SIP_REFIT: SIP order 5 trial: matched=4708 robust_rms=0.287 arcsec worst_quadrant_rms=0.375 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4708 robust_rms_before=0.287 arcsec robust_rms_before_corrected=0.287 arcsec robust_rms_after=0.287 arcsec worst_quadrant_rms_before=0.374 worst_quadrant_rms_after=0.375
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.375 vs 0.374 arcsec) - keeping the current solution
SIP_REFIT: the second refit on the re-matched pairs was not applied - keeping the first refit solution
Accuracy estimation diagnostic: 4708 matched stars entering correct_measured_positions(), 7730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4708 matched stars entering correct_measured_positions(), 7731 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
WCS_QUALITY_DIAG: file=fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits N_match=4708 sigma_overall_arcsec=0.313 sigma_q1_arcsec=0.311 sigma_q2_arcsec=0.435 sigma_q3_arcsec=0.290 sigma_q4_arcsec=0.330 n_q1=1340 n_q2=534 n_q3=1834 n_q4=1000 worst_quadrant_to_overall_ratio=1.388
The image catalog is written to wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits -region wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits to local_wcs_cache/
'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'local_wcs_cache/wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
Saving the final (post-refit) wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits to local_wcs_cache/
'wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits' -> 'local_wcs_cache/wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits'
Saving the final (post-refit) wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits to local_wcs_cache/
'wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits'
Saving the final (post-refit) wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits to local_wcs_cache/
'wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits sigma_overall=0.308 worst_q_ratio=1.356
ref2=Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits sigma_overall=0.390 worst_q_ratio=1.371
new1=fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits sigma_overall=0.321 worst_q_ratio=1.412
new2=fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits sigma_overall=0.313 worst_q_ratio=1.388
reference average sigma_overall=0.349 worst_q_ratio=1.3635
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342_astrometric_residuals.png (4856 matched stars from wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025_astrometric_residuals.png (4857 matched stars from wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040_astrometric_residuals.png (4720 matched stars from wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041_astrometric_residuals.png (4708 matched stars from wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/wcs_fd_Per-05-Q1b1x1_2026-09-17_04-32-04_20.00sec_0.00C_LIGHTs_0040.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-17_CI_Per-05-Q1b1x1_043349_TTUQ1b1x1_1572296_AberuO3p/wcs_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041.fits'
Preparing the HTML report for the field Per-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:28.28 +36:27:44.1: 11.84 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:55.78 +34:45:46.6: 11.68 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:24.43 +36:06:11.1: 11.89 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:58.72 +36:01:58.3: 11.83 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:49.20 +34:05:02.5: 11.81 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:32.07 +35:00:45.8: 10.63 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:29.96 +34:29:10.1: 11.97 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:06.07 +36:04:21.6: 12.05 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:58.72 +36:01:58.3: 11.82 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:49.20 +34:05:02.5: 11.75 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:24.43 +36:06:11.1: 11.85 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:28.28 +36:27:44.1: 11.80 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:55.78 +34:45:46.6: 11.70 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Forced photometry reference-image weighted average: 11.78 +/- 0.01
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:58.72 +36:01:58.3: ref_mag=11.82 +/- 0.01 new_mean_mag=10.8126 delta=1.01 (need > 0.90)
Forced photometry filter KEPT candidate at 04:57:49.20 +34:05:02.5: ref_mag=11.78 +/- 0.01 new_mean_mag=10.8070 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 04:59:28.28 +36:27:44.1: ref_mag=11.82 +/- 0.01 new_mean_mag=10.8825 delta=0.94 (need > 0.90)
Forced photometry filter KEPT candidate at 04:59:24.43 +36:06:11.1: ref_mag=11.87 +/- 0.01 new_mean_mag=10.8643 delta=1.01 (need > 0.90)
Forced photometry reference-image weighted average: 11.69 +/- 0.01
Forced photometry filter REJECTED candidate at 04:56:55.78 +34:45:46.6: ref_mag=11.69 +/- 0.01 new_mean_mag=10.9201 delta=0.77 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:41.63 +34:38:39.5: 11.12 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:48.20 +34:47:38.9: 12.13 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:32.07 +35:00:45.8: 10.59 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:29.96 +34:29:10.1: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.61 +/- 0.00
Forced photometry reference-image weighted average: 11.96 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:32.07 +35:00:45.8: ref_mag=10.61 +/- 0.00 new_mean_mag=9.6739 delta=0.94 (need > 0.90)
Forced photometry filter KEPT candidate at 04:57:29.96 +34:29:10.1: ref_mag=11.96 +/- 0.01 new_mean_mag=10.9138 delta=1.05 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:06.07 +36:04:21.6: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry filter KEPT candidate at 04:59:06.07 +36:04:21.6: ref_mag=12.05 +/- 0.01 new_mean_mag=10.9999 delta=1.05 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:41.63 +34:38:39.5: 11.11 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:48.20 +34:47:38.9: 12.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.11 +/- 0.00
Forced photometry filter KEPT candidate at 04:56:41.63 +34:38:39.5: ref_mag=11.11 +/- 0.00 new_mean_mag=10.1364 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 12.12 +/- 0.01
Forced photometry filter KEPT candidate at 04:56:48.20 +34:47:38.9: ref_mag=12.12 +/- 0.01 new_mean_mag=11.0255 delta=1.10 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:28.70 +35:21:46.5: 12.27 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:28.70 +35:21:46.5: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Forced photometry filter KEPT candidate at 04:55:28.70 +35:21:46.5: ref_mag=12.27 +/- 0.01 new_mean_mag=11.3494 delta=0.92 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:59:26.11 +36:32:16.1: 12.27 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:59:26.11 +36:32:16.1: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry filter KEPT candidate at 04:59:26.11 +36:32:16.1: ref_mag=12.25 +/- 0.01 new_mean_mag=11.2885 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:32.96 +34:57:09.3: 12.29 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:54.48 +35:09:37.5: 11.47 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:32.96 +34:57:09.3: 12.24 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry filter KEPT candidate at 04:56:32.96 +34:57:09.3: ref_mag=12.26 +/- 0.01 new_mean_mag=11.3317 delta=0.93 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:54.48 +35:09:37.5: 11.46 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.47 +/- 0.00
Forced photometry filter KEPT candidate at 04:58:54.48 +35:09:37.5: ref_mag=11.47 +/- 0.00 new_mean_mag=10.5322 delta=0.93 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:46.97 +36:01:10.5: 11.59 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:10.21 +35:05:57.4: 11.66 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:44.55 +35:38:54.9: 11.63 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:46.97 +36:01:10.5: 11.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.60 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:46.97 +36:01:10.5: ref_mag=11.60 +/- 0.01 new_mean_mag=10.6316 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:10.21 +35:05:57.4: 11.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.66 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:10.21 +35:05:57.4: ref_mag=11.66 +/- 0.01 new_mean_mag=10.7088 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:44.55 +35:38:54.9: 11.58 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.61 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:44.55 +35:38:54.9: ref_mag=11.61 +/- 0.01 new_mean_mag=10.5326 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:45.33 +34:48:49.7: 12.41 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:15.55 +34:41:28.6: 12.42 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:17.10 +35:42:22.3: 12.38 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:45.33 +34:48:49.7: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter KEPT candidate at 04:57:45.33 +34:48:49.7: ref_mag=12.43 +/- 0.01 new_mean_mag=11.3184 delta=1.11 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:15.55 +34:41:28.6: 12.41 +/- 0.02 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:17.10 +35:42:22.3: 12.42 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter KEPT candidate at 04:56:15.55 +34:41:28.6: ref_mag=12.41 +/- 0.01 new_mean_mag=11.3291 delta=1.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:17.10 +35:42:22.3: ref_mag=12.40 +/- 0.01 new_mean_mag=11.2987 delta=1.10 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:13.23 +34:27:21.1: 12.36 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:57.30 +35:34:06.9: 12.31 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:13.23 +34:27:21.1: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:13.23 +34:27:21.1: ref_mag=12.35 +/- 0.01 new_mean_mag=11.3233 delta=1.02 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:17.59 +35:59:57.3: 12.27 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:57.30 +35:34:06.9: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:57.30 +35:34:06.9: ref_mag=12.30 +/- 0.01 new_mean_mag=11.2350 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:17.59 +35:59:57.3: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:17.59 +35:59:57.3: ref_mag=12.25 +/- 0.01 new_mean_mag=11.1701 delta=1.08 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:01.44 +34:22:45.0: 11.30 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:06.67 +34:24:03.2: 12.22 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:01.44 +34:22:45.0: 11.28 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.00
Forced photometry filter KEPT candidate at 04:58:01.44 +34:22:45.0: ref_mag=11.29 +/- 0.00 new_mean_mag=10.3420 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:06.67 +34:24:03.2: 12.26 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry filter KEPT candidate at 04:57:06.67 +34:24:03.2: ref_mag=12.24 +/- 0.01 new_mean_mag=11.1905 delta=1.05 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:55:37.36 +34:47:51.6: 12.17 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:55:37.36 +34:47:51.6: 12.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.15 +/- 0.01
Forced photometry filter KEPT candidate at 04:55:37.36 +34:47:51.6: ref_mag=12.15 +/- 0.01 new_mean_mag=11.2099 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:38.72 +34:53:44.6: 11.00 +/- 0.00 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:19.27 +35:40:25.1: 12.06 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:38.72 +34:53:44.6: 10.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.00 +/- 0.00
Forced photometry filter KEPT candidate at 04:58:38.72 +34:53:44.6: ref_mag=11.00 +/- 0.00 new_mean_mag=9.9848 delta=1.01 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:19.27 +35:40:25.1: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry filter KEPT candidate at 04:57:19.27 +35:40:25.1: ref_mag=12.01 +/- 0.01 new_mean_mag=11.1023 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:54:46.89 +35:30:30.4: 12.05 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:54:46.89 +35:30:30.4: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter KEPT candidate at 04:54:46.89 +35:30:30.4: ref_mag=12.06 +/- 0.01 new_mean_mag=11.0882 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:57:52.38 +34:17:23.0: 12.01 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:57:52.38 +34:17:23.0: 12.02 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter KEPT candidate at 04:57:52.38 +34:17:23.0: ref_mag=12.02 +/- 0.01 new_mean_mag=10.9651 delta=1.05 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:41.44 +35:58:36.6: 12.00 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:34.50 +35:00:37.5: 11.92 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:41.44 +35:58:36.6: 11.95 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.97 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:41.44 +35:58:36.6: ref_mag=11.97 +/- 0.01 new_mean_mag=10.9645 delta=1.01 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:34.50 +35:00:37.5: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.90 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:34.50 +35:00:37.5: ref_mag=11.90 +/- 0.01 new_mean_mag=10.8247 delta=1.07 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:56:26.04 +34:37:19.7: 12.04 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:56:26.04 +34:37:19.7: 12.01 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter KEPT candidate at 04:56:26.04 +34:37:19.7: ref_mag=12.02 +/- 0.01 new_mean_mag=10.9270 delta=1.09 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:04.74 +35:44:00.0: 11.88 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:04.74 +35:44:00.0: 11.86 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:04.74 +35:44:00.0: ref_mag=11.87 +/- 0.01 new_mean_mag=10.8989 delta=0.97 (need > 0.90)
Forced photometry on wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits at 04:58:56.05 +35:05:23.5: 11.74 +/- 0.01 detection
Forced photometry on wcs_Per-05-Q1b1x1_2026-01-08_20-03-57_20.00sec_-15.00C_LIGHT_0025.fits at 04:58:56.05 +35:05:23.5: 11.74 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.74 +/- 0.01
Forced photometry filter KEPT candidate at 04:58:56.05 +35:05:23.5: ref_mag=11.74 +/- 0.01 new_mean_mag=10.7145 delta=1.03 (need > 0.90)
Adding exclusion_list_local.txt__out12079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15641.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 33s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 16s
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Considering the candidate 22408_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 22408_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 22458_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 22458_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:04:12.08 +43:02:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22495_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 22495_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:23:36.64 +38:38:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16258_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 16258_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:22.66 +33:46:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15641_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 15641_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 12754_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 12754_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 12171_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 12171_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 16169_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 16169_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:51.99 +33:33:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12651_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 12651_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 16199_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 16199_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:58.97 +33:35:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15042_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 15042_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 14191_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14191_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 14907_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 14907_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:59.56 +34:35:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12692_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 12692_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 16443_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 16443_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:43.02 +33:39:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14581_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14581_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 14813_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14813_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 13848_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 13848_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 12079_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 12079_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 15427_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 15427_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:28.67 +34:14:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14366_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14366_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 14006_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14006_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 12786_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 12786_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 14107_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14107_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 13339_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 13339_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 17280_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 17280_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:49.05 +33:27:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14524_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14524_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 14766_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14766_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 13277_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 13277_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 15067_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 15067_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 13447_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 13447_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 12838_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 12838_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 15189_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 15189_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 15188_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 15188_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 14623_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14623_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 14357_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14357_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 17283_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 17283_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:03.75 +33:17:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13356_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 13356_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 13672_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 13672_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 15346_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 15346_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 12853_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 12853_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 14217_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14217_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 16038_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 16038_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:45.90 +33:49:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14838_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14838_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 17657_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 17657_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:04.56 +33:29:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15354_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 15354_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:07.65 +34:18:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17041_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 17041_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:01.25 +33:24:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13232_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 13232_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 14089_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 14089_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 15306_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 15306_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:00.66 +34:15:59.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 15760_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 15760_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:51.71 +33:58:37.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 18660_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 18660_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 168969_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168969_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:02:35.10 +35:24:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168973_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168973_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 168975_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168975_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 168976_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168976_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 168977_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168977_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 168983_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168983_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:24:23.77 +42:39:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168987_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168987_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 168991_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168991_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:04:38.62 +34:27:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168992_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168992_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:00:32.40 +41:36:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168994_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168994_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:12:12.20 +39:26:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168997_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168997_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:50:13.51 +37:24:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168998_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 168998_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:53:53.31 +36:58:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169048_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169048_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:04:12.09 +43:02:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169142_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169142_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:58:46.54 +35:47:50.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 169211_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169211_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 05:00:16.20 +39:38:29.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 169218_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169218_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:08:20.23 +43:10:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169329_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169329_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:48:04.74 +38:21:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169369_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169369_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:43:57.66 +38:23:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169373_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169373_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:51:25.11 +35:31:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169409_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169409_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 05:00:34.89 +40:12:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169411_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169411_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:44:29.51 +36:26:09.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 169462_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169462_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:51:45.61 +34:21:50.