This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or
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 04 22.1164 2461152.6164 13.48 06:42:47.89 +00:54:51.1
211.13288 -1.50495 galactic Mon Second-epoch detections are separated by 4.4" and 7.2 pix
The object was found in VSX16" CoRoT 102659593
Type: SR
# Max. Min./Amp. JD0 Period
13.609 r Y 0.237 r 2458411.23980 156.171183000000 C
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:47.89 +00:54:51.1: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:47.89 +00:54:51.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102659593,2461152.6164,13.48,0.05,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
CoRoT 102659593 20260422.1164 13.48CV 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 04 22.1164 2461152.6164 13.46 06:50:44.10 +02:07:58.8
210.95334 0.81613 galactic Mon 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 | target | 06:50:44.10 +02:07:58.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:44.10 +02:07:58.8: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:44.10 +02:07:58.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.46,0.05,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 20260422.1164 13.46CV 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 04 22.1164 2461152.6164 13.65 06:54:46.98 -00:19:00.4
213.59520 0.59980 galactic Mon Second-epoch detections are separated by 1.6" and 7.4 pix
The object was found in VSX 7" Gaia DR3 3112515039375055744
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.640 G 15.670 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:46.98 -00:19:00.4: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:46.98 -00:19:00.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112515039375055744,2461152.6164,13.65,0.05,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 3112515039375055744 20260422.1164 13.65CV 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 04 22.1164 2461152.6164 13.47 07:01:27.97 -01:55:22.4
215.78709 1.35277 galactic Mon Second-epoch detections are separated by 2.0" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:01:27.97 -01:55:22.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:27.97 -01:55:22.4: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:27.97 -01:55:22.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260422.1164 13.47CV 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 04 22.1164 2461152.6164 13.60 06:44:49.32 +00:56:57.0
211.33276 -1.03889 galactic Mon 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 | 06:44:49.32 +00:56:57.0 (user input) | T | P | (position from user input) SpType: A6V 2012A&A...541A..34S CoRoT 102753221 J-Ks=0.830+/-0.198 (M)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:49.32 +00:56:57.0: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:49.32 +00:56:57.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.60,0.05,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 20260422.1164 13.60CV 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 04 22.1164 2461152.6164 13.57 06:54:45.18 +00:31:42.1
212.83955 0.97851 galactic Mon Second-epoch detections are separated by 1.4" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:54:45.18 +00:31:42.1 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:45.18 +00:31:42.1: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:45.18 +00:31:42.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.57,0.05,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 20260422.1164 13.57CV 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 04 22.1164 2461152.6164 13.48 06:50:18.58 -02:39:12.8
215.16552 -1.46047 galactic Mon Second-epoch detections are separated by 1.5" 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 | 06:50:18.58 -02:39:12.8 (user input) | T | P | (position from user input) SpType: F7IV 2012A&A...543A.125G CoRoT 102985728
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:18.58 -02:39:12.8: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:18.58 -02:39:12.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.48,0.05,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 20260422.1164 13.48CV 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 04 22.1164 2461152.6164 13.37 07:05:41.85 +00:52:59.6
213.77185 3.57533 galactic Mon Second-epoch detections are separated by 4.6" and 7.0 pix
The object was found in VSX10" Gaia DR3 3114532097757533440
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.530 G 14.560 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:41.85 +00:52:59.6: 14.76 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:41.85 +00:52:59.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114532097757533440,2461152.6164,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114532097757533440 20260422.1164 13.37CV 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 04 22.1164 2461152.6164 13.52 07:07:15.65 +02:10:16.5
212.80061 4.50970 galactic Mon Second-epoch detections are separated by 3.0" and 8.0 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 J106.8199+02.1672 | 07:07:15.65 +02:10:16.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:15.65 +02:10:16.5: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:15.65 +02:10:16.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.8199+02.1672,2461152.6164,13.52,0.05,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 J106.8199+02.1672 20260422.1164 13.52CV 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 04 22.1164 2461152.6164 13.46 06:48:43.92 -01:08:00.6
213.63241 -1.11882 galactic Mon Second-epoch detections are separated by 0.8" and 7.9 pix
The object was found in VSX21" Gaia DR3 3107121492465652096
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.930 G 12.950 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:43.92 -01:08:00.6: 15.01 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:43.92 -01:08:00.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107121492465652096,2461152.6164,13.46,0.05,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 3107121492465652096 20260422.1164 13.46CV 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 04 22.1164 2461152.6164 13.32 07:06:19.07 +01:07:44.0
213.62357 3.82533 galactic Mon Second-epoch detections are separated by 4.7" 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 J106.5830+01.1318 | 07:06:19.07 +01:07:44.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.654+/-0.035 (K)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:19.07 +01:07:44.0: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:19.07 +01:07:44.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.5830+01.1318,2461152.6164,13.32,0.05,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
ATO J106.5830+01.1318 20260422.1164 13.32CV 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 04 22.1164 2461152.6164 13.38 07:02:21.27 -00:52:48.4
214.96070 2.02682 galactic Mon Second-epoch detections are separated by 6.7" 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 | 07:02:21.27 -00:52:48.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:02:21.27 -00:52:48.4: 14.23 +/- 0.22 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:02:21.27 -00:52:48.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.23 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.38,0.05,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 20260422.1164 13.38CV 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 04 22.1164 2461152.6164 13.29 06:44:14.43 +00:14:39.1
211.89385 -1.48995 galactic Mon Second-epoch detections are separated by 0.7" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:44:14.43 +00:14:39.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:14.43 +00:14:39.1: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:14.43 +00:14:39.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.29,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 13.29 06:58:51.85 +02:39:10.6
211.41511 2.86071 galactic Mon Second-epoch detections are separated by 1.4" and 8.0 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 | 06:58:51.85 +02:39:10.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:51.85 +02:39:10.6: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:51.85 +02:39:10.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.29,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 13.31 07:03:28.03 -02:23:33.0
216.43357 1.58249 galactic Mon Second-epoch detections are separated by 2.4" 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 | ATO J105.8705-02.3904 | 07:03:29.85 -02:23:01.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:28.03 -02:23:33.0: 14.57 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:28.03 -02:23:33.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J105.8705-02.3904,2461152.6164,13.31,0.05,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
ATO J105.8705-02.3904 20260422.1164 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 04 22.1164 2461152.6164 13.17 07:11:04.84 +01:22:10.1
213.95296 4.99458 galactic CMi Second-epoch detections are separated by 2.5" 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 J107.7677+01.3676 | 07:11:04.84 +01:22:10.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A6IV (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:11:04.84 +01:22:10.1: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:11:04.84 +01:22:10.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.7677+01.3676,2461152.6164,13.17,0.05,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 J107.7677+01.3676 20260422.1164 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 04 22.1164 2461152.6164 13.28 06:51:10.24 -02:40:54.9
215.28874 -1.28197 galactic Mon Second-epoch detections are separated by 0.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:51:10.24 -02:40:54.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:10.24 -02:40:54.9: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:10.24 -02:40:54.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.28,0.05,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 20260422.1164 13.28CV 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 04 22.1164 2461152.6164 13.32 07:05:19.87 -03:25:08.8
217.55974 1.52586 galactic Mon Second-epoch detections are separated by 2.8" and 8.1 pix
The object was found in VSX 4" Gaia DR3 3107879640093284736
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.360 G 14.380 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:19.87 -03:25:08.8: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:19.87 -03:25:08.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107879640093284736,2461152.6164,13.32,0.05,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 3107879640093284736 20260422.1164 13.32CV 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 04 22.1164 2461152.6164 13.13 07:10:54.83 -04:19:14.2
219.00120 2.34821 galactic Mon Second-epoch detections are separated by 0.7" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.7265-04.3216 | 07:10:54.83 -04:19:14.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:10:54.83 -04:19:14.2: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:10:54.83 -04:19:14.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.7265-04.3216,2461152.6164,13.13,0.05,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
ATO J107.7265-04.3216 20260422.1164 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 04 22.1164 2461152.6164 13.18 06:48:23.40 -02:03:32.1
214.41748 -1.61654 galactic Mon Second-epoch detections are separated by 4.5" 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 | 06:48:23.40 -02:03:32.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:23.40 -02:03:32.1: 15.14 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:23.40 -02:03:32.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.18,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 13.20 07:08:47.34 -00:37:50.4
215.47491 3.57139 galactic Mon Second-epoch detections are separated by 1.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3109638205861304448 | 07:08:45.16 -00:38:21.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.334+/-0.063 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:47.34 -00:37:50.4: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:47.34 -00:37:50.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109638205861304448,2461152.6164,13.20,0.05,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
Gaia DR3 3109638205861304448 20260422.1164 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 04 22.1164 2461152.6164 13.24 06:41:26.71 +02:47:59.4
209.30076 -0.94387 galactic Mon 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 | 06:41:26.71 +02:47:59.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:41:26.71 +02:47:59.4: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:41:26.71 +02:47:59.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.24,0.05,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 20260422.1164 13.24CV 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 04 22.1164 2461152.6164 13.21 06:54:39.89 +01:28:19.3
211.98938 1.38900 galactic Mon Second-epoch detections are separated by 2.4" and 8.0 pix
The object was found in VSX 4" Gaia DR3 3114074769639625216
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.200 G 14.240 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:39.89 +01:28:19.3: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:39.89 +01:28:19.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114074769639625216,2461152.6164,13.21,0.05,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
Gaia DR3 3114074769639625216 20260422.1164 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 04 22.1164 2461152.6164 13.21 06:50:34.33 -01:55:04.8
214.54045 -1.06700 galactic Mon 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 J102.6453-01.9208 | 06:50:33.20 -01:54:57.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:34.33 -01:55:04.8: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:34.33 -01:55:04.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J102.6453-01.9208,2461152.6164,13.21,0.05,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
ATO J102.6453-01.9208 20260422.1164 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 04 22.1164 2461152.6164 13.12 06:58:53.75 +01:26:59.9
212.49098 2.32027 galactic Mon Second-epoch detections are separated by 1.2" and 8.0 pix
The object was found in VSX 5" Gaia DR3 3113930694955439360
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.090 G 14.120 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:53.75 +01:26:59.9: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:53.75 +01:26:59.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113930694955439360,2461152.6164,13.12,0.05,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
Gaia DR3 3113930694955439360 20260422.1164 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 04 22.1164 2461152.6164 13.12 06:46:20.75 +02:44:05.4
209.91771 0.11497 galactic Mon Second-epoch detections are separated by 0.6" and 8.0 pix
The object was found in VSX16" Gaia DR3 3127222660966365824
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.800 G 13.840 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:20.75 +02:44:05.4: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:20.75 +02:44:05.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127222660966365824,2461152.6164,13.12,0.05,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
Gaia DR3 3127222660966365824 20260422.1164 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 04 22.1164 2461152.6164 13.24 06:54:34.58 -00:15:47.7
213.52400 0.57823 galactic Mon Second-epoch detections are separated by 2.2" and 8.0 pix
The object was found in VSX 2" Gaia DR3 3113266766033871616
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.320 G 14.340 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:34.58 -00:15:47.7: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:34.58 -00:15:47.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113266766033871616,2461152.6164,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113266766033871616 20260422.1164 13.24CV 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 04 22.1164 2461152.6164 13.04 07:01:04.13 -04:48:06.3
218.30199 -0.05226 galactic Mon Second-epoch detections are separated by 1.8" and 7.7 pix
The object was found in VSX17" Gaia DR3 3101618780365036416
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.850 G 12.960 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:04.13 -04:48:06.3: 14.18 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:04.13 -04:48:06.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.18 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101618780365036416,2461152.6164,13.04,0.05,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
Gaia DR3 3101618780365036416 20260422.1164 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 04 22.1164 2461152.6164 13.07 07:08:44.96 -01:27:55.0
216.21361 3.18038 galactic Mon Second-epoch detections are separated by 1.9" 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 | 07:08:44.96 -01:27:55.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:44.96 -01:27:55.0: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:44.96 -01:27:55.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.07,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 13.00 06:59:42.31 -02:10:51.3
215.81551 0.84351 galactic Mon Second-epoch detections are separated by 0.9" and 7.6 pix
The object was found in VSX16" Gaia DR3 3109005952316009984
Type: E
# Max. Min./Amp. JD0 Period
15.850 G 16.050 G 0.282804000000 F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:42.31 -02:10:51.3: 14.81 +/- 0.33 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:42.31 -02:10:51.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.81 +/- 0.33
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109005952316009984,2461152.6164,13.00,0.05,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
Gaia DR3 3109005952316009984 20260422.1164 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 04 22.1164 2461152.6164 13.03 06:58:57.70 -01:46:05.7
215.36351 0.86678 galactic Mon Second-epoch detections are separated by 3.1" and 8.1 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 3112034312275453824 | 06:58:58.15 -01:46:47.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:57.70 -01:46:05.7: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:57.70 -01:46:05.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112034312275453824,2461152.6164,13.03,0.05,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 3112034312275453824 20260422.1164 13.03CV 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 04 22.1164 2461152.6164 13.02 07:08:17.23 -04:56:00.7
219.24406 1.48499 galactic Mon Second-epoch detections are separated by 2.1" and 8.1 pix
The object was found in VSX 4" Gaia DR3 3059427667355169920
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.000 G 14.030 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:17.23 -04:56:00.7: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:17.23 -04:56:00.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059427667355169920,2461152.6164,13.02,0.05,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
Gaia DR3 3059427667355169920 20260422.1164 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 04 22.1164 2461152.6164 13.01 07:02:23.56 -01:34:41.4
215.58628 1.71627 galactic Mon 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 | target | 07:02:23.56 -01:34:41.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:02:23.56 -01:34:41.4: 14.57 +/- 0.27 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:02:23.56 -01:34:41.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.57 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.01,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.93 07:01:41.15 +00:06:33.1
214.00351 2.32980 galactic Mon Second-epoch detections are separated by 3.9" and 7.2 pix
The object was found in VSX17" Gaia DR3 3112974502097691264
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.830 G 14.850 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:41.15 +00:06:33.1: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:41.15 +00:06:33.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112974502097691264,2461152.6164,12.93,0.05,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
Gaia DR3 3112974502097691264 20260422.1164 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 04 22.1164 2461152.6164 13.10 07:09:51.76 -03:51:26.7
218.46889 2.32881 galactic Mon 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 | 07:09:51.76 -03:51:26.7 (user input) | T | P | (position from user input) J-Ks=0.176+/-0.041 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:09:51.76 -03:51:26.7: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:09:51.76 -03:51:26.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.10,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 13.03 07:21:05.85 +00:28:16.8
215.90629 6.81149 galactic CMi Second-epoch detections are separated by 0.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:21:05.85 +00:28:16.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:21:05.85 +00:28:16.8: 14.66 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:21:05.85 +00:28:16.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260422.1164 13.03CV 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 04 22.1164 2461152.6164 12.81 07:12:54.81 -06:36:46.4
221.26568 1.73110 galactic Mon Second-epoch detections are separated by 2.8" and 8.3 pix
The object was found in VSX 5" Gaia DR3 3052255449925753856
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.340 G 15.370 G
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:12:54.81 -06:36:46.4: 14.47 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:12:54.81 -06:36:46.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3052255449925753856,2461152.6164,12.81,0.05,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 3052255449925753856 20260422.1164 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 04 22.1164 2461152.6164 12.97 06:41:58.53 +02:45:41.9
209.39530 -0.84357 galactic Mon Second-epoch detections are separated by 2.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:41:58.53 +02:45:41.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:41:58.53 +02:45:41.9: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:41:58.53 +02:45:41.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.97,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.84 07:10:40.40 +01:18:15.9
213.96451 4.87431 galactic CMi 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 J107.6699+01.3042 | 07:10:40.40 +01:18:15.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:10:40.40 +01:18:15.9: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:10:40.40 +01:18:15.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.6699+01.3042,2461152.6164,12.84,0.05,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 J107.6699+01.3042 20260422.1164 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 04 22.1164 2461152.6164 12.93 06:53:46.16 -00:14:32.9
213.41350 0.40816 galactic Mon Second-epoch detections are separated by 2.3" 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 J103.4439-00.2500 | 06:53:47.12 -00:14:49.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.183+/-0.044 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:46.16 -00:14:32.9: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:46.16 -00:14:32.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.4439-00.2500,2461152.6164,12.93,0.05,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
ATO J103.4439-00.2500 20260422.1164 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 04 22.1164 2461152.6164 12.96 07:06:51.27 -02:03:50.2
216.52911 2.48519 galactic Mon Second-epoch detections are separated by 2.6" and 7.7 pix
The object was found in VSX19" Gaia DR3 3109196816365114496
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.230 G 13.250 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:51.27 -02:03:50.2: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:51.27 -02:03:50.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109196816365114496,2461152.6164,12.96,0.05,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 3109196816365114496 20260422.1164 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 04 22.1164 2461152.6164 12.91 07:15:39.63 -00:49:27.4
216.43691 5.00940 galactic Mon Second-epoch detections are separated by 3.3" 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 | Gaia DR3 3110150406482209152 | 07:15:36.92 -00:49:35.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A 1949AnHar.112....1C HD 293657
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:15:39.63 -00:49:27.4: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:15:39.63 -00:49:27.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110150406482209152,2461152.6164,12.91,0.05,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