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 169487_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169487_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:14:54.34 +35:05:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169502_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169502_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:45:28.39 +38:40:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169504_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169504_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 05:00:37.62 +40:15:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169517_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169517_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:57:21.39 +40:02:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169518_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169518_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:44:59.32 +42:36:12.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 169639_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169639_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 05:00:09.41 +39:38:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169651_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169651_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:43:21.27 +36:51:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169702_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169702_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:56:37.09 +35:05:06.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 169749_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169749_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 169758_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169758_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 169791_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169791_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 169834_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169834_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:16:24.03 +36:43:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169836_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169836_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 169843_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169843_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:16:21.84 +36:43:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169867_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169867_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 169874_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169874_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:02:21.16 +40:05:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169900_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169900_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 169901_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169901_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 169909_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169909_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 169955_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169955_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 169999_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 169999_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 170003_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 170003_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:24:36.05 +34:06:47.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 24193_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 24193_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 05:02:28.26 +41:04:30.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 129626_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129626_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 89399_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 89399_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:59:28.25 +36:27:44.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 118196_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 118196_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 125596_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 125596_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:04.76 +35:43:59.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 86620_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 86620_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 128592_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128592_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 130409_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130409_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 102119_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 102119_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:29.96 +34:29:10.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 116610_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 116610_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:34.49 +35:00:37.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 101311_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101311_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 125320_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125320_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 111507_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 111507_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 86966_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 86966_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 130284_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130284_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 128378_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 128378_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:45.03 +33:32:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107921_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 107921_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 110453_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 110453_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131299_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 131299_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128876_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128876_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102184_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 102184_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123586_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123586_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100706_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100706_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:17.19 +33:43:17.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117918_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 117918_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:07.83 +35:10:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85423_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 85423_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88132_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 88132_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100475_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100475_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:17.00 +33:33:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128884_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 128884_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:33.32 +33:40:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105632_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 105632_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125823_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125823_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128776_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128776_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130709_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130709_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100759_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100759_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:06.63 +33:47:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129384_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129384_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101144_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101144_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:54.55 +33:59:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109939_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 109939_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:12.64 +33:18:53.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134239_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 134239_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110556_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 110556_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:53:53.50 +34:38:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123381_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123381_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108232_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 108232_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135654_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 135654_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:49.33 +33:40:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101431_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101431_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:50.82 +34:07:54.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121266_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 121266_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:37.25 +33:29:59.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125675_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125675_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130410_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130410_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124383_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124383_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124507_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124507_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88335_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 88335_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124564_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124564_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110214_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 110214_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123177_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123177_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121872_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 121872_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137272_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 137272_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:27.97 +33:35:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125866_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125866_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101423_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101423_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126912_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126912_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120052_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 120052_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132391_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 132391_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117989_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117989_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89039_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 89039_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106986_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 106986_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121374_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 121374_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128845_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128845_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123829_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123829_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102940_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 102940_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:13.80 +34:11:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116777_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 116777_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87952_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 87952_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113528_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 113528_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128259_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128259_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113237_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 113237_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:41.15 +34:45:23.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115715_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115715_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115936_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115936_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116445_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 116445_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109926_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 109926_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126766_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126766_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129351_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129351_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100620_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100620_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:29.88 +33:37:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115276_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115276_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117083_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117083_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115902_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115902_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113312_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 113312_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:40.80 +34:48:29.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101825_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101825_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:11.59 +34:21:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115763_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115763_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114079_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114079_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105629_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 105629_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101534_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101534_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 133385_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 133385_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 110244_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 110244_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 108605_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 108605_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:51.33 +34:30:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102192_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 102192_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 118271_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 118271_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 109723_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 109723_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 130212_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130212_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 129144_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129144_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 130816_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130816_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 128815_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128815_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 115290_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115290_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 131229_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 131229_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 90419_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 90419_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 110254_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 110254_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 129773_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129773_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 161450_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 161450_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
Rejecting candidate due to large distance (47.3") between the two second-epoch detections
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Considering the candidate 111124_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 111124_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:35.39 +33:17:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114757_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 114757_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:42.97 +34:56:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100658_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100658_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:08.67 +33:39:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115088_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115088_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 125829_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125829_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 112726_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112726_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 131002_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 131002_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 128974_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128974_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 112741_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112741_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 85860_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 85860_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 125938_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125938_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 125965_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125965_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 109728_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 109728_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 113780_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 113780_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111698_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 111698_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 114494_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 114494_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:07.39 +33:32:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114652_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114652_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 114459_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114459_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 108000_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 108000_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 87594_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 87594_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 123402_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123402_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 120152_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 120152_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 127385_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127385_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 89418_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 89418_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 136923_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 136923_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 115031_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115031_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 116147_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 116147_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 112509_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112509_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 124040_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124040_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125450_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125450_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 87325_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 87325_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 100728_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100728_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:52.96 +33:42:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127072_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127072_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 122180_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122180_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124254_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124254_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136920_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 136920_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:11.36 +33:43:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127680_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127680_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 130622_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130622_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 87471_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 87471_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112668_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112668_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 123706_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123706_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 116895_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 116895_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 117825_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 117825_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:03.04 +33:42:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89520_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 89520_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108467_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 108467_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:43.90 +34:27:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125920_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125920_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 112239_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112239_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 133492_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 133492_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100726_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100726_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:49.91 +33:46:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114697_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114697_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 134034_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 134034_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 129607_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129607_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 88677_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 88677_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101646_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101646_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 129611_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129611_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 112805_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112805_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 117035_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117035_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101894_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101894_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 119577_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 119577_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 133877_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 133877_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:58.07 +33:42:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133392_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 133392_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 117277_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117277_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 113992_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 113992_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 108703_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 108703_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:22.65 +33:20:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122517_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122517_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 130739_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130739_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101961_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101961_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:53:28.77 +34:29:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111416_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 111416_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:31.93 +33:14:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117126_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 117126_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:52:52.36 +35:09:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121983_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 121983_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 125175_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125175_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 127216_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127216_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 130825_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 130825_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:48.64 +33:34:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128233_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128233_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 133283_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 133283_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
Rejecting candidate due to large distance (47.0") between the two second-epoch detections
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Considering the candidate 110626_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 110626_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 113416_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 113416_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:20.66 +34:49:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115905_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 115905_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:09.51 +35:02:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112240_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112240_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 88638_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 88638_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 124954_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 124954_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:12.15 +35:47:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129721_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129721_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 102093_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 102093_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 125091_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125091_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 124547_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124547_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 115491_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115491_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 115675_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115675_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 117460_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117460_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 111290_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 111290_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 128466_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 128466_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:51.22 +35:58:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101167_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101167_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 114121_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114121_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 129873_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 129873_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 101056_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101056_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 112898_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112898_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 137148_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 137148_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101491_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101491_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 129581_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129581_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 117100_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117100_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101989_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101989_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 102168_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 102168_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 134776_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 134776_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 112367_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 112367_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:48.28 +33:14:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100463_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100463_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:41.96 +33:33:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100232_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100232_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:50.28 +33:03:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124467_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124467_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 115434_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115434_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 118682_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 118682_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 119769_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 119769_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 125879_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125879_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 122613_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122613_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 111376_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 111376_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 115059_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115059_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101453_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101453_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:58.65 +34:08:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130183_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130183_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 127736_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127736_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 108921_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 108921_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:12.52 +33:48:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127623_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127623_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 111743_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 111743_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
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Considering the candidate 101734_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101734_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100420_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100420_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:27.15 +33:29:37.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122207_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122207_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125088_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125088_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115489_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115489_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111663_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 111663_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113886_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 113886_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115017_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115017_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131260_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 131260_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127648_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127648_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102094_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 102094_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123430_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123430_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148827_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 148827_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123521_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123521_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122679_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122679_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108941_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 108941_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:22.16 +33:21:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101973_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101973_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126157_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126157_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129493_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129493_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120797_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 120797_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111334_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 111334_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123501_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123501_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118389_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 118389_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85655_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 85655_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107956_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 107956_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:06.57 +33:20:19.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123222_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123222_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127480_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127480_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121229_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 121229_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110559_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 110559_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:29.50 +34:36:16.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110466_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 110466_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129791_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 129791_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:29.00 +33:35:37.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100613_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100613_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:25.85 +33:37:56.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132708_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 132708_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121598_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 121598_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127123_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127123_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114405_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114405_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111919_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 111919_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:48.45 +34:41:33.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87481_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 87481_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101203_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101203_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111845_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 111845_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125127_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125127_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115006_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115006_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129708_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129708_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125796_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125796_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120380_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 120380_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121896_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 121896_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:35.43 +35:31:35.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121924_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 121924_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117114_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117114_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116143_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 116143_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86300_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 86300_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127259_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127259_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102042_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 102042_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114119_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114119_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127297_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127297_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88129_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 88129_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133934_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 133934_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136133_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 136133_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:00.64 +33:42:03.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115287_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115287_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101769_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101769_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114900_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114900_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132317_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 132317_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100603_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100603_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:31.79 +33:37:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129984_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129984_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128539_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128539_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104327_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 104327_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:02.75 +34:15:00.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104768_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 104768_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123896_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123896_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100650_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100650_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:25.39 +33:40:16.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102055_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 102055_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126612_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126612_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111719_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 111719_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136930_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 136930_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:10.81 +33:43:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112621_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112621_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89815_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 89815_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102181_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 102181_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105470_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 105470_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:30.04 +33:24:46.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115846_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115846_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129550_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129550_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23838_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 23838_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:56:15.75 +41:59:28.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115061_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115061_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106743_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 106743_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102078_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 102078_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86299_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 86299_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120543_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 120543_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126678_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126678_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104531_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 104531_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129465_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129465_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125486_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125486_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73635_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 73635_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:23:36.64 +38:38:03.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101876_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101876_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127764_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127764_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123511_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123511_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114989_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114989_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119914_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 119914_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132704_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 132704_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121517_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 121517_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125413_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125413_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122769_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122769_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118255_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 118255_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110714_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 110714_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:48.08 +33:16:35.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124739_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124739_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104486_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 104486_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:09.83 +33:27:36.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120119_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 120119_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123702_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123702_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85816_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 85816_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106733_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 106733_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127410_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127410_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113017_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 113017_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127311_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127311_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86797_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 86797_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112375_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112375_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114212_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114212_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110296_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 110296_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100435_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100435_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:21.25 +33:30:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110341_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 110341_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123471_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123471_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107408_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 107408_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:48.09 +33:48:13.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117381_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117381_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130436_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130436_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104358_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 104358_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133935_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 133935_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110120_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 110120_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121654_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 121654_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86748_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 86748_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125117_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125117_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108791_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 108791_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:33.54 +33:19:56.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125452_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125452_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133072_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 133072_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131565_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 131565_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111776_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 111776_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:15.83 +34:38:23.