Gaia DR3 3110150406482209152 20260422.1164 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 04 22.1164 2461152.6164 12.74 07:18:48.75 -01:43:46.8
217.60793 5.29246 galactic Mon Second-epoch detections are separated by 2.7" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3109841924755441024 | 07:18:49.74 -01:43:36.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:18:48.75 -01:43:46.8: 14.76 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:18:48.75 -01:43:46.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109841924755441024,2461152.6164,12.74,0.05,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
Gaia DR3 3109841924755441024 20260422.1164 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 04 22.1164 2461152.6164 12.75 07:11:13.37 -06:42:51.7
221.16152 1.31194 galactic Mon Second-epoch detections are separated by 2.7" and 7.8 pix
The object was found in VSX 5" Gaia DR3 3052250227244975872
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.090 G 15.110 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:11:13.37 -06:42:51.7: 14.66 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:11:13.37 -06:42:51.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3052250227244975872,2461152.6164,12.75,0.05,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
Gaia DR3 3052250227244975872 20260422.1164 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 04 22.1164 2461152.6164 12.86 07:13:31.55 -03:31:14.3
218.59110 3.29510 galactic Mon Second-epoch detections are separated by 3.3" and 8.1 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 J108.3925-03.5224 | 07:13:34.21 -03:31:21.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.624+/-0.040 (K)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:13:31.55 -03:31:14.3: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:13:31.55 -03:31:14.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.3925-03.5224,2461152.6164,12.86,0.05,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
ATO J108.3925-03.5224 20260422.1164 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 04 22.1164 2461152.6164 12.80 07:13:11.35 -00:08:48.2
215.54829 4.77092 galactic Mon Second-epoch detections are separated by 3.3" and 7.6 pix
The object was found in VSX15" ZTF J071311.44-000902.8
Type: RS
# Max. Min./Amp. JD0 Period
16.397 r Y 0.247 r 2458437.89910 3.601844600000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:13:11.35 -00:08:48.2: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:13:11.35 -00:08:48.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J071311.44-000902.8,2461152.6164,12.80,0.05,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
ZTF J071311.44-000902.8 20260422.1164 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 04 22.1164 2461152.6164 12.76 07:11:55.42 -04:52:53.2
219.61539 2.31290 galactic Mon Second-epoch detections are separated by 2.1" and 7.9 pix
The object was found in VSX 3" ZTF J071155.48-045255.5
Type: EW
# Max. Min./Amp. JD0 Period
14.006 r Y 0.183 r 2458384.02500 0.416880200000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:11:55.42 -04:52:53.2: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:11:55.42 -04:52:53.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J071155.48-045255.5,2461152.6164,12.76,0.05,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
ZTF J071155.48-045255.5 20260422.1164 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 04 22.1164 2461152.6164 12.87 07:05:20.10 -02:51:43.7
217.06497 1.78205 galactic Mon Second-epoch detections are separated by 2.2" and 7.3 pix
The object was found in VSX 4" Gaia DR3 3108002544877231872
Type: RS
# Max. Min./Amp. JD0 Period
14.060 G 14.100 G K
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:20.10 -02:51:43.7: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:20.10 -02:51:43.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108002544877231872,2461152.6164,12.87,0.05,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
Gaia DR3 3108002544877231872 20260422.1164 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 04 22.1164 2461152.6164 12.85 06:42:34.69 -00:18:24.7
212.19479 -2.11115 galactic Mon 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 | ATO J100.6438-00.3074 | 06:42:34.69 -00:18:24.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G8IV 2012A&A...543A.125G CoRoT 102648670
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:34.69 -00:18:24.7: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:34.69 -00:18:24.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J100.6438-00.3074,2461152.6164,12.85,0.05,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
ATO J100.6438-00.3074 20260422.1164 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 04 22.1164 2461152.6164 12.84 06:47:08.81 -00:14:49.7
212.66269 -1.06744 galactic Mon Second-epoch detections are separated by 1.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:47:08.81 -00:14:49.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:08.81 -00:14:49.7: 15.11 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:08.81 -00:14:49.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.84,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.79 07:12:55.87 +02:30:42.5
213.14248 5.92612 galactic CMi Second-epoch detections are separated by 3.9" and 8.4 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 3115229256848204672 | 07:12:57.60 +02:30:43.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:12:55.87 +02:30:42.5: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:12:55.87 +02:30:42.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115229256848204672,2461152.6164,12.79,0.05,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
Gaia DR3 3115229256848204672 20260422.1164 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 04 22.1164 2461152.6164 12.86 07:12:17.08 -02:10:59.6
217.25875 3.63575 galactic Mon 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 | 07:12:17.08 -02:10:59.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:12:17.08 -02:10:59.6: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:12:17.08 -02:10:59.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.86,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.84 07:10:29.07 +01:45:55.0
213.53113 5.04224 galactic CMi Second-epoch detections are separated by 3.0" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:10:29.07 +01:45:55.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:10:29.07 +01:45:55.0: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:10:29.07 +01:45:55.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.84,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.82 06:37:16.16 +03:08:58.0
208.51232 -1.71058 galactic Mon Second-epoch detections are separated by 1.1" 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 | 06:37:16.16 +03:08:58.0 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:37:16.16 +03:08:58.0: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:37:16.16 +03:08:58.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.82,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.73 07:21:45.83 -00:10:00.7
216.55425 6.66667 galactic CMi Second-epoch detections are separated by 0.9" 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 | 07:21:45.83 -00:10:00.7 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:21:45.83 -00:10:00.7: 14.08 +/- 0.19 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:21:45.83 -00:10:00.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.08 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.73,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.79 07:03:11.50 +01:23:07.0
213.03823 3.24660 galactic Mon Second-epoch detections are separated by 0.7" and 7.9 pix
The object was found in VSX 4" Gaia DR3 3114624353654375040
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.880 G 13.900 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:11.50 +01:23:07.0: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:11.50 +01:23:07.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114624353654375040,2461152.6164,12.79,0.05,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
Gaia DR3 3114624353654375040 20260422.1164 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 04 22.1164 2461152.6164 12.61 07:06:11.43 -02:51:26.0
217.15858 1.97414 galactic Mon Second-epoch detections are separated by 0.3" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.5527-02.8576 | 07:06:12.65 -02:51:27.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:11.43 -02:51:26.0: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:11.43 -02:51:26.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.5527-02.8576,2461152.6164,12.61,0.05,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
ATO J106.5527-02.8576 20260422.1164 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 04 22.1164 2461152.6164 12.60 07:09:59.80 +01:25:47.9
213.77501 4.78099 galactic CMi Second-epoch detections are separated by 0.5" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.5056+01.4407 | 07:09:59.80 +01:25:47.9 (user input) | DBH (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:09:59.80 +01:25:47.9: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:09:59.80 +01:25:47.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.5056+01.4407,2461152.6164,12.60,0.05,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 J107.5056+01.4407 20260422.1164 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 04 22.1164 2461152.6164 12.69 07:09:22.87 +01:06:33.4
213.99104 4.49789 galactic Mon Second-epoch detections are separated by 2.5" 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 3114460526421262848 | 07:09:22.29 +01:07:01.8 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:09:22.87 +01:06:33.4: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:09:22.87 +01:06:33.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114460526421262848,2461152.6164,12.69,0.05,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
Gaia DR3 3114460526421262848 20260422.1164 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 04 22.1164 2461152.6164 12.76 06:57:55.21 -04:37:47.0
217.79043 -0.67142 galactic Mon Second-epoch detections are separated by 1.8" and 7.4 pix
The object was found in VSX 5" Gaia DR3 3101673034391323264
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.730 G 13.750 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:55.21 -04:37:47.0: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:55.21 -04:37:47.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101673034391323264,2461152.6164,12.76,0.05,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
Gaia DR3 3101673034391323264 20260422.1164 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 04 22.1164 2461152.6164 12.43 07:14:02.20 -01:05:37.5
216.49018 4.52509 galactic Mon Second-epoch detections are separated by 4.7" and 8.6 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 J108.5157-01.0853 | 07:14:03.78 -01:05:07.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.403+/-0.039 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:14:02.20 -01:05:37.5: 14.28 +/- 0.22 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:14:02.20 -01:05:37.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.28 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.5157-01.0853,2461152.6164,12.43,0.05,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 J108.5157-01.0853 20260422.1164 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 04 22.1164 2461152.6164 12.71 06:51:10.58 +01:06:02.7
211.92243 0.44371 galactic Mon Second-epoch detections are separated by 3.5" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:51:10.58 +01:06:02.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:10.58 +01:06:02.7: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:10.58 +01:06:02.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.71,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.71 07:03:25.16 -05:00:41.6
218.75660 0.37215 galactic Mon Second-epoch detections are separated by 1.4" and 7.5 pix
The object was found in VSX16" Gaia DR3 3101503262931006720
Type: VAR
# Max. Min./Amp. JD0 Period
15.490 G 15.550 G 0.560090000000 A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:25.16 -05:00:41.6: 14.43 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:25.16 -05:00:41.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101503262931006720,2461152.6164,12.71,0.05,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
Gaia DR3 3101503262931006720 20260422.1164 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 04 22.1164 2461152.6164 12.61 06:46:13.93 +00:50:43.7
211.58592 -0.77256 galactic Mon Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:46:13.93 +00:50:43.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:13.93 +00:50:43.7: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:13.93 +00:50:43.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.61,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.65 07:17:44.49 -01:00:25.8
216.83998 5.38743 galactic Mon Second-epoch detections are separated by 1.4" 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 | 07:17:44.49 -01:00:25.8 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:17:44.49 -01:00:25.8: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:17:44.49 -01:00:25.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.65,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.68 07:07:24.36 +02:31:25.8
212.50207 4.70226 galactic Mon Second-epoch detections are separated by 2.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:07:24.36 +02:31:25.8 (user input) | T | P | (position from user input) SpType: A2IV (LAMOST DR5) J-Ks=0.403+/-0.035 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:24.36 +02:31:25.8: 14.16 +/- 0.19 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:24.36 +02:31:25.8: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.16 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.68,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.41 07:08:48.82 -03:43:07.6
218.22525 2.16022 galactic Mon Second-epoch detections are separated by 3.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2021-03.7245 | 07:08:48.82 -03:43:07.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:48.82 -03:43:07.6: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:48.82 -03:43:07.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.2021-03.7245,2461152.6164,12.41,0.05,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
ATO J107.2021-03.7245 20260422.1164 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 04 22.1164 2461152.6164 12.58 06:47:18.07 +00:57:53.1
211.60170 -0.48035 galactic Mon 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 J101.8289+00.9643 | 06:47:18.07 +00:57:53.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:18.07 +00:57:53.1: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:18.07 +00:57:53.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101.8289+00.9643,2461152.6164,12.58,0.05,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
ATO J101.8289+00.9643 20260422.1164 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 04 22.1164 2461152.6164 12.47 07:11:44.15 -02:16:15.2
217.27362 3.47369 galactic Mon Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.9286-02.2751 | 07:11:44.15 -02:16:15.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:11:44.15 -02:16:15.2: 14.63 +/- 0.29 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:11:44.15 -02:16:15.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.63 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.9286-02.2751,2461152.6164,12.47,0.05,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 J107.9286-02.2751 20260422.1164 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 04 22.1164 2461152.6164 12.52 07:14:12.70 -04:31:50.9
219.56760 2.98047 galactic Mon Second-epoch detections are separated by 4.2" and 8.0 pix
The object was found in VSX12" Gaia DR3 3059503361857653632
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.360 G 14.390 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:14:12.70 -04:31:50.9: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:14:12.70 -04:31:50.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059503361857653632,2461152.6164,12.52,0.05,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
Gaia DR3 3059503361857653632 20260422.1164 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 04 22.1164 2461152.6164 12.45 07:04:35.25 +02:44:55.5
211.98038 4.17738 galactic Mon Second-epoch detections are separated by 0.9" and 7.9 pix
The object was found in VSX22" ASASSN-V J070436.52+024443.7
Type: SRS
# Max. Min./Amp. JD0 Period
13.790 g Y 0.200 g 2459226.77600 26.941000000000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:35.25 +02:44:55.5: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:35.25 +02:44:55.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J070436.52+024443.7,2461152.6164,12.45,0.05,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
ASASSN-V J070436.52+024443.7 20260422.1164 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 04 22.1164 2461152.6164 12.30 06:35:07.51 -03:03:03.7
213.79397 -5.01831 galactic Mon Second-epoch detections are separated by 1.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J098.7797-03.0546 | 06:35:07.51 -03:03:03.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.459+/-0.035 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:35:07.51 -03:03:03.7: 14.18 +/- 0.19 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:35:07.51 -03:03:03.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.18 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J098.7797-03.0546,2461152.6164,12.30,0.05,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
ATO J098.7797-03.0546 20260422.1164 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 04 22.1164 2461152.6164 12.33 06:59:30.41 +00:22:08.5
213.52346 1.96355 galactic Mon Second-epoch detections are separated by 0.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112954191193204096 | 06:59:30.10 +00:22:23.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:30.41 +00:22:08.5: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:30.41 +00:22:08.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112954191193204096,2461152.6164,12.33,0.05,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
Gaia DR3 3112954191193204096 20260422.1164 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 04 22.1164 2461152.6164 12.29 07:13:32.85 +00:13:15.9
215.26120 5.01888 galactic Mon Second-epoch detections are separated by 0.8" and 7.7 pix
The object was found in VSX24" Gaia DR3 3111293898573338368
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.630 G 13.660 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:13:32.85 +00:13:15.9: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:13:32.85 +00:13:15.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111293898573338368,2461152.6164,12.29,0.05,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 3111293898573338368 20260422.1164 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 04 22.1164 2461152.6164 12.29 06:43:52.81 +01:17:52.0
210.91505 -1.08919 galactic Mon Second-epoch detections are separated by 0.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J100.9704+01.3011 | 06:43:52.90 +01:18:04.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:43:52.81 +01:17:52.0: 14.10 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:43:52.81 +01:17:52.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.10 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J100.9704+01.3011,2461152.6164,12.29,0.05,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 J100.9704+01.3011 20260422.1164 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 04 22.1164 2461152.6164 12.26 06:53:55.11 +02:25:33.1
211.05497 1.65747 galactic Mon Second-epoch detections are separated by 1.7" and 7.7 pix
The object was found in VSX21" Gaia DR3 3126260828808492544
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.820 G 11.840 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:55.11 +02:25:33.1: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:55.11 +02:25:33.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126260828808492544,2461152.6164,12.26,0.05,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
Gaia DR3 3126260828808492544 20260422.1164 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 04 22.1164 2461152.6164 12.18 06:58:57.06 -03:00:41.3
216.46828 0.29648 galactic Mon Second-epoch detections are separated by 0.8" 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 | ATO J104.7305-03.0153 | 06:58:57.14 -03:01:21.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0: 1956ApJS....2..271M LF 9 -03 434 J-Ks=0.295+/-0.034 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:57.06 -03:00:41.3: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:57.06 -03:00:41.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104.7305-03.0153,2461152.6164,12.18,0.05,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 J104.7305-03.0153 20260422.1164 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 04 22.1164 2461152.6164 12.18 07:10:56.81 -04:18:47.7
218.99846 2.35891 galactic Mon Second-epoch detections are separated by 3.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.7416-04.3083 | 07:10:56.81 -04:18:47.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:10:56.81 -04:18:47.7: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:10:56.81 -04:18:47.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.7416-04.3083,2461152.6164,12.18,0.05,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 J107.7416-04.3083 20260422.1164 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 04 22.1164 2461152.6164 12.13 07:04:22.03 -05:00:12.5
218.85764 0.58564 galactic Mon Second-epoch detections are separated by 2.0" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:04:22.03 -05:00:12.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:22.03 -05:00:12.5: 14.66 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:22.03 -05:00:12.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260422.1164 12.13CV 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 04 22.1164 2461152.6164 12.10 07:18:05.03 -01:25:38.0
217.25410 5.27016 galactic Mon Second-epoch detections are separated by 2.9" and 8.0 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 J109.5177-01.4272 | 07:18:05.03 -01:25:38.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A6IV (LAMOST DR5) J-Ks=0.046+/-0.052 (A)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:18:05.03 -01:25:38.0: 14.76 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:18:05.03 -01:25:38.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J109.5177-01.4272,2461152.6164,12.10,0.05,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 J109.5177-01.4272 20260422.1164 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 04 22.1164 2461152.6164 12.05 07:06:54.73 -04:13:50.9
218.46221 1.50373 galactic Mon Second-epoch detections are separated by 1.8" 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 | Large-amplitude variable Gaia DR2 3107563977176844416 | 07:06:56.24 -04:13:48.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A0 1949AnHar.112....1C HD 296299
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:54.73 -04:13:50.9: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:54.73 -04:13:50.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3107563977176844416,2461152.6164,12.05,0.05,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
Large-amplitude variable Gaia DR2 3107563977176844416 20260422.1164 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 04 22.1164 2461152.6164 12.02 06:57:47.71 -01:31:06.6
215.00818 0.72148 galactic Mon Second-epoch detections are separated by 1.8" and 7.7 pix
The object was found in VSX 4" Gaia DR3 3112151242766551808
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.070 G 13.100 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:47.71 -01:31:06.6: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:47.71 -01:31:06.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112151242766551808,2461152.6164,12.02,0.05,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
Gaia DR3 3112151242766551808 20260422.1164 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 04 22.1164 2461152.6164 11.85 06:50:49.70 -01:13:40.1
213.95522 -0.69543 galactic Mon Second-epoch detections are separated by 1.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112361520064709376 | 06:50:48.78 -01:13:52.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.206+/-0.033 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:49.70 -01:13:40.1: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:49.70 -01:13:40.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112361520064709376,2461152.6164,11.85,0.05,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
Gaia DR3 3112361520064709376 20260422.1164 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 04 22.1164 2461152.6164 11.65 07:04:04.45 -04:33:46.2