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112102_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112102_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101696_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101696_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101936_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101936_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113047_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 113047_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:35.27 +34:43:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114108_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114108_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119241_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 119241_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122638_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122638_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100705_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100705_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:57.66 +33:43:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125426_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125426_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112647_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112647_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131305_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 131305_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112631_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112631_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 117465_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117465_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117344_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117344_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 128517_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128517_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123464_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123464_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121096_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 121096_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 111090_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 111090_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130996_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130996_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131514_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 131514_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126159_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126159_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104086_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 104086_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:47.20 +33:28:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90211_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 90211_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114251_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114251_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114066_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114066_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102798_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 102798_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116396_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 116396_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100535_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100535_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:01.85 +33:38:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89159_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 89159_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101256_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101256_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:58.59 +34:01:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114841_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114841_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101542_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101542_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101926_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101926_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:26.92 +34:25:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126261_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126261_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108267_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 108267_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:47.72 +34:27:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104074_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 104074_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:37.96 +33:30:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113246_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 113246_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125847_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125847_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124805_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124805_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112775_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112775_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129379_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129379_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86567_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 86567_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101618_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101618_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:53.00 +34:15:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101867_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101867_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:50.52 +34:19:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116630_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 116630_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128072_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128072_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128617_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 128617_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114590_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114590_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127959_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127959_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105639_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 105639_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:10.60 +34:18:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115893_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115893_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114184_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 114184_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:45.32 +34:48:49.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 112649_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 112649_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:15.58 +34:41:27.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117386_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117386_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87160_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 87160_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:16:01.26 +37:20:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123162_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123162_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101701_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101701_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130787_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130787_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125394_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 125394_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:17.10 +35:42:22.2 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118214_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 118214_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121419_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 121419_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102109_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 102109_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:13.25 +34:27:20.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130282_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130282_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115138_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115138_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102759_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 102759_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:19.00 +33:28:52.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123536_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123536_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123813_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 123813_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:57.30 +35:34:06.9 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105502_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 105502_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:34.72 +33:26:31.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129507_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 129507_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:17.60 +35:59:57.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115538_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 115538_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:32.98 +34:57:09.0 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116470_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 116470_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122675_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122675_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122080_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122080_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126977_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126977_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120116_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 120116_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:28.71 +35:21:46.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 119505_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 119505_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 112288_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 112288_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:35.69 +34:41:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111528_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 111528_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:26.07 +34:37:19.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 89193_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 89193_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 32099_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 32099_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:13:31.53 +41:34:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89371_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 89371_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 107896_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 107896_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:06.67 +34:24:02.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 115035_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115035_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 124670_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124670_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 117318_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117318_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 117231_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117231_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 48618_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 48618_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:59:41.12 +39:56:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132027_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 132027_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 113572_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 113572_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:37.36 +34:47:51.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 108856_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 108856_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 116097_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 116097_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:31.09 +35:03:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113615_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 113615_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:48.20 +34:47:38.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 110563_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 110563_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 109445_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 109445_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:03.78 +33:17:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124814_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 124814_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:19.27 +35:40:25.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 118355_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 118355_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 129075_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129075_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 92722_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 92722_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122081_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 122081_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:46.88 +35:30:30.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 130794_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 130794_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:59:06.04 +36:04:22.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 112630_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112630_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 106013_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 106013_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:52.41 +34:17:22.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 113576_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 113576_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129297_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 129297_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:41.42 +35:58:36.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 135786_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 135786_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:59.01 +33:35:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100939_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100939_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:45.89 +33:49:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130689_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130689_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 100385_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100385_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:04.55 +33:29:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100354_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100354_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:01.28 +33:24:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101086_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101086_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 130180_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 130180_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:58.70 +36:01:58.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 131326_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 131326_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:59:24.44 +36:06:11.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 106007_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 106007_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:07.65 +34:18:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129173_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 129173_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:51.99 +33:33:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122763_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122763_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 121206_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 121206_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:08.92 +33:32:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113509_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 113509_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101426_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101426_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:49.22 +34:05:02.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 126635_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126635_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 115644_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 115644_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 136018_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 136018_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:12.97 +33:43:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120681_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 120681_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:22.65 +33:46:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117793_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 117793_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:56.04 +35:05:23.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 112184_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112184_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 107031_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 107031_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 126066_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126066_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106121_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 106121_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:22.37 +33:24:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117652_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 117652_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:10.20 +35:05:57.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 125701_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125701_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 104458_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 104458_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:48.99 +33:27:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125560_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 125560_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124579_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 124579_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:44.56 +35:38:54.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 101895_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101895_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:14.58 +34:21:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131226_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 131226_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:46.96 +36:01:10.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 131211_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 131211_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:24.35 +33:36:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94341_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 94341_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:51:16.63 +33:02:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69831_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 69831_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:10:03.00 +39:04:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123837_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 123837_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101496_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101496_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 100990_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100990_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:49.57 +33:51:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101707_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101707_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:28.64 +34:14:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134304_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 134304_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 114189_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114189_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 124557_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124557_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 108014_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 108014_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:01.44 +34:22:44.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 111783_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 111783_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 106731_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 106731_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 102107_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 102107_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 104556_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 104556_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:13.81 +34:17:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111823_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 111823_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:41.67 +34:38:38.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 115279_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 115279_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:38.73 +34:53:44.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 136549_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 136549_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:43.03 +33:39:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111912_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 111912_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:07.11 +34:40:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106176_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 106176_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:22.95 +33:22:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106983_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 106983_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:55.19 +34:22:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122908_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122908_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 126932_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126932_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 116500_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 116500_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 112896_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112896_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112628_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 112628_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124751_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124751_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113574_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 113574_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119816_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 119816_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 107098_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 107098_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101826_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101826_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:58.82 +34:20:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127200_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 127200_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130976_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130976_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117091_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117091_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110836_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 110836_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:55:59.69 +34:35:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117179_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 117179_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116557_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 116557_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:32.06 +35:00:46.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 02995_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 02995_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 03:51:50.97 +43:02:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107917_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 107917_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114462_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114462_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126042_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126042_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 114793_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 114793_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101869_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101869_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 126811_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 126811_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101604_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101604_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 133059_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 133059_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108679_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 108679_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100849_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100849_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:53.57 +33:47:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130654_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 130654_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129237_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 129237_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122418_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 122418_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113786_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 113786_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 104124_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 104124_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100719_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 100719_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:30.69 +33:43:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107015_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 107015_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116545_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 116545_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 101326_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101326_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
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Considering the candidate 131915_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 131915_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108461_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 108461_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113040_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 113040_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:57:34.11 +34:42:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105635_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 105635_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:58:00.68 +34:15:58.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 101643_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 101643_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:54:15.84 +34:18:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124352_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 124352_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134333_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 134333_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:51.71 +33:58:37.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 101733_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
Preparing report for the candidate 101733_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21520_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 21520_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 05:03:18.71 +41:26:29.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 93179_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 93179_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:49:19.11 +32:35:16.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74576_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 74576_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:59:15.40 +37:53:21.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 86685_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 86685_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:52:37.66 +36:42:11.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135996_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041
The candidate 135996_fd_Per-05-Q1b1x1_2026-09-17_04-33-07_20.00sec_0.00C_LIGHTs_0041 did not pass the final checks
**** FOUND 04:56:59.26 +33:09:59.9 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 30s
make_report_in_HTML.sh TOTAL: 817s
Prepared the HTML report for the field Per-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:59:26.11 +36:32:16.1
04:59:28.28 +36:27:44.1
04:59:24.43 +36:06:11.1
04:59:06.07 +36:04:21.6
04:58:58.72 +36:01:58.3
04:58:46.97 +36:01:10.5
04:58:17.59 +35:59:57.3
04:58:41.44 +35:58:36.6
04:58:04.74 +35:44:00.0
04:58:17.10 +35:42:22.3
04:58:44.55 +35:38:54.9
04:57:19.27 +35:40:25.1
04:58:57.30 +35:34:06.9
04:54:46.89 +35:30:30.4
04:55:28.70 +35:21:46.5
04:58:54.48 +35:09:37.5
04:58:56.05 +35:05:23.5
04:58:10.21 +35:05:57.4
04:58:32.07 +35:00:45.8
04:58:34.50 +35:00:37.5
04:58:38.72 +34:53:44.6
04:56:32.96 +34:57:09.3
04:57:45.33 +34:48:49.7
04:56:48.20 +34:47:38.9
04:55:37.36 +34:47:51.6
04:56:15.55 +34:41:28.6
04:56:41.63 +34:38:39.5
04:56:26.04 +34:37:19.7
04:57:29.96 +34:29:10.1
04:58:13.23 +34:27:21.1
04:57:06.67 +34:24:03.2
04:58:01.44 +34:22:45.0
04:57:52.38 +34:17:23.0
04:57:49.20 +34:05:02.5
04:57:50.81 +33:51:47.6
04:57:58.94 +33:53:26.0
04:57:54.08 +33:58:12.0
04:58:02.42 +33:58:36.8
04:57:45.98 +34:01:46.9
04:57:54.76 +34:01:54.5
04:58:03.17 +34:04:34.7
04:57:16.08 +34:07:16.1
04:57:46.97 +34:06:30.6
04:58:12.18 +34:08:43.8
04:57:53.23 +34:09:17.3
04:57:40.64 +34:11:36.4
04:56:36.18 +34:14:49.7
04:56:30.86 +34:15:42.8
04:57:01.86 +34:15:03.6
04:57:43.42 +34:14:28.1
04:58:10.15 +34:13:47.0
04:56:46.06 +34:16:33.7
04:55:13.47 +34:22:15.8
04:57:48.25 +34:18:44.0
04:56:47.46 +34:20:59.5
04:57:43.77 +34:22:45.1
04:56:00.39 +34:26:27.8
04:55:35.37 +34:28:01.8
04:55:40.91 +34:30:10.4
04:58:21.94 +34:26:26.1
04:56:59.61 +34:28:47.8
04:57:46.58 +34:27:43.2
04:57:45.79 +34:28:02.7
04:56:28.11 +34:29:52.7
04:55:27.00 +34:38:44.2
04:58:13.85 +34:34:58.5
04:56:39.45 +34:40:25.2
04:56:50.93 +34:40:36.5
04:57:30.07 +33:28:54.9
04:57:46.45 +34:10:12.4
04:57:03.17 +34:12:16.6
04:56:59.98 +34:13:07.7
04:56:45.91 +34:15:07.6
04:56:31.07 +34:17:26.7
04:57:18.59 +34:16:18.5
04:58:02.68 +34:18:39.4
04:58:12.43 +34:18:27.4
04:56:46.52 +33:23:05.7
04:56:11.07 +34:22:11.3
04:56:21.50 +34:22:02.4
04:58:01.38 +34:19:30.6
04:58:20.26 +34:19:17.1
04:56:35.72 +34:25:06.8
04:55:57.17 +34:25:54.0
04:55:20.28 +34:27:58.8
04:58:22.63 +34:23:43.3
04:55:13.19 +34:28:21.3
04:57:34.95 +34:26:05.7
04:57:34.34 +34:26:45.5
04:55:59.31 +34:32:40.2
04:56:34.51 +34:31:49.4
04:55:10.12 +34:33:20.7
04:57:05.50 +34:31:10.6
04:57:22.48 +34:31:57.0
04:57:52.66 +34:33:18.9
04:57:12.91 +34:32:01.4
04:57:31.76 +34:31:51.0
04:58:03.95 +34:31:19.4
04:57:58.76 +34:32:19.6
04:55:54.39 +34:34:17.7
04:57:07.20 +34:32:54.8
04:56:34.68 +34:34:43.8
04:57:34.38 +34:34:55.8
04:56:39.34 +34:36:30.2
04:56:36.85 +34:37:33.4
04:57:18.50 +34:33:47.5
04:57:12.09 +34:36:17.8
04:56:38.36 +34:38:28.4
04:56:09.32 +34:39:17.3
04:56:44.17 +34:39:21.3
04:56:03.80 +34:41:12.0
04:56:39.49 +34:38:58.2
04:57:12.09 +34:38:24.6
04:55:54.19 +34:39:16.3
04:56:00.30 +34:40:38.1
04:57:07.09 +34:38:12.1
04:56:44.50 +34:40:03.7
04:55:43.15 +34:41:35.6
04:55:10.48 +34:43:43.6
04:56:57.19 +34:40:37.0
04:56:22.74 +34:41:46.3
04:57:15.18 +34:40:32.4
04:57:05.84 +34:40:59.3
04:56:52.51 +34:42:13.6
04:55:03.49 +34:43:30.6
04:57:56.28 +34:40:07.4
04:57:32.91 +34:40:35.3
04:57:52.32 +34:40:22.1
04:56:29.26 +34:43:41.0
04:56:49.87 +34:43:14.4
04:56:42.84 +34:43:41.3
04:57:17.61 +34:43:50.7
04:56:16.48 +34:47:05.1
04:57:04.49 +34:46:04.7
04:56:57.64 +34:45:37.5
04:56:55.83 +34:45:46.0
04:55:27.86 +34:49:38.2
04:56:43.07 +34:47:46.1
04:57:08.10 +34:47:46.0
04:57:08.29 +34:48:33.7
04:57:43.34 +34:47:36.3
04:54:56.40 +34:53:50.2
04:58:15.65 +34:48:44.1
04:56:15.01 +34:50:49.3
04:57:10.51 +34:49:23.5
04:58:07.87 +34:46:44.9
04:56:33.27 +34:50:46.7
04:55:34.81 +34:51:24.4
04:57:18.11 +34:50:37.6
04:55:44.12 +34:52:37.8
04:57:49.42 +34:50:18.2
04:58:05.29 +34:50:50.8
04:57:21.74 +34:50:09.4
04:55:36.58 +34:54:06.6
04:57:01.70 +34:52:25.2
04:55:20.74 +34:56:06.4
04:58:00.39 +34:52:51.4
04:56:22.90 +34:54:46.8
04:58:35.08 +34:51:36.0
04:57:13.54 +34:52:29.0
04:55:01.84 +34:56:55.5
04:56:50.38 +34:54:16.3
04:58:28.93 +34:53:04.8
04:58:34.83 +34:52:58.4
04:58:23.79 +34:50:58.5
04:57:54.53 +34:55:31.7
04:58:40.35 +34:54:34.0
04:58:41.26 +34:53:59.2
04:58:27.65 +34:53:52.1
04:57:38.46 +34:53:57.8
04:55:33.75 +34:58:44.7
04:56:19.08 +34:57:43.7
04:57:17.88 +34:56:19.3
04:55:09.86 +34:57:31.4
04:58:37.61 +34:55:40.6
04:55:00.96 +35:00:48.9
04:55:57.06 +35:00:06.9
04:57:59.16 +34:57:13.6
04:56:49.64 +34:58:30.4
04:55:53.87 +34:56:42.3
04:55:19.62 +35:02:58.0
04:58:43.18 +34:55:20.4
04:57:42.03 +35:01:06.6
04:57:53.36 +35:00:42.0
04:58:12.45 +35:01:09.6
04:55:33.55 +35:04:37.6
04:56:16.82 +35:02:58.3
04:56:41.50 +35:03:22.8
04:58:01.58 +35:00:44.2
04:58:18.55 +35:01:59.7
04:55:10.41 +35:07:49.0
04:56:00.89 +35:05:59.7
04:58:14.24 +35:02:38.9
04:55:32.90 +35:07:55.2
04:54:55.75 +35:07:55.2
04:56:28.41 +35:07:17.7
04:54:45.24 +35:10:04.2
04:58:48.76 +35:02:26.4
04:58:36.28 +35:02:35.6
04:58:35.64 +35:04:19.8
04:57:24.04 +35:06:27.5
04:58:25.35 +35:05:03.1
04:57:15.90 +35:06:34.4
04:57:30.14 +35:06:36.5
04:54:06.75 +35:13:44.2
04:54:47.51 +35:13:42.7
04:56:25.70 +35:11:37.0
04:56:06.35 +35:12:24.2
04:56:48.30 +35:10:14.4
04:54:57.53 +35:15:05.5
04:58:36.85 +35:06:13.1
04:58:06.24 +35:11:20.8
04:54:43.46 +35:19:47.5
04:55:08.13 +35:18:10.8
04:55:11.47 +35:17:57.3
04:56:27.99 +35:18:57.9
04:55:25.15 +35:20:41.9
04:55:05.07 +35:20:34.4
04:57:15.52 +33:30:19.1
04:55:45.94 +35:21:31.0
04:54:51.25 +35:23:45.5
04:55:24.29 +35:22:43.0
04:53:49.10 +35:26:42.2
04:55:19.66 +35:26:33.7
04:55:06.80 +35:27:13.8
04:57:34.14 +34:07:14.4
04:55:03.48 +35:28:38.7
04:55:46.37 +35:28:08.5
04:54:23.69 +35:30:36.6
04:55:43.91 +35:28:49.5
04:55:39.53 +35:29:44.2
04:53:57.39 +35:32:17.9
04:54:36.91 +35:31:50.7
04:54:52.60 +35:31:05.5
04:55:50.80 +35:27:50.9
04:56:31.61 +35:29:59.0
04:58:49.38 +35:27:00.8
04:58:53.54 +35:27:58.5
04:55:39.53 +35:33:03.5
04:55:12.08 +35:35:10.4
04:54:41.92 +35:36:08.3
04:56:01.70 +35:32:16.7
04:55:19.25 +35:34:22.5
04:55:48.47 +35:35:06.6
04:58:38.49 +35:30:34.3
04:59:10.11 +35:30:11.3
04:53:58.43 +35:39:18.3
04:58:20.82 +35:32:50.8
04:58:41.28 +35:28:39.6
04:58:40.91 +35:31:39.2
04:55:51.69 +35:35:59.8
04:56:36.96 +35:36:36.6
04:53:46.43 +35:39:21.7
04:54:12.16 +35:39:33.6
04:55:40.63 +35:36:40.5
04:54:09.02 +35:39:48.7
04:58:52.58 +35:32:46.9
04:56:00.46 +35:37:56.2
04:54:48.66 +35:39:42.8
04:55:45.27 +35:38:07.6
04:57:30.28 +35:36:07.8
04:55:29.65 +35:39:50.3
04:59:10.79 +35:33:35.7
04:54:52.89 +35:40:11.5
04:58:23.55 +35:36:55.0
04:54:49.37 +35:41:49.6
04:55:27.31 +35:42:06.6
04:53:35.12 +35:40:33.1
04:55:10.34 +35:42:58.9
04:56:32.93 +35:40:53.4
04:54:37.32 +35:44:05.6
04:58:51.62 +35:36:38.1
04:58:48.20 +35:37:06.4
04:58:53.10 +35:38:34.8
04:54:33.72 +35:43:02.0
04:58:56.28 +35:38:34.5
04:58:24.81 +35:40:53.4
04:54:04.22 +35:48:39.6
04:54:30.72 +35:46:11.8
04:57:46.65 +35:41:59.3
04:59:01.15 +35:40:04.6
04:55:30.08 +35:45:57.8
04:58:55.62 +35:39:57.6
04:54:25.89 +35:48:20.8
04:56:46.38 +35:45:30.6
04:57:06.75 +35:43:50.4
04:58:22.94 +35:42:33.7
04:59:16.11 +35:41:23.0
04:59:10.94 +35:39:11.1
04:53:07.59 +35:48:44.0
04:54:51.01 +35:49:18.9
04:54:35.18 +35:49:45.9
04:54:06.61 +35:51:03.9
04:55:43.97 +35:47:46.9
04:57:29.75 +35:45:08.3
04:58:29.87 +35:43:51.1
04:59:05.05 +35:42:49.0
04:58:35.68 +35:42:13.6
04:58:11.05 +35:44:39.2
04:55:00.82 +35:49:28.9
04:56:43.88 +35:47:20.5
04:57:17.39 +35:46:24.8
04:58:04.62 +35:46:23.9
04:59:06.78 +35:44:46.4
04:57:35.39 +35:47:09.8
04:56:50.77 +35:50:18.3
04:58:44.79 +35:47:22.9
04:58:47.09 +35:47:40.9
04:53:38.69 +35:55:19.6
04:58:17.63 +35:48:36.9
04:54:23.13 +35:55:04.1
04:59:24.25 +35:47:28.1
04:54:32.77 +35:55:15.5
04:57:55.69 +35:48:54.1
04:54:46.79 +35:55:01.9
04:59:08.12 +35:48:34.2
04:54:13.04 +35:56:20.8
04:58:41.68 +35:50:02.3
04:57:28.08 +35:51:45.0
04:58:52.51 +35:50:15.2
04:59:28.82 +35:49:28.8
04:59:05.82 +35:49:46.8
04:53:51.72 +35:56:38.2
04:54:00.64 +35:57:52.7
04:57:59.51 +35:52:27.6
04:57:07.10 +35:53:26.4
04:59:09.44 +35:50:49.1
04:59:13.58 +35:50:02.2
04:57:53.92 +35:54:26.8
04:58:48.76 +35:53:36.5
04:58:30.07 +35:54:10.0
04:58:08.36 +35:53:38.0
04:59:28.13 +35:54:04.1
04:59:13.20 +35:54:16.3
04:58:07.35 +35:57:00.8
04:58:41.94 +35:56:13.9
04:58:26.58 +35:56:58.5
04:55:35.07 +36:01:42.8
04:56:20.92 +36:00:20.6
04:59:29.06 +35:55:19.3
04:59:08.68 +35:56:45.7
04:57:59.96 +35:58:33.2
04:56:00.53 +36:01:23.1
04:58:19.56 +35:58:28.6
04:56:41.97 +36:02:13.9
04:58:09.65 +35:59:09.5
04:58:03.19 +35:57:57.9
04:56:22.74 +36:02:39.8
04:58:55.59 +35:58:34.9
04:59:07.74 +35:58:56.1
04:57:55.89 +35:59:50.2
04:58:48.44 +35:59:26.7
04:56:25.77 +36:02:30.7
04:57:05.54 +36:01:50.9
04:56:36.99 +36:02:52.3
04:58:42.00 +36:00:43.4
04:58:36.02 +36:01:14.0
04:58:51.51 +36:01:23.2
04:59:21.24 +36:01:09.2
04:56:08.90 +36:05:01.6
04:58:04.65 +36:03:52.7
04:59:16.83 +36:02:12.4
04:59:20.50 +36:02:23.8
04:58:37.99 +36:03:35.2
04:58:12.03 +36:04:51.6
04:58:06.38 +36:05:09.4
04:57:25.37 +36:05:47.2
04:58:26.66 +36:04:18.8
04:57:34.69 +36:05:34.4
04:58:26.89 +36:05:19.3
04:59:21.45 +36:03:35.9
04:59:39.38 +36:03:58.9
04:59:20.30 +36:04:48.7
04:57:50.71 +36:07:24.9
04:57:20.42 +36:07:57.4
04:53:59.36 +36:13:31.3
04:58:36.01 +36:07:09.7
04:58:49.84 +36:07:08.1
04:59:32.31 +36:05:05.4
04:59:20.57 +36:06:20.0
04:59:20.58 +36:07:23.9
04:58:18.10 +36:10:23.3
04:58:26.12 +36:10:02.4
04:57:58.94 +36:13:02.9
04:59:41.99 +36:09:44.3
04:59:14.39 +36:12:09.7
04:59:46.38 +36:11:18.9
04:58:43.17 +36:14:43.8
04:59:35.36 +36:12:54.4
04:59:23.87 +36:14:56.5
04:59:22.70 +36:14:15.1
04:59:45.63 +36:13:49.6
04:58:31.29 +36:18:32.2
04:59:13.89 +36:17:30.8
04:58:38.90 +36:18:32.6
04:57:46.02 +33:33:36.5
04:59:49.17 +36:17:23.7
04:59:07.94 +36:20:51.9
04:57:29.99 +33:51:53.0
04:57:31.22 +33:55:16.2
05:00:03.85 +36:50:48.8
04:59:58.79 +36:49:24.1
04:59:57.26 +36:48:09.3
04:59:39.48 +36:48:51.1
04:59:51.47 +36:45:37.2
04:59:57.62 +36:45:31.5
04:59:55.05 +36:43:36.0
04:59:34.00 +36:43:33.1
04:59:44.38 +36:43:21.0
04:59:31.01 +36:43:25.3
04:59:15.41 +36:42:37.9
04:59:31.17 +36:40:42.8
05:00:00.83 +36:39:09.2
04:59:41.14 +36:39:34.0
04:59:30.11 +36:39:02.4
04:59:46.05 +36:36:46.7
04:59:31.44 +36:35:39.8
05:00:00.55 +36:34:56.6
04:59:55.75 +36:34:26.2
04:59:37.46 +36:33:04.6
04:59:56.53 +36:32:22.2
04:59:57.92 +36:30:38.9
04:59:18.31 +36:31:03.5
04:59:35.13 +36:30:25.6
04:59:15.21 +36:29:56.6
04:59:46.18 +36:28:31.9
04:59:49.14 +36:27:55.8
04:59:42.67 +36:26:04.0
04:59:46.13 +36:24:20.8
04:59:30.66 +36:23:25.4
########### Completed Per-05-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 ####
04:57:49.20 +34:05:02.5
04:58:58.72 +36:01:58.3
04:59:28.28 +36:27:44.1
04:59:24.43 +36:06:11.1
04:57:29.96 +34:29:10.1
04:58:32.07 +35:00:45.8
04:59:06.07 +36:04:21.6
04:56:48.20 +34:47:38.9
04:56:41.63 +34:38:39.5
04:55:28.70 +35:21:46.5
04:59:26.11 +36:32:16.1
04:56:32.96 +34:57:09.3
04:58:54.48 +35:09:37.5
04:58:46.97 +36:01:10.5
04:58:10.21 +35:05:57.4
04:58:44.55 +35:38:54.9
04:57:45.33 +34:48:49.7
04:56:15.55 +34:41:28.6
04:58:17.10 +35:42:22.3
04:58:13.23 +34:27:21.1
04:58:57.30 +35:34:06.9
04:58:17.59 +35:59:57.3
04:58:01.44 +34:22:45.0
04:57:06.67 +34:24:03.2
04:55:37.36 +34:47:51.6
04:58:38.72 +34:53:44.6
04:57:19.27 +35:40:25.1
04:54:46.89 +35:30:30.4
04:57:52.38 +34:17:23.0
04:58:41.44 +35:58:36.6
04:58:34.50 +35:00:37.5
04:56:26.04 +34:37:19.7
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04:55:27.31 +35:42:06.6
04:57:43.42 +34:14:28.1
###################################################################################
04:57:49.20 +34:05:02.5 -- not an asteroid (will add it to exclusion list)
04:58:58.72 +36:01:58.3 -- not an asteroid (will add it to exclusion list)
04:59:28.28 +36:27:44.1 -- not an asteroid (will add it to exclusion list)
04:59:24.43 +36:06:11.1 -- not an asteroid (will add it to exclusion list)
04:57:29.96 +34:29:10.1 -- not an asteroid (will add it to exclusion list)
04:58:32.07 +35:00:45.8 -- not an asteroid (will add it to exclusion list)
04:59:06.07 +36:04:21.6 -- not an asteroid (will add it to exclusion list)
04:56:48.20 +34:47:38.9 -- not an asteroid (will add it to exclusion list)
04:56:41.63 +34:38:39.5 -- not an asteroid (will add it to exclusion list)
04:55:28.70 +35:21:46.5 -- not an asteroid (will add it to exclusion list)
04:59:26.11 +36:32:16.1 -- not an asteroid (will add it to exclusion list)
04:56:32.96 +34:57:09.3 -- not an asteroid (will add it to exclusion list)
04:58:54.48 +35:09:37.5 -- not an asteroid (will add it to exclusion list)
04:58:46.97 +36:01:10.5 -- not an asteroid (will add it to exclusion list)
04:58:10.21 +35:05:57.4 -- not an asteroid (will add it to exclusion list)
04:58:44.55 +35:38:54.9 -- not an asteroid (will add it to exclusion list)
04:57:45.33 +34:48:49.7 -- not an asteroid (will add it to exclusion list)
04:56:15.55 +34:41:28.6 -- not an asteroid (will add it to exclusion list)
04:58:17.10 +35:42:22.3 -- not an asteroid (will add it to exclusion list)
04:58:13.23 +34:27:21.1 -- not an asteroid (will add it to exclusion list)
04:58:57.30 +35:34:06.9 -- not an asteroid (will add it to exclusion list)
04:58:17.59 +35:59:57.3 -- not an asteroid (will add it to exclusion list)
04:58:01.44 +34:22:45.0 -- not an asteroid (will add it to exclusion list)
04:57:06.67 +34:24:03.2 -- not an asteroid (will add it to exclusion list)
04:55:37.36 +34:47:51.6 -- not an asteroid (will add it to exclusion list)
04:58:38.72 +34:53:44.6 -- not an asteroid (will add it to exclusion list)
04:57:19.27 +35:40:25.1 -- not an asteroid (will add it to exclusion list)
04:54:46.89 +35:30:30.4 -- not an asteroid (will add it to exclusion list)
04:57:52.38 +34:17:23.0 -- not an asteroid (will add it to exclusion list)
04:58:41.44 +35:58:36.6 -- not an asteroid (will add it to exclusion list)
04:58:34.50 +35:00:37.5 -- not an asteroid (will add it to exclusion list)
04:56:26.04 +34:37:19.7 -- not an asteroid (will add it to exclusion list)
04:58:04.74 +35:44:00.0 -- not an asteroid (will add it to exclusion list)
04:58:56.05 +35:05:23.5 -- not an asteroid (will add it to exclusion list)
04:57:05.54 +36:01:50.9 -- not an asteroid (will add it to exclusion list)
04:54:47.51 +35:13:42.7 -- not an asteroid (will add it to exclusion list)
04:59:34.00 +36:43:33.1 -- not an asteroid (will add it to exclusion list)
04:58:07.35 +35:57:00.8 -- not an asteroid (will add it to exclusion list)
04:59:20.50 +36:02:23.8 -- not an asteroid (will add it to exclusion list)
04:57:45.98 +34:01:46.9 -- not an asteroid (will add it to exclusion list)
04:58:55.62 +35:39:57.6 -- not an asteroid (will add it to exclusion list)
04:57:12.09 +34:36:17.8 -- not an asteroid (will add it to exclusion list)
04:59:15.41 +36:42:37.9 -- not an asteroid (will add it to exclusion list)
04:59:16.83 +36:02:12.4 -- not an asteroid (will add it to exclusion list)
04:55:57.17 +34:25:54.0 -- not an asteroid (will add it to exclusion list)
04:57:58.76 +34:32:19.6 -- not an asteroid (will add it to exclusion list)
04:58:49.84 +36:07:08.1 -- not an asteroid (will add it to exclusion list)
04:59:29.06 +35:55:19.3 -- not an asteroid (will add it to exclusion list)
04:56:39.45 +34:40:25.2 -- not an asteroid (will add it to exclusion list)
04:54:48.66 +35:39:42.8 -- not an asteroid (will add it to exclusion list)
05:00:03.85 +36:50:48.8 -- not an asteroid (will add it to exclusion list)
05:00:00.55 +36:34:56.6 -- not an asteroid (will add it to exclusion list)
04:57:18.59 +34:16:18.5 -- not an asteroid (will add it to exclusion list)
04:54:06.61 +35:51:03.9 -- not an asteroid (will add it to exclusion list)
04:58:26.58 +35:56:58.5 -- not an asteroid (will add it to exclusion list)
04:57:34.69 +36:05:34.4 -- not an asteroid (will add it to exclusion list)
04:58:03.19 +35:57:57.9 -- not an asteroid (will add it to exclusion list)
04:57:46.02 +33:33:36.5 -- not an asteroid (will add it to exclusion list)
04:58:40.91 +35:31:39.2 -- not an asteroid (will add it to exclusion list)
04:58:22.63 +34:23:43.3 -- asteroid (will NOT add it to exclusion list)
04:53:07.59 +35:48:44.0 -- not an asteroid (will add it to exclusion list)
04:58:37.99 +36:03:35.2 -- not an asteroid (will add it to exclusion list)
04:53:35.12 +35:40:33.1 -- not an asteroid (will add it to exclusion list)
04:56:32.93 +35:40:53.4 -- not an asteroid (will add it to exclusion list)
04:59:55.75 +36:34:26.2 -- not an asteroid (will add it to exclusion list)
04:58:48.20 +35:37:06.4 -- not an asteroid (will add it to exclusion list)
04:57:22.48 +34:31:57.0 -- not an asteroid (will add it to exclusion list)
04:58:20.82 +35:32:50.8 -- not an asteroid (will add it to exclusion list)
04:53:57.39 +35:32:17.9 -- not an asteroid (will add it to exclusion list)
04:58:29.87 +35:43:51.1 -- not an asteroid (will add it to exclusion list)
04:58:03.17 +34:04:34.7 -- not an asteroid (will add it to exclusion list)
04:54:23.13 +35:55:04.1 -- not an asteroid (will add it to exclusion list)
04:57:15.52 +33:30:19.1 -- not an asteroid (will add it to exclusion list)
04:59:41.99 +36:09:44.3 -- not an asteroid (will add it to exclusion list)
04:54:06.75 +35:13:44.2 -- not an asteroid (will add it to exclusion list)
04:59:57.92 +36:30:38.9 -- not an asteroid (will add it to exclusion list)
04:56:11.07 +34:22:11.3 -- not an asteroid (will add it to exclusion list)
04:55:03.48 +35:28:38.7 -- not an asteroid (will add it to exclusion list)
04:56:20.92 +36:00:20.6 -- not an asteroid (will add it to exclusion list)
04:55:29.65 +35:39:50.3 -- not an asteroid (will add it to exclusion list)
04:58:01.58 +35:00:44.2 -- not an asteroid (will add it to exclusion list)
04:59:46.05 +36:36:46.7 -- not an asteroid (will add it to exclusion list)
04:57:04.49 +34:46:04.7 -- not an asteroid (will add it to exclusion list)
04:58:08.36 +35:53:38.0 -- not an asteroid (will add it to exclusion list)
04:58:37.61 +34:55:40.6 -- not an asteroid (will add it to exclusion list)
04:55:53.87 +34:56:42.3 -- not an asteroid (will add it to exclusion list)
04:57:53.36 +35:00:42.0 -- not an asteroid (will add it to exclusion list)
04:55:10.12 +34:33:20.7 -- not an asteroid (will add it to exclusion list)
04:53:38.69 +35:55:19.6 -- not an asteroid (will add it to exclusion list)
04:56:41.97 +36:02:13.9 -- not an asteroid (will add it to exclusion list)
04:58:40.35 +34:54:34.0 -- not an asteroid (will add it to exclusion list)
04:56:00.89 +35:05:59.7 -- not an asteroid (will add it to exclusion list)
04:56:49.64 +34:58:30.4 -- not an asteroid (will add it to exclusion list)
04:55:00.96 +35:00:48.9 -- not an asteroid (will add it to exclusion list)
04:54:56.40 +34:53:50.2 -- not an asteroid (will add it to exclusion list)
04:56:31.07 +34:17:26.7 -- not an asteroid (will add it to exclusion list)
04:58:12.18 +34:08:43.8 -- not an asteroid (will add it to exclusion list)
04:59:23.87 +36:14:56.5 -- not an asteroid (will add it to exclusion list)
04:57:52.66 +34:33:18.9 -- not an asteroid (will add it to exclusion list)
04:56:50.93 +34:40:36.5 -- not an asteroid (will add it to exclusion list)
04:56:48.30 +35:10:14.4 -- not an asteroid (will add it to exclusion list)
04:55:59.31 +34:32:40.2 -- not an asteroid (will add it to exclusion list)
04:56:08.90 +36:05:01.6 -- not an asteroid (will add it to exclusion list)
04:56:00.53 +36:01:23.1 -- not an asteroid (will add it to exclusion list)
04:59:39.38 +36:03:58.9 -- not an asteroid (will add it to exclusion list)
04:55:35.07 +36:01:42.8 -- not an asteroid (will add it to exclusion list)
04:58:27.65 +34:53:52.1 -- not an asteroid (will add it to exclusion list)
04:53:59.36 +36:13:31.3 -- not an asteroid (will add it to exclusion list)
04:59:30.66 +36:23:25.4 -- not an asteroid (will add it to exclusion list)
04:57:12.91 +34:32:01.4 -- not an asteroid (will add it to exclusion list)
04:58:36.02 +36:01:14.0 -- not an asteroid (will add it to exclusion list)
04:58:23.79 +34:50:58.5 -- not an asteroid (will add it to exclusion list)
04:55:43.97 +35:47:46.9 -- not an asteroid (will add it to exclusion list)
04:55:03.49 +34:43:30.6 -- not an asteroid (will add it to exclusion list)
04:57:20.42 +36:07:57.4 -- not an asteroid (will add it to exclusion list)
04:59:08.68 +35:56:45.7 -- not an asteroid (will add it to exclusion list)
04:57:56.28 +34:40:07.4 -- not an asteroid (will add it to exclusion list)
04:59:39.48 +36:48:51.1 -- not an asteroid (will add it to exclusion list)
04:58:11.05 +35:44:39.2 -- not an asteroid (will add it to exclusion list)
04:55:00.82 +35:49:28.9 -- not an asteroid (will add it to exclusion list)
04:56:34.51 +34:31:49.4 -- not an asteroid (will add it to exclusion list)
04:55:27.86 +34:49:38.2 -- not an asteroid (will add it to exclusion list)
04:56:09.32 +34:39:17.3 -- not an asteroid (will add it to exclusion list)
04:57:21.74 +34:50:09.4 -- not an asteroid (will add it to exclusion list)
04:55:44.12 +34:52:37.8 -- not an asteroid (will add it to exclusion list)
04:55:20.28 +34:27:58.8 -- not an asteroid (will add it to exclusion list)
04:59:30.11 +36:39:02.4 -- not an asteroid (will add it to exclusion list)
04:55:51.69 +35:35:59.8 -- not an asteroid (will add it to exclusion list)
04:54:51.25 +35:23:45.5 -- not an asteroid (will add it to exclusion list)
04:59:28.82 +35:49:28.8 -- not an asteroid (will add it to exclusion list)
04:59:46.18 +36:28:31.9 -- not an asteroid (will add it to exclusion list)
04:57:29.99 +33:51:53.0 -- not an asteroid (will add it to exclusion list)
04:55:01.84 +34:56:55.5 -- not an asteroid (will add it to exclusion list)
04:58:43.18 +34:55:20.4 -- not an asteroid (will add it to exclusion list)
04:55:43.15 +34:41:35.6 -- not an asteroid (will add it to exclusion list)
04:58:23.55 +35:36:55.0 -- not an asteroid (will add it to exclusion list)
04:57:06.75 +35:43:50.4 -- not an asteroid (will add it to exclusion list)
04:59:31.17 +36:40:42.8 -- not an asteroid (will add it to exclusion list)
04:57:55.69 +35:48:54.1 -- not an asteroid (will add it to exclusion list)
04:56:31.61 +35:29:59.0 -- not an asteroid (will add it to exclusion list)
04:54:49.37 +35:41:49.6 -- not an asteroid (will add it to exclusion list)
04:57:07.10 +35:53:26.4 -- not an asteroid (will add it to exclusion list)
04:58:06.38 +36:05:09.4 -- not an asteroid (will add it to exclusion list)
05:00:00.83 +36:39:09.2 -- not an asteroid (will add it to exclusion list)
04:56:52.51 +34:42:13.6 -- not an asteroid (will add it to exclusion list)
04:57:30.28 +35:36:07.8 -- not an asteroid (will add it to exclusion list)
04:58:18.55 +35:01:59.7 -- not an asteroid (will add it to exclusion list)
04:59:49.14 +36:27:55.8 -- not an asteroid (will add it to exclusion list)
04:58:35.68 +35:42:13.6 -- not an asteroid (will add it to exclusion list)
04:56:00.30 +34:40:38.1 -- not an asteroid (will add it to exclusion list)
04:59:45.63 +36:13:49.6 -- not an asteroid (will add it to exclusion list)
04:55:36.58 +34:54:06.6 -- not an asteroid (will add it to exclusion list)
04:58:38.90 +36:18:32.6 -- not an asteroid (will add it to exclusion list)
04:58:48.44 +35:59:26.7 -- not an asteroid (will add it to exclusion list)