218.43257 0.72284 galactic Mon Second-epoch detections are separated by 0.7" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.0190-04.5636 | 07:04:04.45 -04:33:46.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:04.45 -04:33:46.2: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:04.45 -04:33:46.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.0190-04.5636,2461152.6164,11.65,0.05,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 J106.0190-04.5636 20260422.1164 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 04 22.1164 2461152.6164 11.71 07:04:15.81 -02:22:57.8
216.51597 1.76381 galactic Mon Second-epoch detections are separated by 0.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.0653-02.3877 | 07:04:17.76 -02:23:12.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A3 1949AnHar.112....1C HD 293166
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:15.81 -02:22:57.8: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:15.81 -02:22:57.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.0653-02.3877,2461152.6164,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0653-02.3877 20260422.1164 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 04 22.1164 2461152.6164 11.75 07:06:21.62 -03:11:42.1
217.47839 1.85689 galactic Mon Second-epoch detections are separated by 0.5" and 7.7 pix
The object was found in VSX 4" GDS_J0706214-031145
Type: VAR
# Max. Min./Amp. JD0 Period
12.900 r Y 0.150 r
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:21.62 -03:11:42.1: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:21.62 -03:11:42.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0706214-031145,2461152.6164,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0706214-031145 20260422.1164 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1164 2461152.6164 11.76 06:45:04.86 +02:50:46.6
209.67437 -0.11515 galactic Mon Second-epoch detections are separated by 1.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J101.2601+02.8485 | 06:45:02.95 +02:51:01.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5) J-Ks=0.244+/-0.030 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:45:04.86 +02:50:46.6: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:45:04.86 +02:50:46.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101.2601+02.8485,2461152.6164,11.76,0.05,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
ATO J101.2601+02.8485 20260422.1164 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 04 22.1164 2461152.6164 11.66 06:54:34.45 -00:35:21.9
213.81403 0.42899 galactic Mon 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 | ATO J103.6522-00.6011 | 06:54:35.48 -00:35:37.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5: 1956ApJS....2..271M LF 9 -01 297 J-Ks=0.117+/-0.033 (A)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:34.45 -00:35:21.9: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:34.45 -00:35:21.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.6522-00.6011,2461152.6164,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.6522-00.6011 20260422.1164 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1164 2461152.6164 11.69 07:03:52.81 +00:49:49.1
213.61154 3.14689 galactic Mon Second-epoch detections are separated by 1.1" 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 | ATO J105.9684+00.8315 | 07:03:52.59 +00:49:31.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.172+/-0.031 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:52.81 +00:49:49.1: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:52.81 +00:49:49.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J105.9684+00.8315,2461152.6164,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.9684+00.8315 20260422.1164 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 04 22.1164 2461152.6164 11.35 07:06:44.66 -01:25:53.0
215.95361 2.75047 galactic Mon Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3109303606430140928 | 07:06:45.05 -01:25:41.3 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:44.66 -01:25:53.0: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:44.66 -01:25:53.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109303606430140928,2461152.6164,11.35,0.05,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 3109303606430140928 20260422.1164 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 04 22.1164 2461152.6164 11.31 06:51:33.03 +00:27:11.7
212.54136 0.23172 galactic Mon Second-epoch detections are separated by 0.9" and 7.5 pix
The object was found in VSX25" ZTF J065134.58+002720.2
Type: EW
# Max. Min./Amp. JD0 Period
17.186 r Y 0.220 r 2458429.93560 0.622776000000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:33.03 +00:27:11.7: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:33.03 +00:27:11.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J065134.58+002720.2,2461152.6164,11.31,0.05,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
ZTF J065134.58+002720.2 20260422.1164 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 04 22.1164 2461152.6164 11.24 07:15:44.02 -06:38:23.5
221.61439 2.33917 galactic Mon 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 J108.9305-06.6437 | 07:15:43.96 -06:38:09.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:15:44.02 -06:38:23.5: 14.59 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:15:44.02 -06:38:23.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.9305-06.6437,2461152.6164,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.9305-06.6437 20260422.1164 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1164 2461152.6164 10.99 07:07:54.34 -01:34:49.4
216.21932 2.94023 galactic Mon Second-epoch detections are separated by 2.8" and 8.0 pix
The object was found in VSX 2" Gaia DR3 3109282440834765568
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.250 G 12.280 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:54.34 -01:34:49.4: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:54.34 -01:34:49.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109282440834765568,2461152.6164,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109282440834765568 20260422.1164 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1164 2461152.6164 11.15 07:04:10.78 -03:14:37.7
217.27211 1.35079 galactic Mon Second-epoch detections are separated by 0.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.0599-03.2490 | 07:04:12.73 -03:15:13.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:10.78 -03:14:37.7: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:10.78 -03:14:37.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.0599-03.2490,2461152.6164,11.15,0.05,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
ATO J106.0599-03.2490 20260422.1164 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 04 22.1164 2461152.6164 11.29 07:08:35.59 +01:46:44.6
213.30291 4.62771 galactic CMi Second-epoch detections are separated by 0.9" 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 | ATO J107.1631+01.7787 | 07:08:36.38 +01:46:22.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 1949AnHar.112....1C HD 289699 J-Ks=-0.044+/-0.034 (B)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:35.59 +01:46:44.6: 14.85 +/- 0.35 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:35.59 +01:46:44.6: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.85 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.1631+01.7787,2461152.6164,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1631+01.7787 20260422.1164 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 04 22.1164 2461152.6164 11.38 06:58:08.42 -01:38:50.9
215.16232 0.73934 galactic Mon Second-epoch detections are separated by 0.7" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112051973180962048 | 06:58:08.30 -01:38:32.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1956ApJS....2..271M LF 9 -02 476
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:08.42 -01:38:50.9: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:08.42 -01:38:50.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112051973180962048,2461152.6164,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112051973180962048 20260422.1164 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1164 2461152.6164 11.44 06:40:30.47 -01:04:41.8
212.64585 -2.92348 galactic Mon Second-epoch detections are separated by 0.8" and 7.7 pix
The object was found in VSX 4" CD Mon
Type: M
# Max. Min./Amp. JD0 Period
14.100 pg < 18.000 pg 2430441.00000 268.100000000000 M6.5
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:40:30.47 -01:04:41.8: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:40:30.47 -01:04:41.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CD Mon,2461152.6164,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CD Mon 20260422.1164 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1164 2461152.6164 11.38 06:44:27.28 +02:30:55.6
209.89725 -0.40539 galactic Mon Second-epoch detections are separated by 1.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3127192493115969152 | 06:44:28.06 +02:30:31.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 1949AnHar.112....1C HD 288998 J-Ks=0.247+/-0.033 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:27.28 +02:30:55.6: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:27.28 +02:30:55.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127192493115969152,2461152.6164,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127192493115969152 20260422.1164 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1164 2461152.6164 11.66 07:16:34.06 -05:05:58.8
220.34466 3.23743 galactic Mon Second-epoch detections are separated by 3.0" and 7.3 pix
The object was found in VSX13" Gaia DR3 3059224670018297728
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.440 G 13.470 G 0.026660200000 F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:16:34.06 -05:05:58.8: 14.51 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:16:34.06 -05:05:58.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059224670018297728,2461152.6164,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059224670018297728 20260422.1164 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1164 2461152.6164 11.89 07:17:39.14 -03:44:20.4
219.26179 4.10733 galactic Mon Second-epoch detections are separated by 1.1" and 7.7 pix
The object was found in VSX 3" Gaia DR3 3059953130831431680
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.880 G 12.910 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:17:39.14 -03:44:20.4: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:17:39.14 -03:44:20.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059953130831431680,2461152.6164,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059953130831431680 20260422.1164 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1164 2461152.6164 11.93 07:05:08.67 -01:31:32.2
215.85427 2.35186 galactic Mon 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 | Gaia DR3 3109467884639416576 | 07:05:10.00 -01:31:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:08.67 -01:31:32.2: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:08.67 -01:31:32.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109467884639416576,2461152.6164,11.93,0.05,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
Gaia DR3 3109467884639416576 20260422.1164 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 04 22.1164 2461152.6164 12.02 07:01:19.14 -03:06:44.5
216.82827 0.77612 galactic Mon Second-epoch detections are separated by 0.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.3280-03.1171 | 07:01:19.14 -03:06:44.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.053+/-0.043 (A)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:19.14 -03:06:44.5: 13.31 +/- 0.09 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:19.14 -03:06:44.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.31 +/- 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
ATO J105.3280-03.1171,2461152.6164,12.02,0.05,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
ATO J105.3280-03.1171 20260422.1164 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 04 22.1164 2461152.6164 12.08 07:03:47.20 -03:20:28.7
217.31385 1.21893 galactic Mon Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.9536-03.3472 | 07:03:47.55 -03:20:09.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:47.20 -03:20:28.7: 14.88 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:47.20 -03:20:28.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J105.9536-03.3472,2461152.6164,12.08,0.05,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
ATO J105.9536-03.3472 20260422.1164 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 04 22.1164 2461152.6164 11.97 07:19:20.29 -00:18:57.8
216.40736 6.05948 galactic Mon Second-epoch detections are separated by 1.6" and 7.6 pix
The object was found in VSX 4" Gaia DR3 3110277086535749248
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.720 G 13.760 G 0.047601500000 F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:19:20.29 -00:18:57.8: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:19:20.29 -00:18:57.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110277086535749248,2461152.6164,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110277086535749248 20260422.1164 11.97CV 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 04 22.1164 2461152.6164 12.06 06:44:33.37 -01:39:38.0
213.62611 -2.28799 galactic Mon Second-epoch detections are separated by 0.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3107031877968344192 | 06:44:30.58 -01:39:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0:III: 2010MacCon.unpub..M TYC 4799-1322-1
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:33.37 -01:39:38.0: 14.02 +/- 0.15 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:33.37 -01:39:38.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.02 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107031877968344192,2461152.6164,12.06,0.05,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 3107031877968344192 20260422.1164 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 04 22.1164 2461152.6164 12.21 07:04:54.49 +00:11:36.7
214.29645 3.08508 galactic Mon Second-epoch detections are separated by 0.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112803768556485248 | 07:04:55.43 +00:12:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.202+/-0.036 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:54.49 +00:11:36.7: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:54.49 +00:11:36.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112803768556485248,2461152.6164,12.21,0.05,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
Gaia DR3 3112803768556485248 20260422.1164 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 04 22.1164 2461152.6164 12.26 07:13:04.82 -05:12:25.0
220.03749 2.41808 galactic Mon Second-epoch detections are separated by 2.5" and 8.0 pix
The object was found in VSX12" Gaia DR3 3059182270101246208
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.470 G 14.500 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:13:04.82 -05:12:25.0: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:13:04.82 -05:12:25.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059182270101246208,2461152.6164,12.26,0.05,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
Gaia DR3 3059182270101246208 20260422.1164 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 04 22.1164 2461152.6164 12.25 06:57:11.89 -03:58:11.9
217.12123 -0.53038 galactic Mon 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 | ATO J104.2896-03.9733 | 06:57:10.73 -03:58:39.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B9 1949AnHar.112....1C HD 295858 J-Ks=0.342+/-0.033 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:11.89 -03:58:11.9: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:11.89 -03:58:11.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104.2896-03.9733,2461152.6164,12.25,0.05,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 J104.2896-03.9733 20260422.1164 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 04 22.1164 2461152.6164 12.17 07:05:12.13 -03:19:36.1
217.46281 1.53962 galactic Mon Second-epoch detections are separated by 3.3" 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 J106.3035-03.3194 | 07:05:13.97 -03:19:34.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1949AnHar.112....1C HD 296244
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:12.13 -03:19:36.1: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:12.13 -03:19:36.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.3035-03.3194,2461152.6164,12.17,0.05,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 J106.3035-03.3194 20260422.1164 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 04 22.1164 2461152.6164 12.30 06:56:45.22 +00:46:34.7
212.84687 1.53668 galactic Mon Second-epoch detections are separated by 1.8" and 8.0 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 | 06:56:45.22 +00:46:34.7 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5) J-Ks=0.683+/-0.176 (K)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:56:45.22 +00:46:34.7: 15.05 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:56:45.22 +00:46:34.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.30,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.31 07:15:57.87 -01:33:34.6
217.12742 4.73899 galactic Mon Second-epoch detections are separated by 0.5" and 7.7 pix
The object was found in VSX23" Gaia DR3 3110025298376711168
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.450 G 11.480 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:15:57.87 -01:33:34.6: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:15:57.87 -01:33:34.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110025298376711168,2461152.6164,12.31,0.05,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
Gaia DR3 3110025298376711168 20260422.1164 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 04 22.1164 2461152.6164 12.27 06:34:11.01 -00:21:48.1
211.28602 -4.00430 galactic Mon 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 | Gaia DR3 3119280785395344512 | 06:34:10.83 -00:22:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:34:11.01 -00:21:48.1: 13.17 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:34:11.01 -00:21:48.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.17 +/- 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
Gaia DR3 3119280785395344512,2461152.6164,12.27,0.05,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
Gaia DR3 3119280785395344512 20260422.1164 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 04 22.1164 2461152.6164 12.41 06:49:33.18 -01:23:30.6
213.95593 -1.05391 galactic Mon 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 | ATO J102.3878-01.3922 | 06:49:33.18 -01:23:30.6 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.321+/-0.034 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:49:33.18 -01:23:30.6: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:49:33.18 -01:23:30.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J102.3878-01.3922,2461152.6164,12.41,0.05,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
ATO J102.3878-01.3922 20260422.1164 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 04 22.1164 2461152.6164 12.29 07:07:11.27 -02:58:19.6
217.37503 2.14271 galactic Mon Second-epoch detections are separated by 0.9" 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 | Gaia DR3 3107988968482458496 | 07:07:08.73 -02:58:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:11.27 -02:58:19.6: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:11.27 -02:58:19.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107988968482458496,2461152.6164,12.29,0.05,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 3107988968482458496 20260422.1164 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 04 22.1164 2461152.6164 12.39 06:40:18.01 +00:18:22.2
211.38882 -2.33815 galactic Mon Second-epoch detections are separated by 1.9" and 8.0 pix
The object was found in VSX16" GDS_J0640172+001810
Type: VAR
# Max. Min./Amp. JD0 Period
16.440 r Y 1.940 r
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:40:18.01 +00:18:22.2: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:40:18.01 +00:18:22.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0640172+001810,2461152.6164,12.39,0.05,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
GDS_J0640172+001810 20260422.1164 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 04 22.1164 2461152.6164 12.37 07:18:50.15 -05:15:16.1
220.74463 3.66579 galactic Mon Second-epoch detections are separated by 0.8" 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 | ATO J109.7065-05.2541 | 07:18:49.43 -05:15:37.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:18:50.15 -05:15:16.1: 14.43 +/- 0.31 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:18:50.15 -05:15:16.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.43 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J109.7065-05.2541,2461152.6164,12.37,0.05,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 J109.7065-05.2541 20260422.1164 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 04 22.1164 2461152.6164 12.45 07:04:34.96 -05:56:28.7
219.71560 0.20308 galactic Mon Second-epoch detections are separated by 1.0" and 7.7 pix
The object was found in VSX11" Gaia DR3 3053264973402395520
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.670 G 13.710 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:34.96 -05:56:28.7: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:34.96 -05:56:28.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053264973402395520,2461152.6164,12.45,0.05,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
Gaia DR3 3053264973402395520 20260422.1164 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 04 22.1164 2461152.6164 12.40 06:44:31.61 +00:07:34.9
212.03141 -1.48001 galactic Mon Second-epoch detections are separated by 1.6" 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 | target | 06:44:31.61 +00:07:34.9 (user input) | T | P | (position from user input) SpType: A6V 2012A&A...541A..34S CoRoT 102738816
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:31.61 +00:07:34.9: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:31.61 +00:07:34.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.40,0.05,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
target 20260422.1164 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 04 22.1164 2461152.6164 12.44 07:10:37.59 -04:15:16.7
218.90957 2.31503 galactic Mon Second-epoch detections are separated by 0.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3059490751835095936 | 07:10:35.78 -04:15:51.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1949AnHar.112....1C HD 296608
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:10:37.59 -04:15:16.7: 14.45 +/- 0.27 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:10:37.59 -04:15:16.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.45 +/- 0.27
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059490751835095936,2461152.6164,12.44,0.05,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
Gaia DR3 3059490751835095936 20260422.1164 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 04 22.1164 2461152.6164 12.51 07:05:14.48 +00:02:11.1
214.47451 3.08746 galactic Mon Second-epoch detections are separated by 2.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112749274012032640 | 07:05:14.00 +00:01:39.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.169+/-0.039 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:14.48 +00:02:11.1: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:14.48 +00:02:11.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112749274012032640,2461152.6164,12.51,0.05,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
Gaia DR3 3112749274012032640 20260422.1164 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 04 22.1164 2461152.6164 12.62 07:20:50.47 -00:51:22.9
217.06363 6.14477 galactic Mon Second-epoch detections are separated by 4.8" and 8.6 pix
The object was found in VSX 4" Gaia DR3 3110006336102386176
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.710 G 13.750 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:20:50.47 -00:51:22.9: 14.41 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:20:50.47 -00:51:22.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110006336102386176,2461152.6164,12.62,0.05,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
Gaia DR3 3110006336102386176 20260422.1164 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 04 22.1164 2461152.6164 12.60 07:07:06.96 +01:40:01.4
213.23439 4.24806 galactic Mon Second-epoch detections are separated by 1.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3114694099624336256 | 07:07:06.57 +01:40:21.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:06.96 +01:40:01.4: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:06.96 +01:40:01.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114694099624336256,2461152.6164,12.60,0.05,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