04:59:56.53 +36:32:22.2 -- not an asteroid (will add it to exclusion list)
04:56:36.18 +34:14:49.7 -- not an asteroid (will add it to exclusion list)
04:56:25.77 +36:02:30.7 -- not an asteroid (will add it to exclusion list)
04:57:52.32 +34:40:22.1 -- not an asteroid (will add it to exclusion list)
04:55:10.41 +35:07:49.0 -- not an asteroid (will add it to exclusion list)
04:56:47.46 +34:20:59.5 -- not an asteroid (will add it to exclusion list)
04:55:11.47 +35:17:57.3 -- not an asteroid (will add it to exclusion list)
04:59:22.70 +36:14:15.1 -- not an asteroid (will add it to exclusion list)
04:58:48.76 +35:02:26.4 -- not an asteroid (will add it to exclusion list)
04:57:08.29 +34:48:33.7 -- not an asteroid (will add it to exclusion list)
04:55:39.53 +35:33:03.5 -- not an asteroid (will add it to exclusion list)
04:58:26.89 +36:05:19.3 -- not an asteroid (will add it to exclusion list)
04:54:52.60 +35:31:05.5 -- not an asteroid (will add it to exclusion list)
04:55:30.08 +35:45:57.8 -- not an asteroid (will add it to exclusion list)
04:54:13.04 +35:56:20.8 -- not an asteroid (will add it to exclusion list)
04:58:30.07 +35:54:10.0 -- not an asteroid (will add it to exclusion list)
04:56:34.68 +34:34:43.8 -- not an asteroid (will add it to exclusion list)
04:57:07.09 +34:38:12.1 -- not an asteroid (will add it to exclusion list)
04:59:37.46 +36:33:04.6 -- not an asteroid (will add it to exclusion list)
04:58:42.00 +36:00:43.4 -- not an asteroid (will add it to exclusion list)
04:57:46.58 +34:27:43.2 -- not an asteroid (will add it to exclusion list)
04:54:30.72 +35:46:11.8 -- not an asteroid (will add it to exclusion list)
04:54:37.32 +35:44:05.6 -- not an asteroid (will add it to exclusion list)
04:56:19.08 +34:57:43.7 -- not an asteroid (will add it to exclusion list)
04:55:09.86 +34:57:31.4 -- not an asteroid (will add it to exclusion list)
04:57:15.90 +35:06:34.4 -- not an asteroid (will add it to exclusion list)
04:56:39.34 +34:36:30.2 -- not an asteroid (will add it to exclusion list)
04:57:54.08 +33:58:12.0 -- not an asteroid (will add it to exclusion list)
04:57:10.51 +34:49:23.5 -- not an asteroid (will add it to exclusion list)
04:57:50.81 +33:51:47.6 -- not an asteroid (will add it to exclusion list)
04:56:49.87 +34:43:14.4 -- not an asteroid (will add it to exclusion list)
04:57:31.22 +33:55:16.2 -- not an asteroid (will add it to exclusion list)
04:57:16.08 +34:07:16.1 -- not an asteroid (will add it to exclusion list)
04:57:55.89 +35:59:50.2 -- not an asteroid (will add it to exclusion list)
04:55:32.90 +35:07:55.2 -- not an asteroid (will add it to exclusion list)
04:55:35.37 +34:28:01.8 -- not an asteroid (will add it to exclusion list)
04:55:27.00 +34:38:44.2 -- not an asteroid (will add it to exclusion list)
04:59:07.94 +36:20:51.9 -- not an asteroid (will add it to exclusion list)
04:55:10.34 +35:42:58.9 -- not an asteroid (will add it to exclusion list)
04:57:38.46 +34:53:57.8 -- not an asteroid (will add it to exclusion list)
04:58:06.24 +35:11:20.8 -- not an asteroid (will add it to exclusion list)
04:56:27.99 +35:18:57.9 -- not an asteroid (will add it to exclusion list)
04:59:05.05 +35:42:49.0 -- not an asteroid (will add it to exclusion list)
04:55:12.08 +35:35:10.4 -- not an asteroid (will add it to exclusion list)
04:57:18.50 +34:33:47.5 -- not an asteroid (will add it to exclusion list)
04:58:28.93 +34:53:04.8 -- not an asteroid (will add it to exclusion list)
04:59:21.24 +36:01:09.2 -- not an asteroid (will add it to exclusion list)
04:59:09.44 +35:50:49.1 -- not an asteroid (will add it to exclusion list)
04:54:00.64 +35:57:52.7 -- not an asteroid (will add it to exclusion list)
04:58:10.15 +34:13:47.0 -- not an asteroid (will add it to exclusion list)
04:58:49.38 +35:27:00.8 -- not an asteroid (will add it to exclusion list)
04:54:04.22 +35:48:39.6 -- not an asteroid (will add it to exclusion list)
04:55:33.75 +34:58:44.7 -- not an asteroid (will add it to exclusion list)
04:56:38.36 +34:38:28.4 -- not an asteroid (will add it to exclusion list)
04:57:08.10 +34:47:46.0 -- not an asteroid (will add it to exclusion list)
04:57:13.54 +34:52:29.0 -- not an asteroid (will add it to exclusion list)
04:58:36.01 +36:07:09.7 -- not an asteroid (will add it to exclusion list)
04:57:59.51 +35:52:27.6 -- not an asteroid (will add it to exclusion list)
04:57:45.79 +34:28:02.7 -- not an asteroid (will add it to exclusion list)
04:56:36.96 +35:36:36.6 -- not an asteroid (will add it to exclusion list)
04:58:52.58 +35:32:46.9 -- not an asteroid (will add it to exclusion list)
04:55:19.25 +35:34:22.5 -- not an asteroid (will add it to exclusion list)
04:56:00.39 +34:26:27.8 -- not an asteroid (will add it to exclusion list)
04:58:04.62 +35:46:23.9 -- not an asteroid (will add it to exclusion list)
04:58:55.59 +35:58:34.9 -- not an asteroid (will add it to exclusion list)
04:55:19.66 +35:26:33.7 -- not an asteroid (will add it to exclusion list)
04:56:36.85 +34:37:33.4 -- not an asteroid (will add it to exclusion list)
04:55:40.63 +35:36:40.5 -- not an asteroid (will add it to exclusion list)
04:58:36.85 +35:06:13.1 -- not an asteroid (will add it to exclusion list)
04:59:58.79 +36:49:24.1 -- not an asteroid (will add it to exclusion list)
04:58:41.28 +35:28:39.6 -- not an asteroid (will add it to exclusion list)
04:53:51.72 +35:56:38.2 -- not an asteroid (will add it to exclusion list)
04:57:34.14 +34:07:14.4 -- not an asteroid (will add it to exclusion list)
04:55:54.39 +34:34:17.7 -- not an asteroid (will add it to exclusion list)
04:59:46.38 +36:11:18.9 -- not an asteroid (will add it to exclusion list)
04:55:43.91 +35:28:49.5 -- not an asteroid (will add it to exclusion list)
04:54:46.79 +35:55:01.9 -- not an asteroid (will add it to exclusion list)
04:57:18.11 +34:50:37.6 -- not an asteroid (will add it to exclusion list)
04:59:41.14 +36:39:34.0 -- not an asteroid (will add it to exclusion list)
04:58:02.42 +33:58:36.8 -- not an asteroid (will add it to exclusion list)
04:56:39.49 +34:38:58.2 -- not an asteroid (will add it to exclusion list)
04:59:01.15 +35:40:04.6 -- not an asteroid (will add it to exclusion list)
04:58:35.08 +34:51:36.0 -- not an asteroid (will add it to exclusion list)
04:56:36.99 +36:02:52.3 -- not an asteroid (will add it to exclusion list)
04:54:35.18 +35:49:45.9 -- not an asteroid (will add it to exclusion list)
04:55:24.29 +35:22:43.0 -- not an asteroid (will add it to exclusion list)
04:54:36.91 +35:31:50.7 -- not an asteroid (will add it to exclusion list)
04:54:55.75 +35:07:55.2 -- not an asteroid (will add it to exclusion list)
04:55:19.62 +35:02:58.0 -- not an asteroid (will add it to exclusion list)
04:59:57.62 +36:45:31.5 -- not an asteroid (will add it to exclusion list)
04:58:41.68 +35:50:02.3 -- not an asteroid (will add it to exclusion list)
04:55:40.91 +34:30:10.4 -- not an asteroid (will add it to exclusion list)
04:56:15.01 +34:50:49.3 -- not an asteroid (will add it to exclusion list)
04:57:28.08 +35:51:45.0 -- not an asteroid (will add it to exclusion list)
04:59:31.44 +36:35:39.8 -- not an asteroid (will add it to exclusion list)
04:58:31.29 +36:18:32.2 -- not an asteroid (will add it to exclusion list)
04:58:41.26 +34:53:59.2 -- not an asteroid (will add it to exclusion list)
04:56:46.06 +34:16:33.7 -- not an asteroid (will add it to exclusion list)
04:58:00.39 +34:52:51.4 -- not an asteroid (will add it to exclusion list)
04:57:58.94 +36:13:02.9 -- not an asteroid (will add it to exclusion list)
04:58:51.51 +36:01:23.2 -- not an asteroid (will add it to exclusion list)
04:59:13.20 +35:54:16.3 -- not an asteroid (will add it to exclusion list)
04:56:45.91 +34:15:07.6 -- not an asteroid (will add it to exclusion list)
04:54:52.89 +35:40:11.5 -- not an asteroid (will add it to exclusion list)
04:58:21.94 +34:26:26.1 -- asteroid (will NOT add it to exclusion list)
04:56:50.77 +35:50:18.3 -- not an asteroid (will add it to exclusion list)
04:56:44.17 +34:39:21.3 -- not an asteroid (will add it to exclusion list)
04:55:10.48 +34:43:43.6 -- not an asteroid (will add it to exclusion list)
04:59:42.67 +36:26:04.0 -- not an asteroid (will add it to exclusion list)
04:58:13.85 +34:34:58.5 -- not an asteroid (will add it to exclusion list)
04:55:57.06 +35:00:06.9 -- not an asteroid (will add it to exclusion list)
04:59:07.74 +35:58:56.1 -- not an asteroid (will add it to exclusion list)
04:58:34.83 +34:52:58.4 -- not an asteroid (will add it to exclusion list)
04:56:46.52 +33:23:05.7 -- not an asteroid (will add it to exclusion list)
04:56:59.61 +34:28:47.8 -- not an asteroid (will add it to exclusion list)
04:59:51.47 +36:45:37.2 -- not an asteroid (will add it to exclusion list)
04:53:49.10 +35:26:42.2 -- not an asteroid (will add it to exclusion list)
04:58:47.09 +35:47:40.9 -- not an asteroid (will add it to exclusion list)
04:56:59.98 +34:13:07.7 -- not an asteroid (will add it to exclusion list)
04:56:22.74 +36:02:39.8 -- not an asteroid (will add it to exclusion list)
04:59:16.11 +35:41:23.0 -- not an asteroid (will add it to exclusion list)
04:57:48.25 +34:18:44.0 -- not an asteroid (will add it to exclusion list)
04:59:13.58 +35:50:02.2 -- not an asteroid (will add it to exclusion list)
04:54:09.02 +35:39:48.7 -- not an asteroid (will add it to exclusion list)
04:56:22.90 +34:54:46.8 -- not an asteroid (will add it to exclusion list)
04:55:05.07 +35:20:34.4 -- not an asteroid (will add it to exclusion list)
04:59:14.39 +36:12:09.7 -- not an asteroid (will add it to exclusion list)
04:54:23.69 +35:30:36.6 -- not an asteroid (will add it to exclusion list)
04:54:25.89 +35:48:20.8 -- not an asteroid (will add it to exclusion list)
04:58:38.49 +35:30:34.3 -- not an asteroid (will add it to exclusion list)
04:56:06.35 +35:12:24.2 -- not an asteroid (will add it to exclusion list)
04:54:33.72 +35:43:02.0 -- not an asteroid (will add it to exclusion list)
04:55:45.94 +35:21:31.0 -- not an asteroid (will add it to exclusion list)
04:55:45.27 +35:38:07.6 -- not an asteroid (will add it to exclusion list)
04:59:57.26 +36:48:09.3 -- not an asteroid (will add it to exclusion list)
04:58:12.43 +34:18:27.4 -- not an asteroid (will add it to exclusion list)
04:59:05.82 +35:49:46.8 -- not an asteroid (will add it to exclusion list)
04:56:42.84 +34:43:41.3 -- not an asteroid (will add it to exclusion list)
04:58:52.51 +35:50:15.2 -- not an asteroid (will add it to exclusion list)
04:59:31.01 +36:43:25.3 -- not an asteroid (will add it to exclusion list)
04:56:44.50 +34:40:03.7 -- not an asteroid (will add it to exclusion list)
04:56:33.27 +34:50:46.7 -- not an asteroid (will add it to exclusion list)
04:57:31.76 +34:31:51.0 -- not an asteroid (will add it to exclusion list)
04:58:03.95 +34:31:19.4 -- not an asteroid (will add it to exclusion list)
04:54:12.16 +35:39:33.6 -- not an asteroid (will add it to exclusion list)
04:57:24.04 +35:06:27.5 -- not an asteroid (will add it to exclusion list)
04:58:12.03 +36:04:51.6 -- not an asteroid (will add it to exclusion list)
04:57:03.17 +34:12:16.6 -- not an asteroid (will add it to exclusion list)
04:59:13.89 +36:17:30.8 -- not an asteroid (will add it to exclusion list)
04:57:05.50 +34:31:10.6 -- not an asteroid (will add it to exclusion list)
04:55:39.53 +35:29:44.2 -- not an asteroid (will add it to exclusion list)
04:59:44.38 +36:43:21.0 -- not an asteroid (will add it to exclusion list)
04:57:46.65 +35:41:59.3 -- not an asteroid (will add it to exclusion list)
04:58:22.94 +35:42:33.7 -- not an asteroid (will add it to exclusion list)
04:59:35.36 +36:12:54.4 -- not an asteroid (will add it to exclusion list)
04:59:20.58 +36:07:23.9 -- not an asteroid (will add it to exclusion list)
04:57:12.09 +34:38:24.6 -- not an asteroid (will add it to exclusion list)
04:56:30.86 +34:15:42.8 -- not an asteroid (will add it to exclusion list)
04:57:43.77 +34:22:45.1 -- not an asteroid (will add it to exclusion list)
04:58:15.65 +34:48:44.1 -- not an asteroid (will add it to exclusion list)
04:54:43.46 +35:19:47.5 -- not an asteroid (will add it to exclusion list)
04:54:41.92 +35:36:08.3 -- not an asteroid (will add it to exclusion list)
04:56:46.38 +35:45:30.6 -- not an asteroid (will add it to exclusion list)
04:57:05.84 +34:40:59.3 -- not an asteroid (will add it to exclusion list)
04:59:32.31 +36:05:05.4 -- not an asteroid (will add it to exclusion list)
04:57:15.18 +34:40:32.4 -- not an asteroid (will add it to exclusion list)
04:57:30.14 +35:06:36.5 -- not an asteroid (will add it to exclusion list)
04:58:35.64 +35:04:19.8 -- not an asteroid (will add it to exclusion list)
04:59:28.13 +35:54:04.1 -- not an asteroid (will add it to exclusion list)
04:53:46.43 +35:39:21.7 -- not an asteroid (will add it to exclusion list)
04:55:06.80 +35:27:13.8 -- not an asteroid (will add it to exclusion list)
04:57:34.38 +34:34:55.8 -- not an asteroid (will add it to exclusion list)
04:57:50.71 +36:07:24.9 -- not an asteroid (will add it to exclusion list)
04:59:20.57 +36:06:20.0 -- not an asteroid (will add it to exclusion list)
04:59:06.78 +35:44:46.4 -- not an asteroid (will add it to exclusion list)
04:59:46.13 +36:24:20.8 -- not an asteroid (will add it to exclusion list)
04:55:34.81 +34:51:24.4 -- not an asteroid (will add it to exclusion list)
04:57:43.34 +34:47:36.3 -- not an asteroid (will add it to exclusion list)
04:57:30.07 +33:28:54.9 -- not an asteroid (will add it to exclusion list)
04:57:42.03 +35:01:06.6 -- not an asteroid (will add it to exclusion list)
04:59:18.31 +36:31:03.5 -- not an asteroid (will add it to exclusion list)
04:55:20.74 +34:56:06.4 -- not an asteroid (will add it to exclusion list)
04:57:53.23 +34:09:17.3 -- not an asteroid (will add it to exclusion list)
04:57:35.39 +35:47:09.8 -- not an asteroid (will add it to exclusion list)
04:57:17.61 +34:43:50.7 -- not an asteroid (will add it to exclusion list)
04:57:29.75 +35:45:08.3 -- not an asteroid (will add it to exclusion list)
04:58:24.81 +35:40:53.4 -- not an asteroid (will add it to exclusion list)
04:57:32.91 +34:40:35.3 -- not an asteroid (will add it to exclusion list)
04:58:09.65 +35:59:09.5 -- not an asteroid (will add it to exclusion list)
04:59:55.05 +36:43:36.0 -- not an asteroid (will add it to exclusion list)
04:56:41.50 +35:03:22.8 -- not an asteroid (will add it to exclusion list)
04:58:48.76 +35:53:36.5 -- not an asteroid (will add it to exclusion list)
04:58:41.94 +35:56:13.9 -- not an asteroid (will add it to exclusion list)
04:58:05.29 +34:50:50.8 -- not an asteroid (will add it to exclusion list)
04:57:53.92 +35:54:26.8 -- not an asteroid (will add it to exclusion list)
04:57:59.16 +34:57:13.6 -- not an asteroid (will add it to exclusion list)
04:58:25.35 +35:05:03.1 -- not an asteroid (will add it to exclusion list)
04:53:58.43 +35:39:18.3 -- not an asteroid (will add it to exclusion list)
04:57:01.86 +34:15:03.6 -- not an asteroid (will add it to exclusion list)
04:59:21.45 +36:03:35.9 -- not an asteroid (will add it to exclusion list)
04:56:25.70 +35:11:37.0 -- not an asteroid (will add it to exclusion list)
04:55:46.37 +35:28:08.5 -- not an asteroid (will add it to exclusion list)
04:58:04.65 +36:03:52.7 -- not an asteroid (will add it to exclusion list)
04:57:54.53 +34:55:31.7 -- not an asteroid (will add it to exclusion list)
04:56:00.46 +35:37:56.2 -- not an asteroid (will add it to exclusion list)
04:58:12.45 +35:01:09.6 -- not an asteroid (will add it to exclusion list)
04:56:01.70 +35:32:16.7 -- not an asteroid (will add it to exclusion list)
04:55:50.80 +35:27:50.9 -- not an asteroid (will add it to exclusion list)
04:54:32.77 +35:55:15.5 -- not an asteroid (will add it to exclusion list)
04:55:08.13 +35:18:10.8 -- not an asteroid (will add it to exclusion list)
04:59:35.13 +36:30:25.6 -- not an asteroid (will add it to exclusion list)
04:59:15.21 +36:29:56.6 -- not an asteroid (will add it to exclusion list)
04:56:50.38 +34:54:16.3 -- not an asteroid (will add it to exclusion list)
04:58:53.10 +35:38:34.8 -- not an asteroid (will add it to exclusion list)
04:58:36.28 +35:02:35.6 -- not an asteroid (will add it to exclusion list)
04:54:45.24 +35:10:04.2 -- not an asteroid (will add it to exclusion list)
04:58:26.12 +36:10:02.4 -- not an asteroid (will add it to exclusion list)
04:57:34.34 +34:26:45.5 -- not an asteroid (will add it to exclusion list)
04:57:07.20 +34:32:54.8 -- not an asteroid (will add it to exclusion list)
04:54:57.53 +35:15:05.5 -- not an asteroid (will add it to exclusion list)
04:57:59.96 +35:58:33.2 -- not an asteroid (will add it to exclusion list)
04:56:22.74 +34:41:46.3 -- not an asteroid (will add it to exclusion list)
04:56:55.83 +34:45:46.0 -- not an asteroid (will add it to exclusion list)
04:58:26.66 +36:04:18.8 -- not an asteroid (will add it to exclusion list)
04:57:58.94 +33:53:26.0 -- not an asteroid (will add it to exclusion list)
04:55:48.47 +35:35:06.6 -- not an asteroid (will add it to exclusion list)
04:56:16.48 +34:47:05.1 -- not an asteroid (will add it to exclusion list)
04:58:44.79 +35:47:22.9 -- not an asteroid (will add it to exclusion list)
04:57:17.88 +34:56:19.3 -- not an asteroid (will add it to exclusion list)
04:55:54.19 +34:39:16.3 -- not an asteroid (will add it to exclusion list)
04:58:01.38 +34:19:30.6 -- not an asteroid (will add it to exclusion list)
04:57:17.39 +35:46:24.8 -- not an asteroid (will add it to exclusion list)
04:54:51.01 +35:49:18.9 -- not an asteroid (will add it to exclusion list)
04:59:10.94 +35:39:11.1 -- not an asteroid (will add it to exclusion list)
04:59:10.79 +35:33:35.7 -- not an asteroid (will add it to exclusion list)
04:57:46.97 +34:06:30.6 -- not an asteroid (will add it to exclusion list)
04:59:49.17 +36:17:23.7 -- not an asteroid (will add it to exclusion list)
04:58:07.87 +34:46:44.9 -- not an asteroid (will add it to exclusion list)
04:58:51.62 +35:36:38.1 -- not an asteroid (will add it to exclusion list)
04:56:03.80 +34:41:12.0 -- not an asteroid (will add it to exclusion list)
04:58:02.68 +34:18:39.4 -- not an asteroid (will add it to exclusion list)
04:56:28.11 +34:29:52.7 -- not an asteroid (will add it to exclusion list)
04:59:10.11 +35:30:11.3 -- not an asteroid (will add it to exclusion list)
04:59:24.25 +35:47:28.1 -- not an asteroid (will add it to exclusion list)
04:55:33.55 +35:04:37.6 -- not an asteroid (will add it to exclusion list)
04:56:29.26 +34:43:41.0 -- not an asteroid (will add it to exclusion list)
04:56:57.19 +34:40:37.0 -- not an asteroid (will add it to exclusion list)
04:58:56.28 +35:38:34.5 -- not an asteroid (will add it to exclusion list)
04:56:57.64 +34:45:37.5 -- not an asteroid (will add it to exclusion list)
04:55:25.15 +35:20:41.9 -- not an asteroid (will add it to exclusion list)
04:58:20.26 +34:19:17.1 -- not an asteroid (will add it to exclusion list)
04:59:08.12 +35:48:34.2 -- not an asteroid (will add it to exclusion list)
04:59:20.30 +36:04:48.7 -- not an asteroid (will add it to exclusion list)
04:58:14.24 +35:02:38.9 -- not an asteroid (will add it to exclusion list)
04:56:28.41 +35:07:17.7 -- not an asteroid (will add it to exclusion list)
04:56:35.72 +34:25:06.8 -- not an asteroid (will add it to exclusion list)
04:57:49.42 +34:50:18.2 -- not an asteroid (will add it to exclusion list)
04:56:43.88 +35:47:20.5 -- not an asteroid (will add it to exclusion list)
04:57:01.70 +34:52:25.2 -- not an asteroid (will add it to exclusion list)
04:55:13.47 +34:22:15.8 -- not an asteroid (will add it to exclusion list)
04:58:17.63 +35:48:36.9 -- not an asteroid (will add it to exclusion list)
04:57:40.64 +34:11:36.4 -- not an asteroid (will add it to exclusion list)
04:58:43.17 +36:14:43.8 -- not an asteroid (will add it to exclusion list)
04:57:34.95 +34:26:05.7 -- not an asteroid (will add it to exclusion list)
04:57:25.37 +36:05:47.2 -- not an asteroid (will add it to exclusion list)
04:58:19.56 +35:58:28.6 -- not an asteroid (will add it to exclusion list)
04:58:53.54 +35:27:58.5 -- not an asteroid (will add it to exclusion list)
04:56:43.07 +34:47:46.1 -- not an asteroid (will add it to exclusion list)
04:57:46.45 +34:10:12.4 -- not an asteroid (will add it to exclusion list)
04:56:21.50 +34:22:02.4 -- not an asteroid (will add it to exclusion list)
04:56:16.82 +35:02:58.3 -- not an asteroid (will add it to exclusion list)
04:57:54.76 +34:01:54.5 -- not an asteroid (will add it to exclusion list)
04:58:18.10 +36:10:23.3 -- not an asteroid (will add it to exclusion list)
04:55:13.19 +34:28:21.3 -- not an asteroid (will add it to exclusion list)
04:55:27.31 +35:42:06.6 -- not an asteroid (will add it to exclusion list)
04:57:43.42 +34:14:28.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:53:07.59 +35:48:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:35.12 +35:40:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:38.69 +35:55:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:46.43 +35:39:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:49.10 +35:26:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:51.72 +35:56:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:57.39 +35:32:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:58.43 +35:39:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:59.36 +36:13:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:00.64 +35:57:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:04.22 +35:48:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:06.61 +35:51:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:06.75 +35:13:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:09.02 +35:39:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:12.16 +35:39:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:13.04 +35:56:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:23.13 +35:55:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:23.69 +35:30:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:25.89 +35:48:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:30.72 +35:46:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:32.77 +35:55:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:33.72 +35:43:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:35.18 +35:49:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:36.91 +35:31:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:37.32 +35:44:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:41.92 +35:36:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:43.46 +35:19:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:45.24 +35:10:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:46.79 +35:55:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:46.89 +35:30:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:47.51 +35:13:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:48.66 +35:39:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:49.37 +35:41:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:51.01 +35:49:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:51.25 +35:23:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:52.60 +35:31:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:52.89 +35:40:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:55.75 +35:07:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:56.40 +34:53:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:57.53 +35:15:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:00.82 +35:49:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:00.96 +35:00:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:01.84 +34:56:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:03.48 +35:28:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:03.49 +34:43:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:05.07 +35:20:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:06.80 +35:27:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:08.13 +35:18:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:09.86 +34:57:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:10.12 +34:33:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:10.34 +35:42:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:10.41 +35:07:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:10.48 +34:43:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:11.47 +35:17:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:12.08 +35:35:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:13.19 +34:28:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:13.47 +34:22:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:19.25 +35:34:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:19.62 +35:02:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:19.66 +35:26:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:20.28 +34:27:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:20.74 +34:56:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:24.29 +35:22:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:25.15 +35:20:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:27.00 +34:38:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:27.31 +35:42:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:27.86 +34:49:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:28.70 +35:21:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:29.65 +35:39:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:30.08 +35:45:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:32.90 +35:07:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:33.55 +35:04:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:33.75 +34:58:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:34.81 +34:51:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:35.07 +36:01:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:35.37 +34:28:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:36.58 +34:54:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:37.36 +34:47:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:39.53 +35:29:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:39.53 +35:33:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:40.63 +35:36:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:40.91 +34:30:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:43.15 +34:41:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:43.91 +35:28:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:43.97 +35:47:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:44.12 +34:52:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:45.27 +35:38:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:45.94 +35:21:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:46.37 +35:28:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:48.47 +35:35:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:50.80 +35:27:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:51.69 +35:35:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:53.87 +34:56:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:54.19 +34:39:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:54.39 +34:34:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:57.06 +35:00:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:57.17 +34:25:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:59.31 +34:32:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:00.30 +34:40:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:00.39 +34:26:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:00.46 +35:37:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:00.53 +36:01:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:00.89 +35:05:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:01.70 +35:32:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:03.80 +34:41:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:06.35 +35:12:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:08.90 +36:05:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:09.32 +34:39:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:11.07 +34:22:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:15.01 +34:50:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:15.55 +34:41:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:16.48 +34:47:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:16.82 +35:02:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:19.08 +34:57:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:20.92 +36:00:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:21.50 +34:22:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:22.74 +34:41:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:22.74 +36:02:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:22.90 +34:54:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:25.70 +35:11:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:25.77 +36:02:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:26.04 +34:37:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:27.99 +35:18:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:28.11 +34:29:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:28.41 +35:07:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:29.26 +34:43:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:30.86 +34:15:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:31.07 +34:17:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:31.61 +35:29:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:32.93 +35:40:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:32.96 +34:57:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:33.27 +34:50:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:34.51 +34:31:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:34.68 +34:34:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:35.72 +34:25:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:36.18 +34:14:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:36.85 +34:37:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:36.96 +35:36:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:36.99 +36:02:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:38.36 +34:38:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:39.34 +34:36:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:39.45 +34:40:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:39.49 +34:38:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:41.50 +35:03:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:41.63 +34:38:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:41.97 +36:02:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:42.84 +34:43:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:43.07 +34:47:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:43.88 +35:47:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:44.17 +34:39:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:44.50 +34:40:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:45.91 +34:15:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:46.06 +34:16:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:46.38 +35:45:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:46.52 +33:23:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:47.46 +34:20:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:48.20 +34:47:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:48.30 +35:10:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:49.64 +34:58:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:49.87 +34:43:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:50.38 +34:54:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:50.77 +35:50:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:50.93 +34:40:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:52.51 +34:42:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:55.83 +34:45:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:57.19 +34:40:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:57.64 +34:45:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:59.61 +34:28:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:59.98 +34:13:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:01.70 +34:52:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:01.86 +34:15:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:03.17 +34:12:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:04.49 +34:46:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:05.50 +34:31:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:05.54 +36:01:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:05.84 +34:40:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:06.67 +34:24:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:06.75 +35:43:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:07.09 +34:38:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:07.10 +35:53:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:07.20 +34:32:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:08.10 +34:47:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:08.29 +34:48:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:10.51 +34:49:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:12.09 +34:36:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:12.09 +34:38:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:12.91 +34:32:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:13.54 +34:52:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:15.18 +34:40:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:15.52 +33:30:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:15.90 +35:06:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:16.08 +34:07:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:17.39 +35:46:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:17.61 +34:43:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:17.88 +34:56:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:18.11 +34:50:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:18.50 +34:33:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:18.59 +34:16:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:19.27 +35:40:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:20.42 +36:07:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:21.74 +34:50:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:22.48 +34:31:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:24.04 +35:06:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:25.37 +36:05:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:28.08 +35:51:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:29.75 +35:45:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:29.96 +34:29:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:29.99 +33:51:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:30.07 +33:28:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:30.14 +35:06:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:30.28 +35:36:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:31.22 +33:55:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:31.76 +34:31:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:32.91 +34:40:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:34.14 +34:07:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:34.34 +34:26:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:34.38 +34:34:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:34.69 +36:05:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:34.95 +34:26:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:35.39 +35:47:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:38.46 +34:53:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:40.64 +34:11:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:42.03 +35:01:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:43.34 +34:47:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:43.42 +34:14:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:43.77 +34:22:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:45.33 +34:48:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:45.79 +34:28:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:45.98 +34:01:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:46.02 +33:33:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:46.45 +34:10:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:46.58 +34:27:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:46.65 +35:41:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:46.97 +34:06:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:48.25 +34:18:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:49.20 +34:05:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:49.42 +34:50:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:50.71 +36:07:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:50.81 +33:51:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:52.32 +34:40:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:52.38 +34:17:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:52.66 +34:33:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:53.23 +34:09:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:53.36 +35:00:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:53.92 +35:54:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:54.08 +33:58:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:54.53 +34:55:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:54.76 +34:01:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:55.69 +35:48:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:55.89 +35:59:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:56.28 +34:40:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:58.76 +34:32:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:58.94 +33:53:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:58.94 +36:13:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:59.16 +34:57:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:59.51 +35:52:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:59.96 +35:58:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:00.39 +34:52:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:01.38 +34:19:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:01.44 +34:22:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:01.58 +35:00:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:02.42 +33:58:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:02.68 +34:18:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:03.17 +34:04:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:03.19 +35:57:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:03.95 +34:31:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:04.62 +35:46:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:04.65 +36:03:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:04.74 +35:44:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:05.29 +34:50:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:06.24 +35:11:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:06.38 +36:05:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:07.35 +35:57:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:07.87 +34:46:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:08.36 +35:53:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:09.65 +35:59:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:10.15 +34:13:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:10.21 +35:05:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:11.05 +35:44:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:12.03 +36:04:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:12.18 +34:08:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:12.43 +34:18:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:12.45 +35:01:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:13.23 +34:27:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:13.85 +34:34:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:14.24 +35:02:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:15.65 +34:48:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:17.10 +35:42:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:17.59 +35:59:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:17.63 +35:48:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:18.10 +36:10:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:18.55 +35:01:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:19.56 +35:58:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:20.26 +34:19:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:20.82 +35:32:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:22.94 +35:42:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:23.55 +35:36:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:23.79 +34:50:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:24.81 +35:40:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:25.35 +35:05:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:26.12 +36:10:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:26.58 +35:56:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:26.66 +36:04:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:26.89 +36:05:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:27.65 +34:53:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:28.93 +34:53:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:29.87 +35:43:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:30.07 +35:54:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:31.29 +36:18:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:32.07 +35:00:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:34.50 +35:00:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:34.83 +34:52:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:35.08 +34:51:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:35.64 +35:04:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:35.68 +35:42:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:36.01 +36:07:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:36.02 +36:01:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:36.28 +35:02:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:36.85 +35:06:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:37.61 +34:55:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:37.99 +36:03:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:38.49 +35:30:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:38.72 +34:53:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:38.90 +36:18:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:40.35 +34:54:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:40.91 +35:31:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:41.26 +34:53:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:41.28 +35:28:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:41.44 +35:58:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:41.68 +35:50:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:41.94 +35:56:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:42.00 +36:00:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:43.17 +36:14:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:43.18 +34:55:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:44.55 +35:38:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:44.79 +35:47:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:46.97 +36:01:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:47.09 +35:47:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:48.20 +35:37:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:48.44 +35:59:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:48.76 +35:02:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:48.76 +35:53:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:49.38 +35:27:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:49.84 +36:07:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:51.51 +36:01:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:51.62 +35:36:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:52.51 +35:50:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:52.58 +35:32:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:53.10 +35:38:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:53.54 +35:27:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:54.48 +35:09:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:55.59 +35:58:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:55.62 +35:39:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:56.05 +35:05:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:56.28 +35:38:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:57.30 +35:34:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:58.72 +36:01:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:01.15 +35:40:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:05.05 +35:42:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:05.82 +35:49:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:06.07 +36:04:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:06.78 +35:44:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:07.74 +35:58:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:07.94 +36:20:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:08.12 +35:48:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:08.68 +35:56:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:09.44 +35:50:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:10.11 +35:30:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:10.79 +35:33:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:10.94 +35:39:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:13.20 +35:54:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:13.58 +35:50:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:13.89 +36:17:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:14.39 +36:12:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:15.21 +36:29:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:15.41 +36:42:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:16.11 +35:41:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:16.83 +36:02:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:18.31 +36:31:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:20.30 +36:04:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:20.50 +36:02:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:20.57 +36:06:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:20.58 +36:07:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:21.24 +36:01:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:21.45 +36:03:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:22.70 +36:14:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:23.87 +36:14:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:24.25 +35:47:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:24.43 +36:06:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:26.11 +36:32:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:28.13 +35:54:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:28.28 +36:27:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:28.82 +35:49:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:29.06 +35:55:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:30.11 +36:39:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:30.66 +36:23:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:31.01 +36:43:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:31.17 +36:40:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:31.44 +36:35:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:32.31 +36:05:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:34.00 +36:43:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:35.13 +36:30:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:35.36 +36:12:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:37.46 +36:33:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:39.38 +36:03:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:39.48 +36:48:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:41.14 +36:39:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:41.99 +36:09:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:42.67 +36:26:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:44.38 +36:43:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:45.63 +36:13:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:46.05 +36:36:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:46.13 +36:24:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:46.18 +36:28:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:46.38 +36:11:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:49.14 +36:27:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:49.17 +36:17:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:51.47 +36:45:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:55.05 +36:43:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:55.75 +36:34:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:56.53 +36:32:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:57.26 +36:48:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:57.62 +36:45:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:57.92 +36:30:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:58.79 +36:49:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:00.55 +36:34:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:00.83 +36:39:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:03.85 +36:50:48.8 -- 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)
04:53:07.59 +35:48:44.0 -- not a known variable star
04:53:35.12 +35:40:33.1 -- not a known variable star
04:53:38.69 +35:55:19.6 -- not a known variable star
04:53:46.43 +35:39:21.7 -- not a known variable star
04:53:49.10 +35:26:42.2 -- not a known variable star
04:53:51.72 +35:56:38.2 -- not a known variable star
04:53:57.39 +35:32:17.9 -- not a known variable star
04:53:58.43 +35:39:18.3 -- not a known variable star
04:53:59.36 +36:13:31.3 -- not a known variable star
04:54:00.64 +35:57:52.7 -- not a known variable star
04:54:04.22 +35:48:39.6 -- not a known variable star
04:54:06.61 +35:51:03.9 -- not a known variable star
04:54:06.75 +35:13:44.2 -- not a known variable star
04:54:09.02 +35:39:48.7 -- not a known variable star
04:54:12.16 +35:39:33.6 -- not a known variable star
04:54:13.04 +35:56:20.8 -- not a known variable star
04:54:23.13 +35:55:04.1 -- not a known variable star
04:54:23.69 +35:30:36.6 -- not a known variable star
04:54:25.89 +35:48:20.8 -- not a known variable star
04:54:30.72 +35:46:11.8 -- not a known variable star
04:54:32.77 +35:55:15.5 -- not a known variable star
04:54:33.72 +35:43:02.0 -- not a known variable star
04:54:35.18 +35:49:45.9 -- not a known variable star
04:54:36.91 +35:31:50.7 -- not a known variable star
04:54:37.32 +35:44:05.6 -- not a known variable star
04:54:41.92 +35:36:08.3 -- not a known variable star
04:54:43.46 +35:19:47.5 -- not a known variable star
04:54:45.24 +35:10:04.2 -- not a known variable star
04:54:46.79 +35:55:01.9 -- not a known variable star
04:54:46.89 +35:30:30.4 -- not a known variable star
04:54:47.51 +35:13:42.7 -- not a known variable star
04:54:48.66 +35:39:42.8 -- not a known variable star
04:54:49.37 +35:41:49.6 -- not a known variable star
04:54:51.01 +35:49:18.9 -- not a known variable star
04:54:51.25 +35:23:45.5 -- not a known variable star
04:54:52.60 +35:31:05.5 -- not a known variable star
04:54:52.89 +35:40:11.5 -- not a known variable star
04:54:55.75 +35:07:55.2 -- not a known variable star
04:54:56.40 +34:53:50.2 -- not a known variable star
04:54:57.53 +35:15:05.5 -- not a known variable star
04:55:00.82 +35:49:28.9 -- not a known variable star
04:55:00.96 +35:00:48.9 -- a known variable star
04:55:01.84 +34:56:55.5 -- not a known variable star
04:55:03.48 +35:28:38.7 -- not a known variable star
04:55:03.49 +34:43:30.6 -- not a known variable star
04:55:05.07 +35:20:34.4 -- not a known variable star
04:55:06.80 +35:27:13.8 -- not a known variable star
04:55:08.13 +35:18:10.8 -- not a known variable star
04:55:09.86 +34:57:31.4 -- not a known variable star
04:55:10.12 +34:33:20.7 -- not a known variable star
04:55:10.34 +35:42:58.9 -- not a known variable star
04:55:10.41 +35:07:49.0 -- not a known variable star
04:55:10.48 +34:43:43.6 -- not a known variable star