Gaia DR3 3114694099624336256 20260422.1164 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 04 22.1164 2461152.6164 12.46 06:43:50.92 +01:35:54.7
210.64385 -0.95886 galactic Mon Second-epoch detections are separated by 0.5" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J100.9580+01.5948 | 06:43:50.92 +01:35:54.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:43:50.92 +01:35:54.7: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:43:50.92 +01:35:54.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J100.9580+01.5948,2461152.6164,12.46,0.05,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
ATO J100.9580+01.5948 20260422.1164 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 04 22.1164 2461152.6164 12.52 06:40:25.65 +00:56:10.4
210.84247 -2.02205 galactic Mon 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 J100.0980+00.9292 | 06:40:23.94 +00:56:30.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K2III 2012A&A...543A.125G CoRoT 102563601
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:40:25.65 +00:56:10.4: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:40:25.65 +00:56:10.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J100.0980+00.9292,2461152.6164,12.52,0.05,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 J100.0980+00.9292 20260422.1164 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 04 22.1164 2461152.6164 12.53 06:58:49.25 -01:06:25.7
214.75919 1.13735 galactic Mon Second-epoch detections are separated by 0.7" and 7.6 pix
The object was found in VSX 4" GDS_J0658496-010628
Type: VAR
# Max. Min./Amp. JD0 Period
13.570 r Y 0.200 r
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:49.25 -01:06:25.7: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:49.25 -01:06:25.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0658496-010628,2461152.6164,12.53,0.05,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
GDS_J0658496-010628 20260422.1164 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 04 22.1164 2461152.6164 12.59 07:01:10.31 +00:00:19.8
214.03718 2.16814 galactic Mon Second-epoch detections are separated by 0.8" and 7.7 pix
The object was found in VSX 6" Gaia DR3 3112882349279538816
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.650 G 13.670 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:10.31 +00:00:19.8: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:10.31 +00:00:19.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112882349279538816,2461152.6164,12.59,0.05,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
Gaia DR3 3112882349279538816 20260422.1164 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 04 22.1164 2461152.6164 12.56 07:07:33.28 -03:25:30.2
217.81976 2.01615 galactic Mon Second-epoch detections are separated by 0.3" and 7.8 pix
The object was found in VSX 4" GDS_J0707331-032533
Type: VAR
# Max. Min./Amp. JD0 Period
13.810 r Y 0.420 r
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:33.28 -03:25:30.2: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:33.28 -03:25:30.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0707331-032533,2461152.6164,12.56,0.05,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
GDS_J0707331-032533 20260422.1164 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 04 22.1164 2461152.6164 12.65 07:14:45.40 -01:22:48.0
216.82816 4.55350 galactic Mon 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 | 07:14:45.40 -01:22:48.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:14:45.40 -01:22:48.0: 14.63 +/- 0.32 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:14:45.40 -01:22:48.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.63 +/- 0.32
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.65,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.55 07:15:26.09 -01:11:22.4
216.73658 4.79155 galactic Mon Second-epoch detections are separated by 2.9" 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 J108.8701-01.1937 | 07:15:26.09 -01:11:22.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:15:26.09 -01:11:22.4: 14.56 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:15:26.09 -01:11:22.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.8701-01.1937,2461152.6164,12.55,0.05,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
ATO J108.8701-01.1937 20260422.1164 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 04 22.1164 2461152.6164 12.54 06:43:51.57 +02:08:02.0
210.16878 -0.71192 galactic Mon Second-epoch detections are separated by 1.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3126049894374099968 | 06:43:49.78 +02:07:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1949AnHar.112....1C HD 289007
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:43:51.57 +02:08:02.0: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:43:51.57 +02:08:02.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126049894374099968,2461152.6164,12.54,0.05,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
Gaia DR3 3126049894374099968 20260422.1164 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 04 22.1164 2461152.6164 12.62 06:59:40.39 -00:39:46.1
214.46104 1.52976 galactic Mon 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 | Gaia DR3 3112639799587138944 | 06:59:38.40 -00:39:11.0 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:40.39 -00:39:46.1: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:40.39 -00:39:46.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112639799587138944,2461152.6164,12.62,0.05,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
Gaia DR3 3112639799587138944 20260422.1164 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 04 22.1164 2461152.6164 12.54 06:54:15.99 -00:38:32.4
213.82604 0.33641 galactic Mon Second-epoch detections are separated by 1.3" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:54:15.99 -00:38:32.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:15.99 -00:38:32.4: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:15.99 -00:38:32.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.54,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.59 07:01:49.13 -03:26:18.3
217.17531 0.73787 galactic Mon Second-epoch detections are separated by 1.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3108614766697923456 | 07:01:50.08 -03:26:04.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:49.13 -03:26:18.3: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:49.13 -03:26:18.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108614766697923456,2461152.6164,12.59,0.05,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
Gaia DR3 3108614766697923456 20260422.1164 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 04 22.1164 2461152.6164 12.60 07:17:38.21 -05:59:16.4
221.25627 3.06080 galactic Mon Second-epoch detections are separated by 2.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:17:38.21 -05:59:16.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:17:38.21 -05:59:16.4: 14.63 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:17:38.21 -05:59:16.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.60,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.84 07:09:38.12 +00:33:56.3
214.50530 4.30639 galactic Mon Second-epoch detections are separated by 0.8" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.4044+00.5579 | 07:09:38.12 +00:33:56.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:09:38.12 +00:33:56.3: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:09:38.12 +00:33:56.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.4044+00.5579,2461152.6164,12.84,0.05,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 J107.4044+00.5579 20260422.1164 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 04 22.1164 2461152.6164 12.62 06:59:33.92 -01:45:36.8
215.42528 1.00464 galactic Mon Second-epoch detections are separated by 1.7" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3109125283688240640 | 06:59:35.38 -01:45:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:33.92 -01:45:36.8: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:33.92 -01:45:36.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109125283688240640,2461152.6164,12.62,0.05,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
Gaia DR3 3109125283688240640 20260422.1164 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 04 22.1164 2461152.6164 12.72 07:12:11.46 -02:24:18.5
217.44543 3.51295 galactic Mon Second-epoch detections are separated by 5.4" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:12:11.46 -02:24:18.5 (user input) | T | P | (position from user input) J-Ks=-0.060+/-0.069 (B)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:12:11.46 -02:24:18.5: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:12:11.46 -02:24:18.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.72,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.66 06:56:49.08 +00:46:31.9
212.85489 1.55064 galactic Mon Second-epoch detections are separated by 3.2" and 8.0 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 J104.2021+00.7657 | 06:56:49.08 +00:46:31.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:56:49.08 +00:46:31.9: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:56:49.08 +00:46:31.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104.2021+00.7657,2461152.6164,12.66,0.05,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
ATO J104.2021+00.7657 20260422.1164 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 04 22.1164 2461152.6164 12.76 06:43:47.33 +01:14:22.1
210.95651 -1.13613 galactic Mon 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 | ATO J100.9536+01.2405 | 06:43:47.99 +01:14:36.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:43:47.33 +01:14:22.1: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:43:47.33 +01:14:22.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J100.9536+01.2405,2461152.6164,12.76,0.05,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
ATO J100.9536+01.2405 20260422.1164 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 04 22.1164 2461152.6164 12.59 07:03:36.79 +02:37:09.4
211.98519 3.90180 galactic Mon Second-epoch detections are separated by 1.9" and 8.0 pix
The object was found in VSX 1" Gaia DR3 3115633327372214656
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.460 G 14.490 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:36.79 +02:37:09.4: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:36.79 +02:37:09.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115633327372214656,2461152.6164,12.59,0.05,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
Gaia DR3 3115633327372214656 20260422.1164 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 04 22.1164 2461152.6164 12.71 06:49:56.15 -02:40:54.4
215.14812 -1.55643 galactic Mon Second-epoch detections are separated by 1.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3105921684761121152 | 06:49:58.35 -02:41:03.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1949AnHar.112....1C HD 295506
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:49:56.15 -02:40:54.4: 14.76 +/- 0.31 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:49:56.15 -02:40:54.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.76 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105921684761121152,2461152.6164,12.71,0.05,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
Gaia DR3 3105921684761121152 20260422.1164 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 04 22.1164 2461152.6164 12.66 07:03:04.50 -01:18:36.8
215.42585 1.99044 galactic Mon Second-epoch detections are separated by 1.0" 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 | Gaia DR3 3109532137349277568 | 07:03:05.59 -01:18:09.6 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE SpType: G5 1949AnHar.112....1C HD 293113
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:04.50 -01:18:36.8: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:04.50 -01:18:36.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109532137349277568,2461152.6164,12.66,0.05,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
Gaia DR3 3109532137349277568 20260422.1164 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 04 22.1164 2461152.6164 12.74 06:49:53.06 +02:30:13.8
210.52637 0.79603 galactic Mon Second-epoch detections are separated by 2.0" and 7.8 pix
The object was found in VSX19" Gaia DR3 3126395106665966080
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.810 G 12.850 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:49:53.06 +02:30:13.8: 14.58 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:49:53.06 +02:30:13.8: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.58 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126395106665966080,2461152.6164,12.74,0.05,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
Gaia DR3 3126395106665966080 20260422.1164 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 04 22.1164 2461152.6164 12.81 07:17:41.28 +00:07:01.5
215.83011 5.89155 galactic Mon Second-epoch detections are separated by 1.3" and 8.0 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 J109.4216+00.1163 | 07:17:41.28 +00:07:01.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:17:41.28 +00:07:01.5: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:17:41.28 +00:07:01.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J109.4216+00.1163,2461152.6164,12.81,0.05,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
ATO J109.4216+00.1163 20260422.1164 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 04 22.1164 2461152.6164 12.79 07:19:55.70 -00:15:42.1
216.42692 6.21551 galactic Mon Second-epoch detections are separated by 2.9" and 8.2 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 3110276128764338304 | 07:19:57.22 -00:15:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:19:55.70 -00:15:42.1: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:19:55.70 -00:15:42.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110276128764338304,2461152.6164,12.79,0.05,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
Gaia DR3 3110276128764338304 20260422.1164 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 04 22.1164 2461152.6164 12.85 07:21:06.34 -03:15:03.8
219.22842 5.09706 galactic Mon Second-epoch detections are separated by 1.5" and 8.0 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 J110.2675-03.2520 | 07:21:06.34 -03:15:03.8 (user input) | PULSE (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:21:06.34 -03:15:03.8: 14.26 +/- 0.26 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:21:06.34 -03:15:03.8: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.26 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J110.2675-03.2520,2461152.6164,12.85,0.05,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
ATO J110.2675-03.2520 20260422.1164 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 04 22.1164 2461152.6164 12.85 07:11:45.32 -05:40:07.9
220.29501 1.91223 galactic Mon Second-epoch detections are separated by 6.0" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:11:45.32 -05:40:07.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:11:45.32 -05:40:07.9: 14.39 +/- 0.29 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:11:45.32 -05:40:07.9: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.39 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.85,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.93 07:04:10.39 -03:43:26.5
217.69830 1.12929 galactic Mon Second-epoch detections are separated by 1.5" 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 | ATO J106.0564-03.7184 | 07:04:11.69 -03:43:15.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:10.39 -03:43:26.5: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:10.39 -03:43:26.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.0564-03.7184,2461152.6164,12.93,0.05,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
ATO J106.0564-03.7184 20260422.1164 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 04 22.1164 2461152.6164 12.74 06:55:03.24 -01:02:49.4
214.27601 0.32699 galactic Mon 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 | 06:55:03.24 -01:02:49.4 (user input) | T | P | (position from user input) J-Ks=0.604+/-0.095 (K)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:55:03.24 -01:02:49.4: 13.83 +/- 0.15 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:55:03.24 -01:02:49.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.83 +/- 0.15
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.74,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.77 07:07:00.71 -00:52:19.9
215.48642 3.06585 galactic Mon Second-epoch detections are separated by 3.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:07:00.71 -00:52:19.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:00.71 -00:52:19.9: 14.88 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:00.71 -00:52:19.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.77,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.95 07:01:42.98 -06:22:07.2
219.76899 -0.62600 galactic Mon Second-epoch detections are separated by 1.9" and 7.7 pix
The object was found in VSX 3" Gaia DR3 3052850216999091968
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.070 G 14.090 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:42.98 -06:22:07.2: 14.28 +/- 0.20 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:42.98 -06:22:07.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.28 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3052850216999091968,2461152.6164,12.95,0.05,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
Gaia DR3 3052850216999091968 20260422.1164 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 04 22.1164 2461152.6164 12.72 07:10:02.75 -02:32:02.1
217.31334 2.97791 galactic Mon Second-epoch detections are separated by 3.9" and 8.3 pix
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 J107.5010-02.5329 | 07:10:00.97 -02:32:10.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F 1949AnHar.112....1C HD 296382
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:10:02.75 -02:32:02.1: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:10:02.75 -02:32:02.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.5010-02.5329,2461152.6164,12.72,0.05,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 J107.5010-02.5329 20260422.1164 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 04 22.1164 2461152.6164 12.77 07:04:16.78 -03:01:36.9
217.09071 1.47235 galactic Mon Second-epoch detections are separated by 2.0" 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 | ATO J106.0676-03.0161 | 07:04:16.78 -03:01:36.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:16.78 -03:01:36.9: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:16.78 -03:01:36.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.0676-03.0161,2461152.6164,12.77,0.05,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
ATO J106.0676-03.0161 20260422.1164 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 04 22.1164 2461152.6164 12.86 06:58:03.74 -00:47:07.7
214.38637 1.11549 galactic Mon Second-epoch detections are separated by 1.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112446977034766080 | 06:58:02.09 -00:47:35.2 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:03.74 -00:47:07.7: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:03.74 -00:47:07.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112446977034766080,2461152.6164,12.86,0.05,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
Gaia DR3 3112446977034766080 20260422.1164 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 04 22.1164 2461152.6164 12.87 06:42:44.33 +01:39:57.4
210.45716 -1.17478 galactic Mon Second-epoch detections are separated by 2.4" 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 | ATO J100.6757+01.6632 | 06:42:44.33 +01:39:57.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:44.33 +01:39:57.4: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:44.33 +01:39:57.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J100.6757+01.6632,2461152.6164,12.87,0.05,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 J100.6757+01.6632 20260422.1164 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 04 22.1164 2461152.6164 12.77 06:54:43.78 -02:41:19.4
215.69997 -0.49400 galactic Mon Second-epoch detections are separated by 0.5" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.6947-02.6960 | 06:54:45.13 -02:41:35.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.446+/-0.042 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:43.78 -02:41:19.4: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:43.78 -02:41:19.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.6947-02.6960,2461152.6164,12.77,0.05,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
ATO J103.6947-02.6960 20260422.1164 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 04 22.1164 2461152.6164 12.94 07:01:22.76 -05:01:09.1
218.53072 -0.08298 galactic Mon Second-epoch detections are separated by 3.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3101421727271429888 | 07:01:24.11 -05:00:45.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:22.76 -05:01:09.1: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:22.76 -05:01:09.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101421727271429888,2461152.6164,12.94,0.05,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
Gaia DR3 3101421727271429888 20260422.1164 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 04 22.1164 2461152.6164 12.86 06:57:12.28 -03:57:43.6
217.11498 -0.52534 galactic Mon Second-epoch detections are separated by 3.3" 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 J104.2998-03.9607 | 06:57:12.28 -03:57:43.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:12.28 -03:57:43.6: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:12.28 -03:57:43.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104.2998-03.9607,2461152.6164,12.86,0.05,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
ATO J104.2998-03.9607 20260422.1164 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 04 22.1164 2461152.6164 12.91 07:13:29.25 -03:39:20.6
218.70674 3.22431 galactic Mon Second-epoch detections are separated by 2.7" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3059628568742656768 | 07:13:29.88 -03:39:52.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.210+/-0.062 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:13:29.25 -03:39:20.6: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:13:29.25 -03:39:20.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059628568742656768,2461152.6164,12.91,0.05,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
Gaia DR3 3059628568742656768 20260422.1164 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 04 22.1164 2461152.6164 12.92 07:08:30.77 +01:18:17.8
213.71713 4.39391 galactic CMi Second-epoch detections are separated by 1.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3114481137965513216 | 07:08:31.87 +01:17:49.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.672+/- (Very red! L if it's a dwarf)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:30.77 +01:18:17.8: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:30.77 +01:18:17.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114481137965513216,2461152.6164,12.92,0.05,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
Gaia DR3 3114481137965513216 20260422.1164 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 04 22.1164 2461152.6164 12.84 06:20:54.16 -03:20:44.0
212.43784 -8.31620 galactic Mon Second-epoch detections are separated by 3.6" 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 | ATO J095.2277-03.3466 | 06:20:54.16 -03:20:44.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:20:54.16 -03:20:44.0: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:20:54.16 -03:20:44.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J095.2277-03.3466,2461152.6164,12.84,0.05,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 J095.2277-03.3466 20260422.1164 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 04 22.1164 2461152.6164 12.87 07:14:03.49 -00:18:23.3
215.79066 4.89089 galactic Mon Second-epoch detections are separated by 0.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J108.5090-00.3135 | 07:14:03.49 -00:18:23.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:14:03.49 -00:18:23.3: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:14:03.49 -00:18:23.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.5090-00.3135,2461152.6164,12.87,0.05,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 J108.5090-00.3135 20260422.1164 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 04 22.1164 2461152.6164 12.96 06:45:39.07 +02:45:23.2
209.81930 -0.02950 galactic Mon Second-epoch detections are separated by 0.5" and 7.9 pix
The object was found in VSX14" Gaia DR3 3127203655728648192
Type: RS
# Max. Min./Amp. JD0 Period
16.290 G 16.390 G K