04:55:11.47 +35:17:57.3 -- not a known variable star
04:55:12.08 +35:35:10.4 -- not a known variable star
04:55:13.19 +34:28:21.3 -- not a known variable star
04:55:13.47 +34:22:15.8 -- not a known variable star
04:55:19.25 +35:34:22.5 -- not a known variable star
04:55:19.62 +35:02:58.0 -- not a known variable star
04:55:19.66 +35:26:33.7 -- not a known variable star
04:55:20.28 +34:27:58.8 -- not a known variable star
04:55:20.74 +34:56:06.4 -- not a known variable star
04:55:24.29 +35:22:43.0 -- a known variable star
04:55:25.15 +35:20:41.9 -- not a known variable star
04:55:27.00 +34:38:44.2 -- not a known variable star
04:55:27.31 +35:42:06.6 -- not a known variable star
04:55:27.86 +34:49:38.2 -- not a known variable star
04:55:28.70 +35:21:46.5 -- not a known variable star
04:55:29.65 +35:39:50.3 -- not a known variable star
04:55:30.08 +35:45:57.8 -- not a known variable star
04:55:32.90 +35:07:55.2 -- not a known variable star
04:55:33.55 +35:04:37.6 -- a known variable star
04:55:33.75 +34:58:44.7 -- not a known variable star
04:55:34.81 +34:51:24.4 -- a known variable star
04:55:35.07 +36:01:42.8 -- not a known variable star
04:55:35.37 +34:28:01.8 -- not a known variable star
04:55:36.58 +34:54:06.6 -- not a known variable star
04:55:37.36 +34:47:51.6 -- not a known variable star
04:55:39.53 +35:29:44.2 -- a known variable star
04:55:39.53 +35:33:03.5 -- not a known variable star
04:55:40.63 +35:36:40.5 -- not a known variable star
04:55:40.91 +34:30:10.4 -- not a known variable star
04:55:43.15 +34:41:35.6 -- not a known variable star
04:55:43.91 +35:28:49.5 -- not a known variable star
04:55:43.97 +35:47:46.9 -- not a known variable star
04:55:44.12 +34:52:37.8 -- not a known variable star
04:55:45.27 +35:38:07.6 -- not a known variable star
04:55:45.94 +35:21:31.0 -- not a known variable star
04:55:46.37 +35:28:08.5 -- not a known variable star
04:55:48.47 +35:35:06.6 -- not a known variable star
04:55:50.80 +35:27:50.9 -- not a known variable star
04:55:51.69 +35:35:59.8 -- not a known variable star
04:55:53.87 +34:56:42.3 -- not a known variable star
04:55:54.19 +34:39:16.3 -- not a known variable star
04:55:54.39 +34:34:17.7 -- a known variable star
04:55:57.06 +35:00:06.9 -- not a known variable star
04:55:57.17 +34:25:54.0 -- not a known variable star
04:55:59.31 +34:32:40.2 -- not a known variable star
04:56:00.30 +34:40:38.1 -- not a known variable star
04:56:00.39 +34:26:27.8 -- not a known variable star
04:56:00.46 +35:37:56.2 -- not a known variable star
04:56:00.53 +36:01:23.1 -- not a known variable star
04:56:00.89 +35:05:59.7 -- not a known variable star
04:56:01.70 +35:32:16.7 -- not a known variable star
04:56:03.80 +34:41:12.0 -- a known variable star
04:56:06.35 +35:12:24.2 -- not a known variable star
04:56:08.90 +36:05:01.6 -- not a known variable star
04:56:09.32 +34:39:17.3 -- not a known variable star
04:56:11.07 +34:22:11.3 -- not a known variable star
04:56:15.01 +34:50:49.3 -- not a known variable star
04:56:15.55 +34:41:28.6 -- not a known variable star
04:56:16.48 +34:47:05.1 -- not a known variable star
04:56:16.82 +35:02:58.3 -- not a known variable star
04:56:19.08 +34:57:43.7 -- not a known variable star
04:56:20.92 +36:00:20.6 -- not a known variable star
04:56:21.50 +34:22:02.4 -- not a known variable star
04:56:22.74 +34:41:46.3 -- not a known variable star
04:56:22.74 +36:02:39.8 -- not a known variable star
04:56:22.90 +34:54:46.8 -- not a known variable star
04:56:25.70 +35:11:37.0 -- not a known variable star
04:56:25.77 +36:02:30.7 -- not a known variable star
04:56:26.04 +34:37:19.7 -- not a known variable star
04:56:27.99 +35:18:57.9 -- not a known variable star
04:56:28.11 +34:29:52.7 -- not a known variable star
04:56:28.41 +35:07:17.7 -- not a known variable star
04:56:29.26 +34:43:41.0 -- not a known variable star
04:56:30.86 +34:15:42.8 -- not a known variable star
04:56:31.07 +34:17:26.7 -- not a known variable star
04:56:31.61 +35:29:59.0 -- not a known variable star
04:56:32.93 +35:40:53.4 -- not a known variable star
04:56:32.96 +34:57:09.3 -- not a known variable star
04:56:33.27 +34:50:46.7 -- not a known variable star
04:56:34.51 +34:31:49.4 -- not a known variable star
04:56:34.68 +34:34:43.8 -- not a known variable star
04:56:35.72 +34:25:06.8 -- not a known variable star
04:56:36.18 +34:14:49.7 -- not a known variable star
04:56:36.85 +34:37:33.4 -- not a known variable star
04:56:36.96 +35:36:36.6 -- not a known variable star
04:56:36.99 +36:02:52.3 -- not a known variable star
04:56:38.36 +34:38:28.4 -- not a known variable star
04:56:39.34 +34:36:30.2 -- not a known variable star
04:56:39.45 +34:40:25.2 -- not a known variable star
04:56:39.49 +34:38:58.2 -- not a known variable star
04:56:41.50 +35:03:22.8 -- not a known variable star
04:56:41.63 +34:38:39.5 -- not a known variable star
04:56:41.97 +36:02:13.9 -- not a known variable star
04:56:42.84 +34:43:41.3 -- not a known variable star
04:56:43.07 +34:47:46.1 -- not a known variable star
04:56:43.88 +35:47:20.5 -- not a known variable star
04:56:44.17 +34:39:21.3 -- not a known variable star
04:56:44.50 +34:40:03.7 -- not a known variable star
04:56:45.91 +34:15:07.6 -- not a known variable star
04:56:46.06 +34:16:33.7 -- not a known variable star
04:56:46.38 +35:45:30.6 -- a known variable star
04:56:46.52 +33:23:05.7 -- not a known variable star
04:56:47.46 +34:20:59.5 -- not a known variable star
04:56:48.20 +34:47:38.9 -- not a known variable star
04:56:48.30 +35:10:14.4 -- not a known variable star
04:56:49.64 +34:58:30.4 -- not a known variable star
04:56:49.87 +34:43:14.4 -- not a known variable star
04:56:50.38 +34:54:16.3 -- not a known variable star
04:56:50.77 +35:50:18.3 -- a known variable star
04:56:50.93 +34:40:36.5 -- not a known variable star
04:56:52.51 +34:42:13.6 -- not a known variable star
04:56:55.83 +34:45:46.0 -- not a known variable star
04:56:57.19 +34:40:37.0 -- not a known variable star
04:56:57.64 +34:45:37.5 -- not a known variable star
04:56:59.61 +34:28:47.8 -- not a known variable star
04:56:59.98 +34:13:07.7 -- a known variable star
04:57:01.70 +34:52:25.2 -- not a known variable star
04:57:01.86 +34:15:03.6 -- not a known variable star
04:57:03.17 +34:12:16.6 -- not a known variable star
04:57:04.49 +34:46:04.7 -- not a known variable star
04:57:05.50 +34:31:10.6 -- not a known variable star
04:57:05.54 +36:01:50.9 -- not a known variable star
04:57:05.84 +34:40:59.3 -- not a known variable star
04:57:06.67 +34:24:03.2 -- not a known variable star
04:57:06.75 +35:43:50.4 -- not a known variable star
04:57:07.09 +34:38:12.1 -- not a known variable star
04:57:07.10 +35:53:26.4 -- not a known variable star
04:57:07.20 +34:32:54.8 -- not a known variable star
04:57:08.10 +34:47:46.0 -- not a known variable star
04:57:08.29 +34:48:33.7 -- not a known variable star
04:57:10.51 +34:49:23.5 -- not a known variable star
04:57:12.09 +34:36:17.8 -- not a known variable star
04:57:12.09 +34:38:24.6 -- not a known variable star
04:57:12.91 +34:32:01.4 -- not a known variable star
04:57:13.54 +34:52:29.0 -- not a known variable star
04:57:15.18 +34:40:32.4 -- not a known variable star
04:57:15.52 +33:30:19.1 -- a known variable star
04:57:15.90 +35:06:34.4 -- not a known variable star
04:57:16.08 +34:07:16.1 -- not a known variable star
04:57:17.39 +35:46:24.8 -- a known variable star
04:57:17.61 +34:43:50.7 -- not a known variable star
04:57:17.88 +34:56:19.3 -- not a known variable star
04:57:18.11 +34:50:37.6 -- not a known variable star
04:57:18.50 +34:33:47.5 -- not a known variable star
04:57:18.59 +34:16:18.5 -- a known variable star
04:57:19.27 +35:40:25.1 -- not a known variable star
04:57:20.42 +36:07:57.4 -- not a known variable star
04:57:21.74 +34:50:09.4 -- not a known variable star
04:57:22.48 +34:31:57.0 -- not a known variable star
04:57:24.04 +35:06:27.5 -- not a known variable star
04:57:25.37 +36:05:47.2 -- not a known variable star
04:57:28.08 +35:51:45.0 -- not a known variable star
04:57:29.75 +35:45:08.3 -- a known variable star
04:57:29.96 +34:29:10.1 -- not a known variable star
04:57:29.99 +33:51:53.0 -- not a known variable star
04:57:30.07 +33:28:54.9 -- a known variable star
04:57:30.14 +35:06:36.5 -- not a known variable star
04:57:30.28 +35:36:07.8 -- not a known variable star
04:57:31.22 +33:55:16.2 -- not a known variable star
04:57:31.76 +34:31:51.0 -- not a known variable star
04:57:32.91 +34:40:35.3 -- not a known variable star
04:57:34.14 +34:07:14.4 -- not a known variable star
04:57:34.34 +34:26:45.5 -- not a known variable star
04:57:34.38 +34:34:55.8 -- not a known variable star
04:57:34.69 +36:05:34.4 -- not a known variable star
04:57:34.95 +34:26:05.7 -- not a known variable star
04:57:35.39 +35:47:09.8 -- not a known variable star
04:57:38.46 +34:53:57.8 -- not a known variable star
04:57:40.64 +34:11:36.4 -- not a known variable star
04:57:42.03 +35:01:06.6 -- not a known variable star
04:57:43.34 +34:47:36.3 -- not a known variable star
04:57:43.42 +34:14:28.1 -- not a known variable star
04:57:43.77 +34:22:45.1 -- not a known variable star
04:57:45.33 +34:48:49.7 -- not a known variable star
04:57:45.79 +34:28:02.7 -- not a known variable star
04:57:45.98 +34:01:46.9 -- not a known variable star
04:57:46.02 +33:33:36.5 -- not a known variable star
04:57:46.45 +34:10:12.4 -- not a known variable star
04:57:46.58 +34:27:43.2 -- not a known variable star
04:57:46.65 +35:41:59.3 -- not a known variable star
04:57:46.97 +34:06:30.6 -- not a known variable star
04:57:48.25 +34:18:44.0 -- a known variable star
04:57:49.20 +34:05:02.5 -- not a known variable star
04:57:49.42 +34:50:18.2 -- not a known variable star
04:57:50.71 +36:07:24.9 -- a known variable star
04:57:50.81 +33:51:47.6 -- not a known variable star
04:57:52.32 +34:40:22.1 -- not a known variable star
04:57:52.38 +34:17:23.0 -- not a known variable star
04:57:52.66 +34:33:18.9 -- not a known variable star
04:57:53.23 +34:09:17.3 -- not a known variable star
04:57:53.36 +35:00:42.0 -- not a known variable star
04:57:53.92 +35:54:26.8 -- not a known variable star
04:57:54.08 +33:58:12.0 -- not a known variable star
04:57:54.53 +34:55:31.7 -- not a known variable star
04:57:54.76 +34:01:54.5 -- not a known variable star
04:57:55.69 +35:48:54.1 -- not a known variable star
04:57:55.89 +35:59:50.2 -- not a known variable star
04:57:56.28 +34:40:07.4 -- not a known variable star
04:57:58.76 +34:32:19.6 -- not a known variable star
04:57:58.94 +33:53:26.0 -- a known variable star
04:57:58.94 +36:13:02.9 -- not a known variable star
04:57:59.16 +34:57:13.6 -- a known variable star
04:57:59.51 +35:52:27.6 -- not a known variable star
04:57:59.96 +35:58:33.2 -- not a known variable star
04:58:00.39 +34:52:51.4 -- not a known variable star
04:58:01.38 +34:19:30.6 -- a known variable star
04:58:01.44 +34:22:45.0 -- not a known variable star
04:58:01.58 +35:00:44.2 -- not a known variable star
04:58:02.42 +33:58:36.8 -- not a known variable star
04:58:02.68 +34:18:39.4 -- not a known variable star
04:58:03.17 +34:04:34.7 -- not a known variable star
04:58:03.19 +35:57:57.9 -- not a known variable star
04:58:03.95 +34:31:19.4 -- a known variable star
04:58:04.62 +35:46:23.9 -- not a known variable star
04:58:04.65 +36:03:52.7 -- not a known variable star
04:58:04.74 +35:44:00.0 -- not a known variable star
04:58:05.29 +34:50:50.8 -- not a known variable star
04:58:06.24 +35:11:20.8 -- not a known variable star
04:58:06.38 +36:05:09.4 -- not a known variable star
04:58:07.35 +35:57:00.8 -- not a known variable star
04:58:07.87 +34:46:44.9 -- not a known variable star
04:58:08.36 +35:53:38.0 -- not a known variable star
04:58:09.65 +35:59:09.5 -- not a known variable star
04:58:10.15 +34:13:47.0 -- not a known variable star
04:58:10.21 +35:05:57.4 -- not a known variable star
04:58:11.05 +35:44:39.2 -- not a known variable star
04:58:12.03 +36:04:51.6 -- not a known variable star
04:58:12.18 +34:08:43.8 -- not a known variable star
04:58:12.43 +34:18:27.4 -- not a known variable star
04:58:12.45 +35:01:09.6 -- not a known variable star
04:58:13.23 +34:27:21.1 -- not a known variable star
04:58:13.85 +34:34:58.5 -- not a known variable star
04:58:14.24 +35:02:38.9 -- not a known variable star
04:58:15.65 +34:48:44.1 -- not a known variable star
04:58:17.10 +35:42:22.3 -- not a known variable star
04:58:17.59 +35:59:57.3 -- a known variable star
04:58:17.63 +35:48:36.9 -- not a known variable star
04:58:18.10 +36:10:23.3 -- not a known variable star
04:58:18.55 +35:01:59.7 -- not a known variable star
04:58:19.56 +35:58:28.6 -- not a known variable star
04:58:20.26 +34:19:17.1 -- not a known variable star
04:58:20.82 +35:32:50.8 -- not a known variable star
04:58:22.94 +35:42:33.7 -- not a known variable star
04:58:23.55 +35:36:55.0 -- not a known variable star
04:58:23.79 +34:50:58.5 -- not a known variable star
04:58:24.81 +35:40:53.4 -- not a known variable star
04:58:25.35 +35:05:03.1 -- not a known variable star
04:58:26.12 +36:10:02.4 -- not a known variable star
04:58:26.58 +35:56:58.5 -- not a known variable star
04:58:26.66 +36:04:18.8 -- not a known variable star
04:58:26.89 +36:05:19.3 -- not a known variable star
04:58:27.65 +34:53:52.1 -- not a known variable star
04:58:28.93 +34:53:04.8 -- not a known variable star
04:58:29.87 +35:43:51.1 -- not a known variable star
04:58:30.07 +35:54:10.0 -- not a known variable star
04:58:31.29 +36:18:32.2 -- not a known variable star
04:58:32.07 +35:00:45.8 -- not a known variable star
04:58:34.50 +35:00:37.5 -- not a known variable star
04:58:34.83 +34:52:58.4 -- not a known variable star
04:58:35.08 +34:51:36.0 -- not a known variable star
04:58:35.64 +35:04:19.8 -- not a known variable star
04:58:35.68 +35:42:13.6 -- not a known variable star
04:58:36.01 +36:07:09.7 -- not a known variable star
04:58:36.02 +36:01:14.0 -- not a known variable star
04:58:36.28 +35:02:35.6 -- a known variable star
04:58:36.85 +35:06:13.1 -- not a known variable star
04:58:37.61 +34:55:40.6 -- not a known variable star
04:58:37.99 +36:03:35.2 -- not a known variable star
04:58:38.49 +35:30:34.3 -- not a known variable star
04:58:38.72 +34:53:44.6 -- not a known variable star
04:58:38.90 +36:18:32.6 -- not a known variable star
04:58:40.35 +34:54:34.0 -- not a known variable star
04:58:40.91 +35:31:39.2 -- a known variable star
04:58:41.26 +34:53:59.2 -- not a known variable star
04:58:41.28 +35:28:39.6 -- not a known variable star
04:58:41.44 +35:58:36.6 -- not a known variable star
04:58:41.68 +35:50:02.3 -- not a known variable star
04:58:41.94 +35:56:13.9 -- a known variable star
04:58:42.00 +36:00:43.4 -- not a known variable star
04:58:43.17 +36:14:43.8 -- not a known variable star
04:58:43.18 +34:55:20.4 -- not a known variable star
04:58:44.55 +35:38:54.9 -- not a known variable star
04:58:44.79 +35:47:22.9 -- not a known variable star
04:58:46.97 +36:01:10.5 -- a known variable star
04:58:47.09 +35:47:40.9 -- a known variable star
04:58:48.20 +35:37:06.4 -- not a known variable star
04:58:48.44 +35:59:26.7 -- not a known variable star
04:58:48.76 +35:02:26.4 -- not a known variable star
04:58:48.76 +35:53:36.5 -- not a known variable star
04:58:49.38 +35:27:00.8 -- not a known variable star
04:58:49.84 +36:07:08.1 -- not a known variable star
04:58:51.51 +36:01:23.2 -- a known variable star
04:58:51.62 +35:36:38.1 -- not a known variable star
04:58:52.51 +35:50:15.2 -- not a known variable star
04:58:52.58 +35:32:46.9 -- not a known variable star
04:58:53.10 +35:38:34.8 -- not a known variable star
04:58:53.54 +35:27:58.5 -- not a known variable star
04:58:54.48 +35:09:37.5 -- not a known variable star
04:58:55.59 +35:58:34.9 -- not a known variable star
04:58:55.62 +35:39:57.6 -- not a known variable star
04:58:56.05 +35:05:23.5 -- not a known variable star
04:58:56.28 +35:38:34.5 -- not a known variable star
04:58:57.30 +35:34:06.9 -- a known variable star
04:58:58.72 +36:01:58.3 -- a known variable star
04:59:01.15 +35:40:04.6 -- not a known variable star
04:59:05.05 +35:42:49.0 -- not a known variable star
04:59:05.82 +35:49:46.8 -- a known variable star
04:59:06.07 +36:04:21.6 -- not a known variable star
04:59:06.78 +35:44:46.4 -- not a known variable star
04:59:07.74 +35:58:56.1 -- a known variable star
04:59:07.94 +36:20:51.9 -- not a known variable star
04:59:08.12 +35:48:34.2 -- not a known variable star
04:59:08.68 +35:56:45.7 -- not a known variable star
04:59:09.44 +35:50:49.1 -- not a known variable star
04:59:10.11 +35:30:11.3 -- not a known variable star
04:59:10.79 +35:33:35.7 -- not a known variable star
04:59:10.94 +35:39:11.1 -- not a known variable star
04:59:13.20 +35:54:16.3 -- not a known variable star
04:59:13.58 +35:50:02.2 -- not a known variable star
04:59:13.89 +36:17:30.8 -- not a known variable star
04:59:14.39 +36:12:09.7 -- not a known variable star
04:59:15.21 +36:29:56.6 -- not a known variable star
04:59:15.41 +36:42:37.9 -- not a known variable star
04:59:16.11 +35:41:23.0 -- not a known variable star
04:59:16.83 +36:02:12.4 -- not a known variable star
04:59:18.31 +36:31:03.5 -- not a known variable star
04:59:20.30 +36:04:48.7 -- not a known variable star
04:59:20.50 +36:02:23.8 -- not a known variable star
04:59:20.57 +36:06:20.0 -- not a known variable star
04:59:20.58 +36:07:23.9 -- a known variable star
04:59:21.24 +36:01:09.2 -- not a known variable star
04:59:21.45 +36:03:35.9 -- not a known variable star
04:59:22.70 +36:14:15.1 -- not a known variable star
04:59:23.87 +36:14:56.5 -- not a known variable star
04:59:24.25 +35:47:28.1 -- not a known variable star
04:59:24.43 +36:06:11.1 -- not a known variable star
04:59:26.11 +36:32:16.1 -- not a known variable star
04:59:28.13 +35:54:04.1 -- not a known variable star
04:59:28.28 +36:27:44.1 -- not a known variable star
04:59:28.82 +35:49:28.8 -- not a known variable star
04:59:29.06 +35:55:19.3 -- not a known variable star
04:59:30.11 +36:39:02.4 -- not a known variable star
04:59:30.66 +36:23:25.4 -- not a known variable star
04:59:31.01 +36:43:25.3 -- not a known variable star
04:59:31.17 +36:40:42.8 -- not a known variable star
04:59:31.44 +36:35:39.8 -- not a known variable star
04:59:32.31 +36:05:05.4 -- not a known variable star
04:59:34.00 +36:43:33.1 -- a known variable star
04:59:35.13 +36:30:25.6 -- not a known variable star
04:59:35.36 +36:12:54.4 -- not a known variable star
04:59:37.46 +36:33:04.6 -- not a known variable star
04:59:39.38 +36:03:58.9 -- not a known variable star
04:59:39.48 +36:48:51.1 -- not a known variable star
04:59:41.14 +36:39:34.0 -- not a known variable star
04:59:41.99 +36:09:44.3 -- not a known variable star
04:59:42.67 +36:26:04.0 -- not a known variable star
04:59:44.38 +36:43:21.0 -- not a known variable star
04:59:45.63 +36:13:49.6 -- not a known variable star
04:59:46.05 +36:36:46.7 -- not a known variable star
04:59:46.13 +36:24:20.8 -- not a known variable star
04:59:46.18 +36:28:31.9 -- not a known variable star
04:59:46.38 +36:11:18.9 -- not a known variable star
04:59:49.14 +36:27:55.8 -- not a known variable star
04:59:49.17 +36:17:23.7 -- not a known variable star
04:59:51.47 +36:45:37.2 -- not a known variable star
04:59:55.05 +36:43:36.0 -- not a known variable star
04:59:55.75 +36:34:26.2 -- not a known variable star
04:59:56.53 +36:32:22.2 -- not a known variable star
04:59:57.26 +36:48:09.3 -- a known variable star
04:59:57.62 +36:45:31.5 -- not a known variable star
04:59:57.92 +36:30:38.9 -- a known variable star
04:59:58.79 +36:49:24.1 -- not a known variable star
05:00:00.55 +36:34:56.6 -- not a known variable star
05:00:00.83 +36:39:09.2 -- not a known variable star
05:00:03.85 +36:50:48.8 -- not a known variable star
Found 392 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
428 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 428 (excluding asteroids and hot pixels, 392 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)2461300.89739203 -observatory V36
12:38:47.47 -04:13:48.8 Mercury (-0.4mag)
13:58:12.95 -17:57:15.5 Venus (-4.8mag)
07:40:46.85 +22:13:03.3 Mars (1.2mag)
09:17:09.95 +16:22:41.3 Jupiter (-1.8mag)
00:49:13.50 +02:21:13.3 Saturn (0.4mag)
04:13:37.86 +21:01:51.7 Uranus (5.7mag)
00:12:45.66 -00:09:49.8 Neptune (7.7mag)
20:24:58.21 -23:41:36.4 Pluto (14.5mag)
16:19:54.58 -26:53:20.6 Moon (-10.0mag)
-rw-r--r-- 1 apache apache 363 Sep 17 04:35 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461300.89739203:
09:17:15.99 +16:22:11.4 Io (6.0mag)
09:17:15.25 +16:22:15.5 Europa (6.2mag)
09:16:56.65 +16:23:51.3 Ganymede (5.6mag)
09:17:26.66 +16:21:16.7 Callisto (6.8mag)
09:15:21.48 +16:42:54.9 Himalia (15.7mag)
09:17:14.20 +16:22:21.2 Thebe (16.5mag)
09:14:49.77 +16:37:04.2 Elara (17.7mag)
09:20:46.04 +15:47:38.4 Pasiphae (17.9mag)
09:17:30.88 +16:43:16.1 Carme (18.9mag)
00:49:24.42 +02:20:45.9 Titan (8.3mag)
00:49:13.71 +02:20:52.8 Rhea (9.6mag)
00:48:59.69 +02:22:13.9 Iapetus (11.0mag)
00:48:59.99 +02:21:28.0 Hyperion (14.3mag)
00:47:50.32 +02:10:06.0 Phoebe (16.3mag)
-rw-r--r-- 1 apache apache 568 Sep 17 04:36 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461300.89739203:
23:29:19.78 +10:53:23.3 JWST
16:51:09.53 +42:35:38.0 Chandra
12:25:35.65 -61:57:19.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 17 04:36 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461300.89739203 -observatory V36
03:45:14.87 +19:44:48.8 17.3mag P/1996 R2 (Lagerkvist)
18:07:23.43 -34:01:01.4 14.5mag P/2010 H2 (Vales)
07:26:42.45 -70:52:58.3 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:16:32.61 +33:58:08.6 17.7mag C/2017 K2 (PANSTARRS)
05:02:36.76 +46:47:11.5 16.2mag P/2021 N1 (ZTF)
22:05:45.79 +27:22:14.6 17.5mag C/2022 E2 (ATLAS)
07:17:24.33 +25:47:47.4 16.9mag C/2022 N2 (PANSTARRS)
10:58:44.64 +26:53:17.6 17.1mag C/2022 QE78 (ATLAS)
09:54:57.86 +05:10:33.4 18.0mag C/2022 R6 (PANSTARRS)
15:27:37.12 -16:31:52.9 15.0mag C/2023 R1 (PANSTARRS)
08:46:45.48 +33:33:48.7 15.9mag C/2024 E1 (Wierzchos)
15:08:14.88 +15:12:50.8 18.0mag C/2024 G6 (ATLAS)
18:28:31.69 +42:43:40.4 13.7mag C/2024 J3 (ATLAS)
20:13:09.79 +48:37:13.7 17.4mag C/2024 R4 (PANSTARRS)
05:40:24.13 -13:11:05.7 15.0mag C/2024 T5 (ATLAS)
07:14:27.20 +16:28:14.5 17.8mag C/2025 J1 (Borisov)
11:34:35.70 +17:58:00.9 16.6mag C/2025 V2 (Rankin)
13:28:14.45 -00:42:37.0 16.7mag C/2025 Y1 (ATLAS)
17:11:14.11 +72:10:56.4 15.9mag C/2026 A2 (Bok)
02:59:31.16 +45:41:14.9 17.5mag C/2026 B2 (Sun-Gao)
12:22:43.48 +12:06:37.0 17.6mag A/2026 E1
22:34:34.45 -35:08:36.1 13.6mag 10P/Tempel
01:35:12.57 +38:46:11.2 17.5mag 11P/Tempel-Swift-LINEAR
11:54:58.91 -06:14:28.1 16.3mag 29P/Schwassmann-Wachmann
12:28:54.33 -08:15:14.3 17.8mag 63P/Wild
06:58:09.03 +18:24:51.0 17.1mag 78P/Gehrels
03:16:08.60 +15:01:42.2 17.3mag 88P/Howell
06:12:34.80 +32:24:19.0 17.3mag 112P/Urata-Niijima
08:00:57.49 +22:02:27.0 17.8mag 114P/Wiseman-Skiff
10:50:12.04 +18:40:59.4 14.8mag 123P/West-Hartley
13:09:14.28 -24:47:00.4 17.5mag 124P/Mrkos
06:29:03.59 +20:17:47.8 15.8mag 128P/Shoemaker-Holt
01:38:17.54 -15:29:58.7 14.5mag 161P/Hartley-IRAS
09:32:32.50 +08:40:16.2 12.5mag 169P/NEAT
03:30:55.48 +07:31:17.0 14.6mag 220P/McNaught
05:14:17.65 +39:18:47.7 15.3mag 260P/McNaught
08:58:13.60 +34:32:43.9 17.3mag 295P/LINEAR
15:32:13.07 -01:22:19.5 17.9mag 391P/Kowalski
09:36:21.53 +16:20:21.5 17.8mag 450P/LONEOS
-rw-r--r-- 1 apache apache 1.9K Sep 17 04:35 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:21:12.24 +57:37:51.30 SN 2026aafh 2026-09-14.11 15.02
23:36:00.27 -19:28:18.00 SN 2026aaks 2026-09-14.44 16.89
16:35:24.86 -05:32:38.20 SN2026aasi 2026-09-12.99 16.58
16:46:08.71 +37:25:21.80 SN2026aafk 2026-09-13.25 17.4
23:48:37.86 +50:25:24.60 SN2026aafs 2026-09-13.47 17
21:20:27.02 +02:10:42.50 SN2026aagh -------
08:02:26.85 -24:37:44.10 ASASSN-26fe 2026-09-13.34 13.67
02:29:34.91 +23:06:56.30 SN2026aars 2026-09-12.27 16.93
02:47:25.52 -32:58:34.50 SN 2026znh 2026-09-9.92 16.26
04:59:14.53 -83:27:58.80 ASASSN-26fd 2026-09-9.11 17.27
17:52:06.79 -23:43:20.70 ASASSN-26fc 2026-09-8.79 12.14
03:52:53.26 -14:19:28.70 SN 2026zfw 2026-09-8 17.78
01:53:26.46 +10:07:25.10 SN2026aacj 2026-09-7.17 16.27
20:04:34.47 +62:38:38.10 SN2026zji 2026-09-7.14 15.87
22:37:05.59 +34:24:35.70 SN2026aaiv 2026-09-7.22 13.48
22:24:21.29 -10:25:31.60 ASASSN-26fb 2026-09-5.3 13.93
00:44:54.28 +41:33:10.50 AT2026aabo 2026-09-3.29 15.02
00:52:12.40 -58:22:08.60 SN 2026zhl 2026-08-31.92 16.51
19:53:57.87 +61:00:19.70 ASASSN-26fa 2026-08-31.18 14.63
00:21:50.96 -09:29:16.30 AT2026zwp 2026-08-31.41 15.59
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.79 -22:25:29.10 V8055 2026-08-30 10.76
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
00:42:12.76 +41:16:28.4 PNV J00421276+4116284 2026-09-10.9176 18.67Cmag
17:52:06.80 -23:43:20.7 TCP J17520680-2343207 2026-09-08.7896 12.6mag
-rw-r--r-- 1 apache apache 190K Sep 17 04:35 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
23:15:50.170 -00:21:47.12 AT 2026zta 2026-08-18.74 22.24
02:46:12.842 +06:11:52.33 AT 2026zsz 2026-08-23.78 19.3
22:38:13.667 +15:06:36.55 AT 2026zsy 2026-08-19.88 18.99
16:29:10.420 +50:17:23.09 SN 2026zsx 2026-08-23.92 18.643
00:30:37.105 +16:40:45.90 AT 2026zsw 2026-08-22.04 19.582
00:15:59.164 +45:15:18.02 AT 2026zsv 2026-08-15.37 21.2462
18:01:12.850 +23:06:59.14 AT 2026zsu 2026-08-12.17 20.552
16:34:01.788 +10:33:21.97 AT 2026zst 2026-08-05.18 20.8897
07:35:51.970 +14:30:02.34 AT 2026zss 2026-08-23.51 19.3532
12:34:19.746 +36:30:42.03 AT 2026zsr 2026-08-18.15 16.215
13:54:24.090 +08:32:46.11 AT 2026zsq 2026-08-17.15 19.6164
14:02:03.482 +00:12:24.13 AT 2026zsp 2026-08-18.15 20.1377
14:26:57.209 +16:14:29.77 AT 2026zso 2026-08-18.15 19.8733
15:19:36.047 +10:32:58.31 AT 2026zsn 2026-08-24.15 19.7907
14:53:08.508 -01:21:20.01 AT 2026zsm 2026-08-06.17 20.2832
23:26:24.962 -03:37:54.53 AT 2026zsl 2026-08-22.08 20.35
23:49:47.831 -44:13:09.26 AT 2026zsk 2026-08-23.60 17.63
03:00:56.094 +06:15:25.68 SN 2026zsj 2026-08-14.49 20.5067
01:07:44.807 +15:37:35.66 AT 2026zsi 2026-08-16.46 21.3122
01:56:39.058 -03:54:29.73 AT 2026zsh 2026-08-18.46 20.8101
-rw-r--r-- 1 apache apache 89K Sep 17 04:35 tns_transients_list.txt