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:45:39.07 +02:45:23.2: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:45:39.07 +02:45:23.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127203655728648192,2461152.6164,12.96,0.05,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 3127203655728648192 20260422.1164 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 04 22.1164 2461152.6164 12.86 06:54:39.48 +02:38:02.2
210.95374 1.91665 galactic Mon Second-epoch detections are separated by 2.1" 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 | Gaia DR3 3126271617766100608 | 06:54:40.63 +02:38:19.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:39.48 +02:38:02.2: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:39.48 +02:38:02.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126271617766100608,2461152.6164,12.86,0.05,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
Gaia DR3 3126271617766100608 20260422.1164 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 04 22.1164 2461152.6164 12.83 07:05:20.28 +02:45:52.5
212.05159 4.35153 galactic Mon Second-epoch detections are separated by 1.8" and 8.0 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 J106.3331+02.7602 | 07:05:20.28 +02:45:52.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.419+/-0.039 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:20.28 +02:45:52.5: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:20.28 +02:45:52.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.3331+02.7602,2461152.6164,12.83,0.05,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
ATO J106.3331+02.7602 20260422.1164 12.83CV 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 04 22.1164 2461152.6164 12.96 07:21:25.31 -03:35:02.6
219.56132 5.01249 galactic Mon Second-epoch detections are separated by 3.9" and 8.4 pix
The object was found in VSX 8" ASASSN-V J072125.37-033510.1
Type: M
# Max. Min./Amp. JD0 Period
13.400 V 15.800 V 2457393.00000 262.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:21:25.31 -03:35:02.6: 14.59 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:21:25.31 -03:35:02.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J072125.37-033510.1,2461152.6164,12.96,0.05,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
ASASSN-V J072125.37-033510.1 20260422.1164 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 04 22.1164 2461152.6164 12.96 07:04:51.59 -02:12:03.8
216.42263 1.97942 galactic Mon Second-epoch detections are separated by 1.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3108863080225629056 | 07:04:52.15 -02:11:38.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:51.59 -02:12:03.8: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:51.59 -02:12:03.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108863080225629056,2461152.6164,12.96,0.05,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 3108863080225629056 20260422.1164 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 04 22.1164 2461152.6164 13.01 06:51:18.29 -01:23:07.0
214.14968 -0.66122 galactic Mon Second-epoch detections are separated by 1.5" and 7.5 pix
The object was found in VSX 2" Gaia DR3 3106340014576032512
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.050 G 14.070 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:18.29 -01:23:07.0: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:18.29 -01:23:07.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106340014576032512,2461152.6164,13.01,0.05,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
Gaia DR3 3106340014576032512 20260422.1164 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 04 22.1164 2461152.6164 12.88 07:08:04.47 -01:43:39.9
216.36983 2.91020 galactic Mon Second-epoch detections are separated by 0.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.0154-01.7229 | 07:08:03.70 -01:43:22.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:04.47 -01:43:39.9: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:04.47 -01:43:39.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.0154-01.7229,2461152.6164,12.88,0.05,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 J107.0154-01.7229 20260422.1164 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 04 22.1164 2461152.6164 12.94 06:44:56.78 +01:18:45.2
211.02358 -0.84537 galactic Mon 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 | Gaia DR3 3125922381086607360 | 06:44:54.09 +01:18:59.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:56.78 +01:18:45.2: 14.76 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:56.78 +01:18:45.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125922381086607360,2461152.6164,12.94,0.05,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
Gaia DR3 3125922381086607360 20260422.1164 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 04 22.1164 2461152.6164 12.88 06:50:59.49 +00:13:41.2
212.67801 0.00469 galactic Mon Second-epoch detections are separated by 2.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.7477+00.2283 | 06:50:57.58 +00:13:52.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1956ApJS....2..271M LF 9 +00 109 J-Ks=0.496+/-0.131 (K)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:59.49 +00:13:41.2: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:59.49 +00:13:41.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J102.7477+00.2283,2461152.6164,12.88,0.05,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 J102.7477+00.2283 20260422.1164 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 04 22.1164 2461152.6164 12.93 06:37:33.36 +01:24:38.3
210.09181 -2.44344 galactic Mon 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 | Gaia DR3 3120640434603280512 | 06:37:33.55 +01:24:10.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:37:33.36 +01:24:38.3: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:37:33.36 +01:24:38.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3120640434603280512,2461152.6164,12.93,0.05,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
Gaia DR3 3120640434603280512 20260422.1164 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 04 22.1164 2461152.6164 12.84 06:54:59.82 +00:10:52.0
213.17646 0.87447 galactic Mon Second-epoch detections are separated by 1.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113319370792417024 | 06:54:59.68 +00:10:24.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1956ApJS....2..271M LF 9 +00 286
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:59.82 +00:10:52.0: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:59.82 +00:10:52.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113319370792417024,2461152.6164,12.84,0.05,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 3113319370792417024 20260422.1164 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 04 22.1164 2461152.6164 13.02 06:37:27.06 -02:40:37.8
213.72426 -4.33115 galactic Mon Second-epoch detections are separated by 1.8" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3106651897920988800 | 06:37:24.95 -02:40:05.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 1949AnHar.112....1C HD 295232
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:37:27.06 -02:40:37.8: 14.63 +/- 0.25 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:37:27.06 -02:40:37.8: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.63 +/- 0.25
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106651897920988800,2461152.6164,13.02,0.05,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
Gaia DR3 3106651897920988800 20260422.1164 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 04 22.1164 2461152.6164 13.04 06:28:32.48 -00:56:46.0
211.15997 -5.52521 galactic Mon Second-epoch detections are separated by 3.9" and 8.2 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 | 06:28:32.48 -00:56:46.0 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:28:32.48 -00:56:46.0: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:28:32.48 -00:56:46.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.04,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 12.96 06:46:45.89 -00:18:52.0
212.67905 -1.18313 galactic Mon Second-epoch detections are separated by 0.7" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113417188665485824 | 06:46:44.04 -00:18:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1956ApJS....2..271M LF 9 -01 57
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:45.89 -00:18:52.0: 15.02 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:45.89 -00:18:52.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113417188665485824,2461152.6164,12.96,0.05,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 3113417188665485824 20260422.1164 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 04 22.1164 2461152.6164 12.96 06:49:07.30 -01:40:16.7
214.15562 -1.27722 galactic Mon Second-epoch detections are separated by 2.7" 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 | 06:49:07.30 -01:40:16.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:49:07.30 -01:40:16.7: 14.17 +/- 0.22 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:49:07.30 -01:40:16.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.17 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,12.96,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 13.04 06:47:23.74 +01:25:44.4
211.19934 -0.24753 galactic Mon Second-epoch detections are separated by 1.4" and 7.9 pix
The object was found in VSX25" Gaia DR3 3125762818759969664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.370 G 14.400 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:23.74 +01:25:44.4: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:23.74 +01:25:44.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125762818759969664,2461152.6164,13.04,0.05,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
Gaia DR3 3125762818759969664 20260422.1164 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 04 22.1164 2461152.6164 12.94 06:35:47.89 +00:35:26.6
210.62055 -3.20924 galactic Mon Second-epoch detections are separated by 2.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3120480691881910656 | 06:35:48.30 +00:35:49.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:35:47.89 +00:35:26.6: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:35:47.89 +00:35:26.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3120480691881910656,2461152.6164,12.94,0.05,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
Gaia DR3 3120480691881910656 20260422.1164 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 04 22.1164 2461152.6164 13.06 06:25:54.91 -00:53:16.5
210.80654 -6.08260 galactic Mon Second-epoch detections are separated by 2.7" 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 J096.4669-00.8880 | 06:25:54.91 -00:53:16.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:25:54.91 -00:53:16.5: 14.16 +/- 0.20 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:25:54.91 -00:53:16.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.16 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J096.4669-00.8880,2461152.6164,13.06,0.05,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 J096.4669-00.8880 20260422.1164 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 04 22.1164 2461152.6164 13.05 06:59:45.84 -03:24:18.8
216.91125 0.29704 galactic Mon Second-epoch detections are separated by 1.2" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3102672696621973888 | 06:59:45.53 -03:23:40.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G 1949AnHar.112....1C HD 295941
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:45.84 -03:24:18.8: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:45.84 -03:24:18.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102672696621973888,2461152.6164,13.05,0.05,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
Gaia DR3 3102672696621973888 20260422.1164 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 04 22.1164 2461152.6164 13.02 06:43:45.74 +00:35:16.0
211.53346 -1.43953 galactic Mon Second-epoch detections are separated by 2.6" and 8.1 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 3125582872512184960 | 06:43:43.59 +00:34:43.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:43:45.74 +00:35:16.0: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:43:45.74 +00:35:16.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125582872512184960,2461152.6164,13.02,0.05,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
Gaia DR3 3125582872512184960 20260422.1164 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 04 22.1164 2461152.6164 13.03 07:08:43.12 +01:18:06.7
213.74340 4.43829 galactic Mon Second-epoch detections are separated by 3.1" and 8.2 pix
The object was found in VSX 6" Gaia DR3 3114478256045530880
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.160 G 14.190 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:43.12 +01:18:06.7: 14.70 +/- 0.34 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:43.12 +01:18:06.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.70 +/- 0.34
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114478256045530880,2461152.6164,13.03,0.05,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 3114478256045530880 20260422.1164 13.03CV 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 04 22.1164 2461152.6164 13.08 07:07:40.48 -03:15:05.8
217.67934 2.12239 galactic Mon Second-epoch detections are separated by 0.8" and 7.7 pix
The object was found in VSX 7" Gaia DR3 3107920768701471488
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.140 G 14.170 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:07:40.48 -03:15:05.8: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:07:40.48 -03:15:05.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107920768701471488,2461152.6164,13.08,0.05,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 3107920768701471488 20260422.1164 13.08CV 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 04 22.1164 2461152.6164 13.01 06:45:33.69 -00:26:17.2
212.65193 -1.50725 galactic Mon Second-epoch detections are separated by 1.1" and 7.6 pix
The object was found in VSX 4" CoRoT 102785122
Type: EA
# Max. Min./Amp. JD0 Period
14.112 V Y 0.113 V 2454412.42910 14.231450000000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:45:33.69 -00:26:17.2: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:45:33.69 -00:26:17.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102785122,2461152.6164,13.01,0.05,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
CoRoT 102785122 20260422.1164 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 04 22.1164 2461152.6164 13.12 06:50:49.64 +02:42:35.2
210.45039 1.09952 galactic Mon Second-epoch detections are separated by 3.0" 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 3126498117161077504 | 06:50:48.04 +02:42:41.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:49.64 +02:42:35.2: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:49.64 +02:42:35.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126498117161077504,2461152.6164,13.12,0.05,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
Gaia DR3 3126498117161077504 20260422.1164 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 04 22.1164 2461152.6164 13.18 06:50:09.69 -03:29:03.2
215.88857 -1.87158 galactic Mon Second-epoch detections are separated by 2.3" and 7.3 pix
The object was found in VSX 2" BEST-II lra2a_00642
Type: ELL/RS/BY
# Max. Min./Amp. JD0 Period
14.562 CR Y 0.090 CR 4.226000000000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:09.69 -03:29:03.2: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:09.69 -03:29:03.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BEST-II lra2a_00642,2461152.6164,13.18,0.05,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
BEST-II lra2a_00642 20260422.1164 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 04 22.1164 2461152.6164 13.03 06:44:50.75 +01:05:47.0
211.20447 -0.96639 galactic Mon Second-epoch detections are separated by 3.6" and 8.4 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 3125637852391270784 | 06:44:48.40 +01:06:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K2III 2012A&A...543A.125G CoRoT 102751495
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:50.75 +01:05:47.0: 14.76 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:50.75 +01:05:47.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125637852391270784,2461152.6164,13.03,0.05,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 3125637852391270784 20260422.1164 13.03CV 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 04 22.1164 2461152.6164 13.00 06:47:41.10 +00:31:32.3
212.03625 -0.59527 galactic Mon Second-epoch detections are separated by 1.0" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113534462753024768 | 06:47:38.55 +00:31:15.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1949AnHar.112....1C HD 292275
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:41.10 +00:31:32.3: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:41.10 +00:31:32.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113534462753024768,2461152.6164,13.00,0.05,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
Gaia DR3 3113534462753024768 20260422.1164 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 04 22.1164 2461152.6164 13.11 06:38:52.44 +01:12:25.3
210.42383 -2.24364 galactic Mon Second-epoch detections are separated by 1.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.391 Ingeborg 401 -371 546 16.1 -0 0
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:38:52.44 +01:12:25.3: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:38:52.44 +01:12:25.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461152.6164,13.11,0.05,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
VARIABLE_NAME 20260422.1164 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 04 22.1164 2461152.6164 13.06 07:09:21.65 +01:07:26.5
213.97555 4.50009 galactic Mon Second-epoch detections are separated by 3.6" and 7.2 pix
The object was found in VSX 3" Gaia DR3 3114460526421262848
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.120 G 14.150 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:09:21.65 +01:07:26.5: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:09:21.65 +01:07:26.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114460526421262848,2461152.6164,13.06,0.05,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
Gaia DR3 3114460526421262848 20260422.1164 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 04 22.1164 2461152.6164 13.17 06:53:02.86 +01:17:30.2
211.96568 0.94707 galactic Mon Second-epoch detections are separated by 1.6" and 7.5 pix
The object was found in VSX 6" Gaia DR3 3114067687234902528
Type: E
# Max. Min./Amp. JD0 Period
14.230 G 14.580 G 0.407488000000 B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:53:02.86 +01:17:30.2: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:53:02.86 +01:17:30.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114067687234902528,2461152.6164,13.17,0.05,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
Gaia DR3 3114067687234902528 20260422.1164 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 04 22.1164 2461152.6164 13.02 07:20:48.79 -00:38:29.4
216.86850 6.23742 galactic Mon Second-epoch detections are separated by 0.9" 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 | Gaia DR3 3110203694134612608 | 07:20:48.68 -00:38:09.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:20:48.79 -00:38:29.4: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:20:48.79 -00:38:29.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110203694134612608,2461152.6164,13.02,0.05,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
Gaia DR3 3110203694134612608 20260422.1164 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 04 22.1164 2461152.6164 13.06 06:40:19.45 +00:59:57.5
210.77451 -2.01620 galactic Mon Second-epoch detections are separated by 1.8" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3125854726759911936 | 06:40:18.90 +01:00:14.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:40:19.45 +00:59:57.5: 14.09 +/- 0.16 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:40:19.45 +00:59:57.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.09 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125854726759911936,2461152.6164,13.06,0.05,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
Gaia DR3 3125854726759911936 20260422.1164 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 04 22.1164 2461152.6164 13.06 07:03:16.47 -02:05:55.1
216.15015 1.67417 galactic Mon 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 | Gaia DR3 3108879371035083648 | 07:03:18.88 -02:05:41.8 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:16.47 -02:05:55.1: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:16.47 -02:05:55.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108879371035083648,2461152.6164,13.06,0.05,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
Gaia DR3 3108879371035083648 20260422.1164 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 04 22.1164 2461152.6164 13.10 07:06:54.21 +02:10:49.3
212.75175 4.43434 galactic Mon Second-epoch detections are separated by 1.4" and 7.6 pix
The object was found in VSX 3" ASASSN-V J070654.13+021046.6
Type: EA
# Max. Min./Amp. JD0 Period
13.650 V 13.870 V 2457387.86000 2.427510000000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:54.21 +02:10:49.3: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:54.21 +02:10:49.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J070654.13+021046.6,2461152.6164,13.10,0.05,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
ASASSN-V J070654.13+021046.6 20260422.1164 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 04 22.1164 2461152.6164 13.10 07:04:11.58 -04:39:48.8
218.53566 0.70297 galactic Mon Second-epoch detections are separated by 1.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3101542325647512448 | 07:04:10.97 -04:40:17.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.294+/-0.039 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:04:11.58 -04:39:48.8: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:04:11.58 -04:39:48.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101542325647512448,2461152.6164,13.10,0.05,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
Gaia DR3 3101542325647512448 20260422.1164 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 04 22.1164 2461152.6164 13.18 06:50:34.27 -02:44:32.3
215.27431 -1.44275 galactic Mon Second-epoch detections are separated by 8.7" and 9.1 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 | 06:50:34.27 -02:44:32.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:34.27 -02:44:32.3: 14.57 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:34.27 -02:44:32.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.18,0.05,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 20260422.1164 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 04 22.1164 2461152.6164 13.40 07:17:47.06 -06:57:41.9
222.13641 2.64032 galactic Mon Second-epoch detections are separated by 2.8" and 7.4 pix
The object was found in VSX 5" Gaia DR3 3057963117862558080
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.370 G 14.470 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:17:47.06 -06:57:41.9: 14.56 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:17:47.06 -06:57:41.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3057963117862558080,2461152.6164,13.40,0.05,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 3057963117862558080 20260422.1164 13.40CV 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 04 22.1164 2461152.6164 13.20 06:47:10.25 +02:54:03.4
209.86390 0.37408 galactic Mon Second-epoch detections are separated by 3.5" and 8.0 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 J101.7790+02.9110 | 06:47:09.06 +02:54:43.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:10.25 +02:54:03.4: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:10.25 +02:54:03.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101.7790+02.9110,2461152.6164,13.20,0.05,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 J101.7790+02.9110 20260422.1164 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 04 22.1164 2461152.6164 13.23 06:51:11.56 -02:22:08.7
215.01270 -1.13455 galactic Mon Second-epoch detections are separated by 1.7" 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 | ATO J102.7908-02.3649 | 06:51:10.85 -02:21:53.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:11.56 -02:22:08.7: 15.06 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:11.56 -02:22:08.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J102.7908-02.3649,2461152.6164,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.7908-02.3649 20260422.1164 13.23CV 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 04 22.1164 2461152.6164 13.30 06:58:42.35 -04:00:08.5
217.32175 -0.21065 galactic Mon Second-epoch detections are separated by 3.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3102564188568694912 | 06:58:44.54 -03:59:49.9 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE SpType: F2 1949AnHar.112....1C HD 295961
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:58:42.35 -04:00:08.5: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:58:42.35 -04:00:08.5: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102564188568694912,2461152.6164,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102564188568694912 20260422.1164 13.30CV 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 04 22.1164 2461152.6164 13.18 06:55:11.83 +00:56:25.3
212.52340 1.26514 galactic Mon Second-epoch detections are separated by 2.3" and 8.0 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 J103.7913+00.9506 | 06:55:10.02 +00:56:20.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:55:11.83 +00:56:25.3: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:55:11.83 +00:56:25.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.7913+00.9506,2461152.6164,13.18,0.05,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
ATO J103.7913+00.9506 20260422.1164 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 04 22.1164 2461152.6164 13.18 06:47:19.81 +01:08:22.4
211.44944 -0.39415 galactic Mon Second-epoch detections are separated by 1.8" and 8.0 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 J101.8303+01.1393 | 06:47:19.81 +01:08:22.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:19.81 +01:08:22.4: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:19.81 +01:08:22.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101.8303+01.1393,2461152.6164,13.18,0.05,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
ATO J101.8303+01.1393 20260422.1164 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 04 22.1164 2461152.6164 13.29 06:45:17.60 +00:43:39.8
211.58361 -1.03511 galactic Mon Second-epoch detections are separated by 2.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3125607134785759744 | 06:45:16.18 +00:44:03.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0IV 2012A&A...541A..34S CoRoT 102771943
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:45:17.60 +00:43:39.8: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:45:17.60 +00:43:39.8: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125607134785759744,2461152.6164,13.29,0.05,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 3125607134785759744 20260422.1164 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 04 22.1164 2461152.6164 13.20 06:30:04.32 +01:18:38.3
209.32225 -4.15178 galactic Mon Second-epoch detections are separated by 1.3" and 7.6 pix
The object was found in VSX 3" Gaia DR3 3120812576892617856
Type: RS
# Max. Min./Amp. JD0 Period
14.230 G 14.300 G K
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:30:04.32 +01:18:38.3: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:30:04.32 +01:18:38.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3120812576892617856,2461152.6164,13.20,0.05,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
Gaia DR3 3120812576892617856 20260422.1164 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 04 22.1164 2461152.6164 13.40 06:49:09.00 -01:39:01.6
214.14027 -1.26141 galactic Mon Second-epoch detections are separated by 4.4" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3106318947754976512 | 06:49:07.61 -01:38:36.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1956ApJS....2..271M LF 9 -02 116
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:49:09.00 -01:39:01.6: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:49:09.00 -01:39:01.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106318947754976512,2461152.6164,13.40,0.05,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 3106318947754976512 20260422.1164 13.40CV 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 04 22.1164 2461152.6164 13.44 06:43:05.05 -02:53:58.0
214.56315 -3.17906 galactic Mon Second-epoch detections are separated by 5.2" and 7.4 pix
The object was found in VSX 5" Gaia DR3 3105749679909906560
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.560 G 14.590 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:43:05.05 -02:53:58.0: 14.09 +/- 0.19 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:43:05.05 -02:53:58.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.09 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105749679909906560,2461152.6164,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105749679909906560 20260422.1164 13.44CV 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 04 22.1164 2461152.6164 13.35 06:51:28.37 -00:06:29.0
213.03207 -0.04150 galactic Mon Second-epoch detections are separated by 1.7" 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 | Gaia DR3 3113342490594252544 | 06:51:28.85 -00:06:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:51:28.37 -00:06:29.0: 14.88 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:51:28.37 -00:06:29.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113342490594252544,2461152.6164,13.35,0.05,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 3113342490594252544 20260422.1164 13.35CV 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 04 22.1164 2461152.6164 13.54 07:20:51.30 -01:01:32.3
217.21636 6.06991 galactic Mon Second-epoch detections are separated by 2.5" 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 | 07:20:51.30 -01:01:32.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:20:51.30 -01:01:32.3: 14.68 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:20:51.30 -01:01:32.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.54,0.05,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 20260422.1164 13.54CV 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 04 22.1164 2461152.6164 13.46 06:35:00.97 -02:07:00.6
212.94636 -4.61820 galactic Mon Second-epoch detections are separated by 1.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:35:00.97 -02:07:00.6 (user input) | T | P | (position from user input) J-Ks=0.639+/-0.046 (K)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:35:00.97 -02:07:00.6: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:35:00.97 -02:07:00.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.46,0.05,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 20260422.1164 13.46CV 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 04 22.1164 2461152.6164 13.54 07:01:56.30 -04:37:28.1
218.24351 0.22149 galactic Mon Second-epoch detections are separated by 2.5" 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 3101717186656904192 | 07:01:58.42 -04:37:13.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A 1949AnHar.112....1C HD 296150
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:56.30 -04:37:28.1: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:56.30 -04:37:28.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101717186656904192,2461152.6164,13.54,0.05,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 3101717186656904192 20260422.1164 13.54CV 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 04 22.1164 2461152.6164 13.39 07:21:14.17 +01:37:58.6
214.88125 7.37350 galactic CMi Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:21:14.17 +01:37:58.6 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:21:14.17 +01:37:58.6: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:21:14.17 +01:37:58.6: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.39,0.05,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 20260422.1164 13.39CV 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 04 22.1164 2461152.6164 13.37 06:57:16.81 -02:44:41.2
216.04049 0.04715 galactic Mon Second-epoch detections are separated by 3.3" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.3064-02.7341 | 06:57:14.38 -02:44:22.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8III 1956ApJS....2..271M LF 9 -03 378
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:57:16.81 -02:44:41.2: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:57:16.81 -02:44:41.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104.3064-02.7341,2461152.6164,13.37,0.05,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 J104.3064-02.7341 20260422.1164 13.37CV 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 04 22.1164 2461152.6164 13.46 06:55:15.83 +01:54:59.5
211.66174 1.72474 galactic Mon Second-epoch detections are separated by 1.3" 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 | ATO J103.8143+01.9184 | 06:55:15.83 +01:54:59.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:55:15.83 +01:54:59.5: 14.91 +/- 0.35 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:55:15.83 +01:54:59.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.91 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.8143+01.9184,2461152.6164,13.46,0.05,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 J103.8143+01.9184 20260422.1164 13.46CV 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 04 22.1164 2461152.6164 13.37 06:42:59.41 +00:50:08.3
211.22471 -1.49812 galactic Mon Second-epoch detections are separated by 2.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3125789447557134976 | 06:43:00.13 +00:50:27.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G2IV 2012A&A...543A.125G CoRoT 102668843
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:59.41 +00:50:08.3: 14.99 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:59.41 +00:50:08.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3125789447557134976,2461152.6164,13.37,0.05,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
Large-amplitude variable Gaia DR2 3125789447557134976 20260422.1164 13.37CV 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 04 22.1164 2461152.6164 13.51 07:18:56.81 -01:17:53.1
217.23869 5.52108 galactic Mon Second-epoch detections are separated by 2.1" and 7.9 pix
The object was found in VSX 3" Gaia DR3 3109874635226045696
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.580 G 14.610 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:18:56.81 -01:17:53.1: 14.52 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:18:56.81 -01:17:53.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109874635226045696,2461152.6164,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109874635226045696 20260422.1164 13.51CV 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 04 22.1164 2461152.6164 13.46 07:01:59.53 +00:49:51.0
213.39563 2.72707 galactic Mon Second-epoch detections are separated by 1.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.4965+00.8201 | 07:01:59.53 +00:49:51.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:59.53 +00:49:51.0: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:59.53 +00:49:51.0: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J105.4965+00.8201,2461152.6164,13.46,0.05,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 J105.4965+00.8201 20260422.1164 13.46CV 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 04 22.1164 2461152.6164 13.43 06:44:27.84 +03:07:19.1
209.35875 -0.12627 galactic Mon Second-epoch detections are separated by 4.7" 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 | 06:44:27.84 +03:07:19.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:27.84 +03:07:19.1: 15.00 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:27.84 +03:07:19.1: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.43,0.05,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 20260422.1164 13.43CV 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 04 22.1164 2461152.6164 13.65 06:44:36.42 -00:34:42.3
212.66802 -1.78359 galactic Mon Second-epoch detections are separated by 1.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3107426121606726016 | 06:44:37.81 -00:34:18.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A8V 2012A&A...541A..34S CoRoT 102743523
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:36.42 -00:34:42.3: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:36.42 -00:34:42.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107426121606726016,2461152.6164,13.65,0.05,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 3107426121606726016 20260422.1164 13.65CV 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 04 22.1164 2461152.6164 13.67 06:47:07.42 +01:46:46.4
210.85639 -0.14807 galactic Mon Second-epoch detections are separated by 4.1" 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 | ATO J101.7795+01.7786 | 06:47:07.42 +01:46:46.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:07.42 +01:46:46.4: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:07.42 +01:46:46.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101.7795+01.7786,2461152.6164,13.67,0.05,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 J101.7795+01.7786 20260422.1164 13.67CV 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 04 22.1164 2461152.6164 13.47 06:46:21.39 +02:10:55.9
210.41065 -0.13488 galactic Mon Second-epoch detections are separated by 2.1" and 8.1 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 3126414691716758272 | 06:46:22.14 +02:11:31.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:21.39 +02:10:55.9: 14.83 +/- 0.35 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:21.39 +02:10:55.9: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 14.83 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126414691716758272,2461152.6164,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126414691716758272 20260422.1164 13.47CV 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 04 22.1164 2461152.6164 13.67 07:08:00.99 -01:31:56.9
216.18938 2.98680 galactic Mon 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 | ATO J107.0072-01.5341 | 07:08:00.99 -01:31:56.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:00.99 -01:31:56.9: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:00.99 -01:31:56.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.0072-01.5341,2461152.6164,13.67,0.05,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 J107.0072-01.5341 20260422.1164 13.67CV 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 04 22.1164 2461152.6164 13.72 06:45:46.33 +01:57:40.7
210.54055 -0.36560 galactic Mon Second-epoch detections are separated by 2.9" 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 | ATO J101.4542+01.9640 | 06:45:46.33 +01:57:40.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:45:46.33 +01:57:40.7: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:45:46.33 +01:57:40.7: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101.4542+01.9640,2461152.6164,13.72,0.05,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 J101.4542+01.9640 20260422.1164 13.72CV 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 04 22.1164 2461152.6164 13.76 06:52:07.48 +01:07:57.9
212.00202 0.66927 galactic Mon Second-epoch detections are separated by 2.2" 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 | ATO J103.0348+01.1266 | 06:52:08.58 +01:07:23.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:52:07.48 +01:07:57.9: 14.88 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:52:07.48 +01:07:57.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.0348+01.1266,2461152.6164,13.76,0.05,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
ATO J103.0348+01.1266 20260422.1164 13.76CV 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 04 22.1164 2461152.6164 13.71 06:39:39.98 +00:06:19.3
211.49523 -2.57081 galactic Mon Second-epoch detections are separated by 2.8" 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 | 06:39:39.98 +00:06:19.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:39:39.98 +00:06:19.3: 15.07 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:39:39.98 +00:06:19.3: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6164,13.71,0.05,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 20260422.1164 13.71CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461152.61678406 22.04.2026 02:48:00.143 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 34594
Objects passed selection criteria: 34513
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 29154.5
Average stars matched: 28286.5 (97.0228 %)
Memory usage VmPeak: 136944 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 21 23:25:39 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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461152.61678406 22.04.2026 02:48:00.143 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 684
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 227 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 243951
Objects passed selection criteria: 243411
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 219696
Average stars matched: 211528 (96.2825 %)
Memory usage VmPeak: 1994364 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 21 23:33:02 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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.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: 2461152.61609425
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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
Image size: 941.4'x626.8' 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: 06:51:24.791 -02:02:55.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:24.791 -02:02:55.83
Angular distance between the image centers 0.0881 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
Image size: 941.4'x626.8' 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: 06:51:24.396 -02:03:41.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:24.396 -02:03:41.62
Angular distance between the image centers 0.0964 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 06:51:24.791 -02:02:55.83
Second-epoch second image center 06:51:24.396 -02:03:41.62
Angular distance between the image centers 0.01282 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.wAU1SsKPL4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.6OpPWBrj77
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits &> /tmp/tmp.Ua66fQ0OVJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits &> /tmp/tmp.CQ1Z24TS0h
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 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 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 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): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 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 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 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): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -> calib.txt_param_ref_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (aperture=6.0)
Read 36412 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 39.2377 to 51.3659 deg, Dec -2.9720 to +7.3737 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 39.2377 to 51.3659 deg, Dec -2.9720 to 7.3737 deg
Loaded 3163 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): 10 out of 10 total matches.
Matched with Tycho-2 10 out of 36412 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits -> calib.txt_param_ref_wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.2 pix fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
2.2 pix fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
2.1 pix wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.5 mag. fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
14.5 mag. fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.6 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wAU1SsKPL4 (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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/util/wcs_image_calibration.sh: line 129: echo: write error: Broken pipe
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 457 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 14588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.11"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 392 matched stars entering correct_measured_positions(), 14615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.01"
Accuracy estimation diagnostic: 390 matched stars entering correct_measured_positions(), 15067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6OpPWBrj77 (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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 51 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 51 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Ua66fQ0OVJ (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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2360, passed=22222
Got 22222 stars (including 19834 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat
util/solve_plate_with_UCAC5 got 22222 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 20750 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 20754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 20754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.CQ1Z24TS0h (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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2365, passed=22132
Got 22132 stars (including 19740 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat
util/solve_plate_with_UCAC5 got 22132 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 20700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 20700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 20700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits'
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out52510.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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: 0s
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Considering the candidate 52507_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 52507_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:33.06 -01:56:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52510_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 52510_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:38:08.54 -01:28:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 2.172 3106909218001458560 099.53605034664 -01.47152094130 11.0094 10.4057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 52511_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 52511_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:04:59.46 -05:12:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52649_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 52649_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:20:06.42 +01:45:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52837_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 52837_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:31.25 +01:05:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52935_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 52935_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:09:13.71 -02:21:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01285_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 01285_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:03:53.14 -06:53:22.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
Creating symlink local_wcs_cache/exclusion_list.txt
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
Plate-solving the images
wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
Image size: 941.4'x626.8' 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: 06:51:24.791 -02:02:55.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:24.791 -02:02:55.83
Angular distance between the image centers 0.0881 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
Image size: 941.4'x626.8' 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: 06:51:24.396 -02:03:41.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:24.396 -02:03:41.62
Angular distance between the image centers 0.0964 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 06:51:24.791 -02:02:55.83
Second-epoch second image center 06:51:24.396 -02:03:41.62
Angular distance between the image centers 0.01282 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.pjd2ua6PR9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.KNTGfR46zN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits &> /tmp/tmp.BT9Elhwt9O
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits &> /tmp/tmp.z7phNnUT7v
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 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 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 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): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.34
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 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 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 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): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -> calib.txt_param_ref_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (aperture=4.6)
Read 257656 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 39.1911 to 51.4130 deg, Dec -2.9804 to +7.3961 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 39.1911 to 51.4130 deg, Dec -2.9804 to 7.3961 deg
Loaded 3200 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): 37 out of 44 total matches.
Matched with Tycho-2 44 out of 257656 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits -> calib.txt_param_ref_wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 653 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.0 pix fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
2.0 pix fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
2.0 pix wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Limiting magnitude estimates:
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
13.8 mag. fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
13.8 mag. fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.1 (80% of stars) with default.sex.telephoto_lens_vSTL
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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.pjd2ua6PR9 (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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 369 matched stars entering correct_measured_positions(), 265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 366 matched stars entering correct_measured_positions(), 92781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 431 matched stars entering correct_measured_positions(), 92827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.42"
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 121659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.KNTGfR46zN (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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 68 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 44 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 44 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BT9Elhwt9O (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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=67, blended=23235, passed=184916
Got 184916 stars (including 161417 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat
util/solve_plate_with_UCAC5 got 184916 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 176897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 176896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 176893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.z7phNnUT7v (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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.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_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=73, blended=23390, passed=185839
Got 185839 stars (including 162186 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat
util/solve_plate_with_UCAC5 got 185839 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 178755 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 178754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 178754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 930 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-47-00_20.00sec_-5.00C_LIGHTs_0023.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Mon-02-Q1b1x1_214902_TTUQ1b1x1_296015_X9c6l6Or/wcs_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024.fits
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out228912.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_local.txt__out288322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288348.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295231.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 349s
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: 158s
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Considering the candidate 288191_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288191_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288196_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288196_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:42:13.03 +03:11:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.827 3127475514279986176 100.55337972649 +03.19450697437 14.5491 13.8240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288205_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288205_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:08:31.34 -01:20:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.056 3109389372638321536 107.13008995486 -01.34751304128 14.3223 13.8491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288206_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288206_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:34:57.60 -02:03:04.9: 13.45 +/- 0.09 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:34:57.60 -02:03:04.9: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.45 +/- 0.09
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Considering the candidate 288207_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288207_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288214_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288214_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288215_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288215_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288216_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288216_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:57:59.78 -03:42:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.526 3102632220850591488 104.49857615253 -03.71219974685 14.3215 13.8938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288220_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288220_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288226_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288226_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:39:48.96 +01:09:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.517 3125872112787850752 099.95380648619 +01.15118133169 14.1561 13.3983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288229_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288229_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:32:53.67 -02:29:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.355 3117239713858684160 098.22332076145 -02.49032534994 14.1143 13.6557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288235_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288235_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288244_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288244_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288247_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288247_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288249_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288249_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:01:20.00 -00:56:38.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)
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Considering the candidate 288251_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288251_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:05:29.24 +00:36:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.667 3114330779752025472 106.37153886758 +00.60895977490 13.9155 12.9822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288253_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288253_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:46:04.33 +01:26:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288255_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288255_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:56:41.84 -00:14:39.0: 13.96 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:56:41.84 -00:14:39.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.96 +/- 0.18
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Considering the candidate 288262_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288262_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:43:27.63 -00:18:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.295 3119458012928725376 100.86468471943 -00.31680254256 14.0480 13.1750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288277_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288277_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288280_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288280_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288284_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288284_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:09:19.03 -01:02:03.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 288288_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288288_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:18:25.11 -00:33:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288293_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288293_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288294_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288294_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288299_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288299_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:52:56.07 +01:21:54.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)
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Considering the candidate 288300_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288300_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:01:36.01 +01:08:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288304_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288304_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:47:09.37 +00:44:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.103 3125644724339983744 101.78871008674 +00.74104857530 14.2112 13.6608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288307_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288307_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:58:16.51 -01:15:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.891 3112208589169679232 104.56840739062 -01.26417702453 14.3482 13.6695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288318_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288318_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:08:42.75 -04:47:41.3: 12.77 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:08:42.75 -04:47:41.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.77 +/- 0.05
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Considering the candidate 288319_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288319_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:21:43.23 -01:03:25.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)
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Considering the candidate 288321_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288321_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:44:07.29 +00:48:15.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 288322_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288322_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288324_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288324_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:52:01.06 +01:29:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288326_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288326_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288327_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288327_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:29:54.13 +03:09:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.576 3124296963600786048 097.47492007358 +03.15619664476 14.0357 13.2323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288328_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288328_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288329_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288329_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288334_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288334_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:01:25.18 -00:51:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 5.040 3112572012122478976 105.35435761923 -00.86556119454 14.1848 13.5538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288338_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288338_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288340_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288340_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:50:48.85 +00:23:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 5.746 3113562912617709440 102.70303164580 +00.39751525708 14.0885 13.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288342_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288342_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:08:53.95 -04:21:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.103 3107520890069262208 107.22433824374 -04.36676847100 14.0174 13.4723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288344_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288344_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:50:51.74 -05:58:27.0: 13.80 +/- 0.14 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:50:51.74 -05:58:27.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.80 +/- 0.14
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Considering the candidate 288346_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288346_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288347_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288347_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288348_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288348_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288349_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288349_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:11.26 +00:34:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.512 3111339047269866624 108.54686574862 +00.57202174382 14.0222 13.4584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288350_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288350_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288357_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288357_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288366_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288366_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288367_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288367_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:37.96 +02:27:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288368_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288368_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:20:34.67 -00:45:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.009 3110195589538432128 110.14411394911 -00.76414228504 14.1144 13.6305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288372_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288372_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 288377_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288377_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288382_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288382_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:55:36.74 -01:03:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.261 3112415331715647360 103.90268016435 -01.05696012761 13.7754 12.6606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288384_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288384_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288399_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288399_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:39:53.31 -03:15:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288415_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288415_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:56:46.02 +01:59:35.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)
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Considering the candidate 288424_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288424_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:40:04.63 +00:50:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 4.642 3119843902850541440 100.01912767682 +00.83366555482 13.9892 13.3410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288426_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288426_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:06:04.99 +02:16:12.0: 13.41 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:06:04.99 +02:16:12.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.41 +/- 0.10
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Considering the candidate 288427_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288427_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:28:19.61 +01:29:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.766 3123823692563048960 097.08035178939 +01.48692562365 14.0161 13.2294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288428_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288428_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288429_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288429_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288431_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288431_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:04:07.25 +01:01:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288435_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288435_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:02.88 +02:12:05.2: 11.98 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:02.88 +02:12:05.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 11.98 +/- 0.03
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Considering the candidate 288440_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288440_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:28.46 -04:02:40.4: 13.96 +/- 0.15 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:28.46 -04:02:40.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.96 +/- 0.15
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Considering the candidate 288444_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288444_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:07:27.26 +01:14:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.764 3114661840129447680 106.86288543921 +01.24655473404 13.9477 13.4256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288449_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288449_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:21:12.46 -01:58:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288450_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288450_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 288458_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288458_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:49:53.35 +01:01:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.290 3113667331861561728 102.47196760975 +01.02256213902 13.9973 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288463_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288463_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288466_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288466_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288473_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288473_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:18:57.29 -03:17:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.463 3060069713422807296 109.73872149105 -03.29004521166 13.9133 13.2895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288476_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288476_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:42:30.36 +00:58:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 4.265 3125806726206403200 100.62650063837 +00.96875962341 13.6495 13.0741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288478_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288478_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:43:04.69 +01:03:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 4.662 3125820714918979840 100.76924916467 +01.05284958449 13.7488 12.9598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288481_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288481_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288482_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288482_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:16:20.55 -01:16:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 4.961 3110071241645875328 109.08444145769 -01.26765089449 13.7793 13.4437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288483_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288483_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288486_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288486_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288487_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288487_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:55:21.43 +02:36:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.305 3127768946444825344 103.83921986292 +02.61375150655 13.7963 13.4117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288488_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288488_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288493_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288493_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:52.03 -01:20:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288500_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288500_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 288501_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288501_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:43:06.99 -04:44:16.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)
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Considering the candidate 288504_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288504_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288516_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288516_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:18:03.43 +01:06:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288517_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288517_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288520_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288520_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:18:12.00 -02:02:25.8: 11.97 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:18:12.00 -02:02:25.8: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 11.97 +/- 0.03
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Considering the candidate 288523_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288523_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288527_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288527_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:12:35.69 -04:37:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.171 3059498173536851072 108.14873398337 -04.61938055361 13.8382 13.1662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288532_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288532_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:53:04.61 -05:33:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288537_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288537_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288538_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288538_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:16:59.14 +00:50:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.549 3111716970031710464 109.24683455781 +00.84420606088 13.6681 13.1142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288540_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288540_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288542_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288542_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:11:37.01 +01:52:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288545_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288545_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:19:46.21 -00:10:24.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 288549_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288549_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:22:43.62 -00:18:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288556_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288556_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:48:09.56 +03:04:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288559_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288559_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:21:09.43 -00:16:27.4: 12.71 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:21:09.43 -00:16:27.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.71 +/- 0.05
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Considering the candidate 288562_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288562_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288563_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288563_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:08:54.98 +00:18:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 4.536 3114274330999832832 107.22848021299 +00.30867156996 13.6712 12.8607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288564_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288564_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:29:29.73 -00:06:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288568_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288568_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:16:07.42 +01:27:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288569_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288569_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288572_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288572_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:34.57 -01:29:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288574_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288574_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:08:52.37 -00:44:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 4.721 3109635113484885248 107.21776257479 -00.74292765116 13.7584 13.3194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288576_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288576_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:36:00.17 -01:43:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.742 3118793942263638400 099.00070840221 -01.72803940748 13.7274 13.0717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288577_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288577_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288578_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288578_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:23.85 -04:11:38.4: 11.30 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:23.85 -04:11:38.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 11.30 +/- 0.01
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Considering the candidate 288580_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288580_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:11:34.77 +01:34:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 5.747 3114874007212799872 107.89391146696 +01.58006011879 13.6108 13.0873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288582_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288582_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288584_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288584_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:22:41.78 +02:15:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288586_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288586_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288587_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288587_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:11:59.78 -06:50:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288590_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288590_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:38:37.55 -02:21:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288592_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288592_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288593_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288593_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:32.21 -04:43:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288597_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288597_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:33.36 -02:20:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288599_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288599_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:05:19.38 -01:29:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.115 3109468056438096000 106.33034015352 -01.48790042039 13.5034 12.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288600_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288600_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:54:45.29 +02:52:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 4.628 3127827186201254400 103.68837355721 +02.86967542190 13.8439 13.3150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288606_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288606_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288608_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288608_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288609_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288609_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288610_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288610_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:11:51.91 +02:28:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288614_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288614_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:59.60 -04:42:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288615_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288615_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288617_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288617_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:11:16.42 -02:07:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.075 3108444995228839296 107.81831127898 -02.12859756211 13.5607 13.0872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288618_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288618_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:24.52 +00:13:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288620_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288620_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:53:15.97 +02:48:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.558 3126338722334559232 103.31631362468 +02.81242703418 13.7625 13.2418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288621_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288621_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288625_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288625_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288626_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288626_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:31:47.95 -00:35:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.679 3119256626203802880 097.94986559533 -00.58771369680 13.3413 12.2844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288627_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288627_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:54.50 +00:41:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288629_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288629_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288631_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288631_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288633_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288633_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288635_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288635_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:10:43.25 -00:45:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.867 3109448299588893696 107.67994343014 -00.75654112424 13.5980 12.7977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288636_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288636_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:15:07.71 -03:19:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288637_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288637_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:09:44.90 -03:41:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 3.405 3107703821317850368 107.43704622586 -03.69891737982 13.8124 13.3638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288642_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288642_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:15:08.03 +02:31:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288643_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288643_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288644_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288644_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:20:40.88 +01:06:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288646_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288646_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:06:29.33 +01:21:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.622 3114586076906068736 106.62167396384 +01.36430483885 13.5250 12.8340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288648_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288648_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:34:58.99 +02:18:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.322 3126983787762998784 098.74596416222 +02.31292312162 13.4504 12.7980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288651_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288651_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288653_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288653_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:19:27.14 -02:57:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288656_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288656_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:10:07.87 -03:36:43.2: 12.94 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:10:07.87 -03:36:43.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.94 +/- 0.06
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Considering the candidate 288657_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288657_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:06:14.85 -02:57:51.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)
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Considering the candidate 288658_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288658_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:18:52.39 -00:04:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 2.373 3110297156923792640 109.71831495544 -00.07574220333 13.4389 12.7124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288660_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288660_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:12:59.06 -00:15:50.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
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Considering the candidate 288662_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288662_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288665_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288665_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:08.15 -03:40:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288667_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288667_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:09:41.45 -00:55:18.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)
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Considering the candidate 288668_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288668_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:51:28.91 +01:57:04.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 288669_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288669_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:34.14 -00:57:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288672_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288672_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288674_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288674_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:38.08 +02:54:37.6: 13.32 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:38.08 +02:54:37.6: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.32 +/- 0.08
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Considering the candidate 288676_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288676_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:43:11.71 -02:02:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288680_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288680_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:18:37.30 -03:12:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.540 3060082907562330624 109.65485609712 -03.20929670587 13.7341 13.2004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288681_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288681_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:07:20.70 -00:46:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.959 3109623190655283968 106.83616090144 -00.78220607274 13.4448 12.9601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288685_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288685_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288689_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288689_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:40:52.96 -01:58:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288691_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288691_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288692_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288692_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288694_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288694_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288696_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288696_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288697_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288697_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288698_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288698_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288700_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288700_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:48:49.54 +03:05:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288701_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288701_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:51:40.87 -03:42:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 2.570 3102775191720876800 102.92016284722 -03.70592443961 13.4568 13.2110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288704_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288704_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:07:44.37 -01:11:01.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)
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Considering the candidate 288705_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288705_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:11:23.96 -00:34:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.223 3110953359207885056 107.84935637987 -00.57097982644 13.4770 13.3188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288708_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288708_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288709_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288709_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288710_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288710_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288711_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288711_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:08:26.32 +02:46:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 3.764 3115944175624624768 107.10939963129 +02.76846114600 13.3302 12.8585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288712_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288712_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288713_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288713_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:21:28.48 +00:26:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.482 3123319429043167104 095.36848542826 +00.43769589899 13.2224 12.7090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288717_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288717_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:56:43.60 +02:46:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.645 3127766919219874688 104.18143344956 +02.78191443907 13.3299 12.8376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288720_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288720_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:10.01 -06:22:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288722_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288722_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:43:16.53 +00:21:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288728_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288728_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288729_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288729_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:07:25.43 +02:12:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288731_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288731_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288732_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288732_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:53:54.62 +01:48:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288733_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288733_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:46:12.64 +00:51:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288734_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288734_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:53.60 +02:27:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288737_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288737_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 288740_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288740_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288742_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288742_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288744_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288744_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:09:58.03 +00:39:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.257 3114287490778891904 107.49132137484 +00.66128257443 13.4911 13.1180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288749_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288749_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:12:43.65 -02:48:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288750_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288750_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:15:19.63 -07:04:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288751_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288751_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:42.03 -01:47:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288757_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288757_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:16:32.51 -01:58:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288759_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288759_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:16:36.38 -06:36:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288762_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288762_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:03:27.01 -05:01:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288764_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288764_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288771_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288771_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:18:42.41 +01:10:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288772_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288772_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:16:04.50 +00:48:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288775_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288775_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:57:27.85 -01:45:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 3.542 3112044139160625024 104.36522484805 -01.75663240647 13.3959 12.7743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288776_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288776_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:45:55.44 -00:10:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.697 3113470622359621632 101.48089769576 -00.17232549732 12.6864 11.5266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288778_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288778_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:42:09.74 -03:38:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 2.416 3105548125684846336 100.54031504037 -03.63619866648 12.9583 12.1518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288779_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288779_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:19:07.10 -06:36:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288780_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288780_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288786_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288786_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:15:59.90 +01:17:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288787_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288787_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:08:33.16 +00:32:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 3.805 3114294122208651008 107.13787303785 +00.53631806316 13.1529 12.4015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288788_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288788_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288791_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288791_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:12:19.63 -01:08:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288792_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288792_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:02:38.85 +02:01:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.632 3115480319158580992 105.66142971541 +02.02301120173 13.0682 12.5265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288793_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288793_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288799_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288799_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:53:30.41 -06:31:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288801_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288801_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288802_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288802_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:46:35.94 +02:52:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288804_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288804_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:17.41 -01:16:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288805_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288805_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288808_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288808_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288809_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288809_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:19:17.25 -01:27:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288811_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288811_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:05:04.26 -05:27:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288813_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288813_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288817_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288817_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:09:57.35 -01:59:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.245 3108464614638568192 107.48875942657 -01.98545206208 13.0794 12.6389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288818_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288818_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:51:02.47 +01:07:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 3.991 3114047075689570688 102.75980879911 +01.12058532275 12.9570 12.4765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288820_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288820_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:52:09.30 +00:34:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 3.762 3113585005929929984 103.03834255055 +00.57848204790 12.7509 11.9519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288821_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288821_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:54:08.24 -05:52:59.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 288822_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288822_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:20:37.24 -01:34:25.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)
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Considering the candidate 288823_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288823_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288825_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288825_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:04:36.72 -01:40:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 3.076 3109456094950953344 106.15260396703 -01.66850726094 12.9200 12.5571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288826_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288826_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 288829_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288829_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:09.24 +00:52:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288832_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288832_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:43:29.67 +01:56:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288835_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288835_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:21:33.27 -02:10:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288837_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288837_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:09:20.67 +02:38:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 3.373 3115211248046545280 107.33583139358 +02.64499890828 12.8789 12.5036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288838_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288838_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288841_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288841_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:18:18.05 -00:24:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288843_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288843_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:01:13.83 -03:36:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 3.574 3102603805347108864 105.30706796189 -03.61185024820 12.7881 12.0508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288845_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288845_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288847_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288847_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:09:18.45 -01:42:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 2.834 3109224617692615680 107.32664531728 -01.70983647051 12.2567 11.3087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288848_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288848_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:16:12.76 -04:06:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288850_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288850_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:21:00.19 -01:49:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288851_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288851_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:31:32.02 +01:02:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 2.237 3120742414307317632 097.88316696000 +01.04315327108 12.7165 12.2164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288852_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288852_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:53:50.80 +01:53:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288853_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288853_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:16:32.81 -02:31:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288854_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288854_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288857_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288857_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:20:33.75 -04:55:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288858_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288858_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:21:15.23 -02:52:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288860_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288860_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:01.03 -00:19:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288861_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288861_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288862_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288862_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288864_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288864_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288865_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288865_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288868_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288868_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:43:27.92 -03:56:28.3: 11.72 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:43:27.92 -03:56:28.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 11.72 +/- 0.02
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Considering the candidate 288869_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288869_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288871_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288871_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:11:39.63 -00:56:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 3.183 3109383424102195072 107.91479278939 -00.94259728715 12.2917 11.8590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288876_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288876_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:08:48.38 +00:19:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 4.010 3114274601576731904 107.20115234593 +00.32769523318 12.5229 11.7962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288880_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288880_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:19:17.66 +01:47:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288882_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288882_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:47:44.67 +02:19:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288883_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288883_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:38:47.94 +00:39:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 3.743 3119814529571933824 099.69953942625 +00.66545390352 11.2963 9.9962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288884_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288884_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:18:50.98 -00:49:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288886_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288886_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:53:11.77 -01:33:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288888_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288888_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288890_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288890_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:03.49 -04:55:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288891_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288891_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:21:14.31 -02:12:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288892_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288892_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288894_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 288894_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 288899_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288899_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:24.43 +01:15:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288901_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288901_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:18:52.33 -01:57:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288902_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288902_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:16:02.26 -02:48:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288903_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288903_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:45:59.06 -04:51:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288905_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288905_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:56:43.78 -03:43:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288908_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 288908_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:16:54.92 -06:19:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289130_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289130_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:20:21.16 -06:07:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.76, MAG_FAINT_SEARCH_LIMIT=10.74)GAIADR2_OUTPUT=# 1.612 3008152384963645184 095.08797473371 -06.12654381191 10.5149 10.2963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289309_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289309_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:21:54.57 +01:33:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289547_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289547_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:38.91 -03:56:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289641_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289641_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:07:49.57 -05:43:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289647_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289647_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:05:27.26 -03:20:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.92, MAG_FAINT_SEARCH_LIMIT=11.90)GAIADR2_OUTPUT=# 2.893 3107881255000913152 106.36288380293 -03.34481404916 11.7246 10.8001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289681_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289681_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:51:37.29 +00:26:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289688_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 289688_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 289736_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289736_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:12:31.46 +01:47:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289745_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289745_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:50:14.55 -00:47:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289764_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289764_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:48:15.53 +01:46:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289851_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289851_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:51:39.75 +00:25:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 2.630 3113575518340150144 102.91541977930 +00.42535450446 11.9815 11.7792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289884_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 289884_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 289889_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289889_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:46:13.02 +02:40:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289975_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 289975_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:27:18.89 +00:20:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289984_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 289984_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 290014_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290014_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:11.47 -02:19:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290023_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290023_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:40:37.75 +00:43:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 2.330 3119794424826044928 100.15717896773 +00.71691830212 11.9547 11.2893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290082_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 290082_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 290166_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 290166_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 290193_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 290193_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 290231_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290231_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:12:43.28 +02:02:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290297_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290297_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:50:41.62 -00:33:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290378_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 290378_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 290384_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290384_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:33:06.41 +01:14:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 3.303 3120764095302536320 098.27668814582 +01.24558265169 12.4587 11.9747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290387_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290387_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:26:56.40 +00:49:08.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 290396_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290396_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:19:39.37 -04:12:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 2.255 3059689076241014272 109.91356328670 -04.21137790261 12.2923 11.8327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290422_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290422_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:21:53.78 +02:20:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290428_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290428_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:29:09.55 -05:33:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290478_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290478_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:36:41.11 -05:13:20.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 290501_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290501_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:44:32.11 +03:08:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 1.001 3127298492907667840 101.13405560409 +03.14936616107 12.3190 11.4547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290610_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290610_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:41.23 +00:46:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290648_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290648_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:21:54.68 +02:22:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290667_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290667_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:23:43.03 +02:39:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290700_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290700_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:41:37.46 +03:12:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 2.936 3127486917412984320 100.40610817052 +03.20929581198 12.4224 11.5651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290713_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290713_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:12:11.75 -01:59:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290739_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290739_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:47:43.40 +02:24:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290758_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290758_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:03:21.59 -04:07:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.420 3101775525191969408 105.83967354142 -04.12738694134 12.8115 11.9175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290779_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290779_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:22:45.49 -02:10:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290783_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 290783_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 290787_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290787_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:47:15.86 +02:25:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 1.724 3126425545095312128 101.81640110765 +02.41641919175 12.5279 11.6391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290811_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 290811_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 290820_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290820_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:03.74 -03:54:15.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 290833_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290833_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:49:33.85 -07:06:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290875_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290875_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:38.26 +01:13:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290906_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290906_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:21:45.64 +02:21:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290955_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 290955_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 290959_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290959_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:24:43.19 -05:30:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290986_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 290986_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 290991_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290991_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:06:42.29 -03:09:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 3.236 3107979111536590592 106.67588059035 -03.15417042601 13.0043 12.3122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290997_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 290997_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:27:08.97 +00:16:35.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 291001_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291001_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291012_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291012_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291024_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291024_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:26:19.66 +01:23:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 3.315 3123455008273752704 096.58153352703 +01.38735719100 12.8884 12.3897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291046_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291046_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:21:17.09 -00:11:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 4.477 3121734483032022144 095.32070803228 -00.20016618751 12.9368 12.0752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291071_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291071_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:08:14.33 -03:20:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.123 3107916435071192576 107.05938152547 -03.33918560888 12.7734 12.0959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.123#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291072_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291072_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:21:18.10 +02:01:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291109_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291109_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:35:16.34 -04:45:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.254 3103909715920100864 098.81776045801 -04.76603712068 12.8544 12.1285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291116_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291116_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:02:39.60 -04:37:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 3.548 3101534633371804672 105.66529147356 -04.63116397367 12.8393 12.0875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291141_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291141_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:38:39.47 -01:31:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 3.138 3106905262331173632 099.66491829980 -01.52429610039 12.4571 11.4111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291149_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291149_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 291163_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291163_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:15:55.55 -06:13:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291183_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291183_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:54:30.11 -04:07:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.698 3102509449203351296 103.62527411825 -04.12544889351 12.9516 12.4533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291195_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291195_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:35:26.34 -00:39:35.9: 11.09 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:35:26.34 -00:39:35.9: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 11.09 +/- 0.01
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Considering the candidate 291205_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291205_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291212_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291212_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:40:13.61 +01:34:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.392 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291247_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291247_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291275_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291275_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:39.79 -04:48:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291289_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291289_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:20:44.67 -02:33:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291297_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291297_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:22:50.01 -05:23:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291342_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291342_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291360_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291360_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:20:04.10 +02:27:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 3.822 3136010743866990592 110.01751277450 +02.46283457989 13.1513 12.5385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291378_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291378_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:40:17.54 -04:25:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291380_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291380_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291435_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291435_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:34:15.04 -05:19:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291438_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291438_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291461_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291461_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:12:45.23 -07:09:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291478_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291478_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:37:44.34 +02:40:58.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 291496_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291496_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:31:44.95 -05:21:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291517_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291517_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:06:52.49 -00:27:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 3.803 3109706135063598592 106.71842488065 -00.45571211931 13.1534 12.3288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291525_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291525_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291528_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291528_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:26:20.81 -03:09:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 2.822 3117129075501324160 096.58656414943 -03.16615954689 13.2570 12.7303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291560_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291560_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291565_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291565_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:12:52.31 +01:55:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291573_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291573_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:26:00.46 +01:40:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.922 3123897669081160064 096.50148930238 +01.68122666642 13.0585 12.2412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291598_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291598_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:38:54.28 +00:00:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 3.640 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291599_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291599_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:05.13 -05:55:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291614_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291614_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:19:10.74 -00:58:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291615_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291615_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291631_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291631_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:29:23.00 +02:43:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291640_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291640_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291645_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291645_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:06:30.48 -06:00:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291654_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291654_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291671_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291671_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:01:22.84 -06:08:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.095 3052874406254774656 105.34484077065 -06.13892768243 13.2836 12.7701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291711_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291711_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:32:16.74 -00:38:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291712_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291712_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:45:04.84 -01:02:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291719_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291719_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291726_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291726_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291732_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291732_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291741_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291741_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:20:04.62 +02:28:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291773_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291773_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:06:46.03 -06:03:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291794_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291794_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:00:51.62 -03:52:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.857 3101842737140035328 105.21494516568 -03.86819152005 13.1228 12.5967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291797_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291797_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:56:45.78 +00:46:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 4.429 3113784979607011712 104.19017946265 +00.76807653068 13.3516 13.0131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291811_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291811_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:20:25.43 -01:40:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291820_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291820_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:02:47.31 -04:14:50.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 291829_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291829_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:08:43.19 -05:05:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291844_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291844_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291867_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291867_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:53:07.37 -01:52:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291872_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291872_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291874_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291874_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:01:22.60 -03:06:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.699 3108642426286693376 105.34338227084 -03.10135969197 12.9086 11.8972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291895_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291895_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:59:36.46 +02:34:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291912_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291912_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:54:23.39 -01:37:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 2.488 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291925_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291925_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:01.67 -02:44:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291962_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291962_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291963_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291963_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:26:05.07 -04:38:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291969_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 291969_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 291975_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291975_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:11:26.56 -01:03:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.652 3109380129868098176 107.86006082161 -01.05220251966 13.3067 12.8199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291982_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 291982_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:21:10.25 -02:12:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292005_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292005_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292027_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292027_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292030_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292030_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:16.22 +01:04:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.627 3111747928155889280 109.31793449730 +01.07463202130 13.3570 12.6617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292052_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292052_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:40:19.08 +02:16:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 4.239 3126841542746665088 100.07927776885 +02.27567706898 13.2041 12.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292062_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292062_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:50:38.79 +01:32:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292068_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292068_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:12:28.67 -02:27:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292076_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292076_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:16:34.73 -01:08:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292083_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292083_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292096_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292096_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292101_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292101_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:37.52 -05:46:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292103_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292103_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:02:48.31 -04:14:27.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 292110_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292110_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:10:57.04 -04:52:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292146_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292146_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292153_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292153_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:23:57.53 -04:42:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292170_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292170_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:24:42.12 +00:55:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.837 3123411410063307136 096.17537123953 +00.92203400438 13.4069 12.7060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292185_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292185_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292191_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292191_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:09:55.61 -06:36:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292205_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292205_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292219_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292219_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:10:06.09 +01:43:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 4.839 3114519998829575296 107.52537717806 +01.72760034637 13.5809 13.0823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292225_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292225_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:41:18.57 -00:51:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292227_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292227_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292229_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292229_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:40:19.83 -03:22:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 3.454 3105616604643085952 100.08227451735 -03.38133788963 13.4827 13.0462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292240_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292240_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:56:33.98 -06:52:22.1: 10.27 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:56:33.98 -06:52:22.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 10.27 +/- 0.01
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Considering the candidate 292241_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292241_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292242_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292242_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:06:28.83 -05:57:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292250_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292250_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292269_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292269_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292282_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292282_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:39:29.61 -00:38:11.5: 13.35 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:39:29.61 -00:38:11.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.35 +/- 0.07
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Considering the candidate 292289_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292289_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:06:29.73 -05:59:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292307_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292307_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:56:22.09 -00:53:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 3.603 3112424230887731712 104.09176485857 -00.88726742447 13.5854 13.1578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292311_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292311_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:34:40.08 +03:03:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.992 3130061870566911360 098.66661929344 +03.05447202759 13.5218 13.0620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292320_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292320_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292347_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292347_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:53:06.87 +02:39:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.259 3126327624139131904 103.27834999029 +02.66222062235 13.3598 12.4211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292348_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292348_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:42:39.13 -02:16:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292351_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292351_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292356_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292356_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:22:33.15 -02:41:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292360_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292360_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:46:37.15 +02:26:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 1.785 3126439911764580096 101.65516521375 +02.44447897807 13.6481 13.1065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292366_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292366_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292403_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292403_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:48:31.64 -04:05:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292432_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292432_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:04:00.63 -03:17:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 5.549 3107890532129879680 106.00168451418 -03.29622223652 13.4503 12.6854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292439_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292439_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:29:17.11 -03:08:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 0.834 3117094303446320256 097.32145709055 -03.14369003432 13.4636 12.6989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292443_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292443_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:48:48.53 +00:23:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.184 3113610294697190784 102.20183118370 +00.39122776001 13.6085 13.0669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292451_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292451_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:10:19.36 -04:08:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.557 3107624690838875520 107.58011994727 -04.14429608637 13.6473 13.2554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292456_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292456_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:55:39.10 -06:15:18.1: 12.34 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:55:39.10 -06:15:18.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.34 +/- 0.04
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Considering the candidate 292457_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292457_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292458_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292458_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:50.65 +02:53:49.2: 12.20 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:50.65 +02:53:49.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.20 +/- 0.03
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Considering the candidate 292470_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292470_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:47:46.00 +02:20:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292471_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292471_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:47:33.82 -06:11:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292473_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292473_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292478_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292478_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:32:41.72 +01:49:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292484_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292484_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:22:26.75 -01:42:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.702 3118286620726617088 095.61146393470 -01.71725039683 13.3380 12.8429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292498_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292498_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:10:08.95 +02:20:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292501_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292501_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:44:26.03 -06:06:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 3.940 3100303317781995776 101.10954090124 -06.10697565398 13.0595 11.9466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292505_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292505_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292517_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292517_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292539_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292539_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292544_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292544_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:48:30.69 +00:57:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.961 3125654791743165184 102.12743384694 +00.96221421685 13.6988 13.2550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292552_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292552_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:20:47.55 -01:16:42.7: 12.91 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:20:47.55 -01:16:42.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.91 +/- 0.07
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Considering the candidate 292553_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292553_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:31:36.96 +00:48:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.977 3120722382580331520 097.90368843308 +00.81018091994 13.6357 13.0094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292578_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292578_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:33.86 +02:07:18.0: 13.09 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:33.86 +02:07:18.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.09 +/- 0.08
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Considering the candidate 292589_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292589_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:12:23.45 -05:25:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292594_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292594_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:19:49.02 -06:01:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292595_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292595_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292618_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292618_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:19:04.61 -05:42:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292619_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292619_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:11.65 -00:21:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292632_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292632_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 292649_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292649_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:46.48 -02:44:15.0: 13.11 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:46.48 -02:44:15.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.11 +/- 0.07
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Considering the candidate 292677_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292677_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292688_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292688_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292692_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292692_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:08:53.87 -03:51:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.800 3107694853426314624 107.22456365729 -03.86588354665 13.3330 12.4820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292713_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292713_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:33.23 -03:28:06.5: 12.98 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:33.23 -03:28:06.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.98 +/- 0.06
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Considering the candidate 292717_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292717_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:03:06.51 -00:13:08.0: 13.57 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:03:06.51 -00:13:08.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.57 +/- 0.10
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Considering the candidate 292718_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292718_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:03:08.22 -06:51:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292724_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292724_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:48.75 +01:46:40.6: 10.93 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:48.75 +01:46:40.6: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 10.93 +/- 0.01
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Considering the candidate 292749_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292749_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:27.99 +00:52:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292751_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292751_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:21:58.11 +01:31:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292772_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292772_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292779_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292779_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:05:24.57 -01:00:14.5: 12.25 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:05:24.57 -01:00:14.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.25 +/- 0.03
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Considering the candidate 292783_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292783_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:13.60 +00:52:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292807_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292807_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:22:43.49 -02:10:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292824_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292824_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:58:40.01 -06:20:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292826_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292826_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292834_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292834_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:07:23.01 -06:11:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.992 3053011089291501184 106.84551594434 -06.19124440033 13.6810 13.1704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292839_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292839_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:53:59.75 -02:44:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292840_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292840_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292842_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292842_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:40:25.88 -01:49:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292865_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292865_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:29:32.88 -02:51:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292867_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292867_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292883_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292883_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:01.05 -00:29:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.557 3110968919870221568 108.25448279768 -00.49114095096 13.6157 13.1652 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292903_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292903_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292916_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292916_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292922_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292922_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:46:12.57 -05:08:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292939_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292939_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:35:21.88 -05:17:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292944_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292944_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:01:26.90 -00:55:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.467 3112570461635443584 105.36207810215 -00.92448145232 13.7792 12.9935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292955_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292955_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292965_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292965_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:50.62 -07:08:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292976_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292976_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:31:58.45 -00:58:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.333 3119139287696476160 097.99329399089 -00.96953887067 12.9750 11.7594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292985_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292985_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:10:42.55 -01:49:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 5.652 3108561474741535360 107.67777569414 -01.82779928472 13.8012 13.5079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292996_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292996_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292997_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 292997_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 292998_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 292998_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:21:06.71 -03:14:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.290 3059901071527241728 110.27785224367 -03.24709950855 13.5191 12.7858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293001_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293001_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293014_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293014_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:47:06.77 +01:33:42.4: 9.98 +/- 0.00 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:47:06.77 +01:33:42.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 9.98 +/- 0.00
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Considering the candidate 293038_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293038_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:56:36.59 +02:42:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 4.095 3127764891995931648 104.15213331048 +02.71143748089 13.6251 13.1744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293039_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293039_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:48:59.33 -05:34:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293055_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293055_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293079_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293079_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:48:33.33 +01:51:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.110 3126156100326316672 102.13887908049 +01.85185846155 13.5491 12.7408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293080_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293080_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:34:09.42 -00:32:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.953 3119224229266078336 098.53855094837 -00.54001848259 13.4778 12.5108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293092_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293092_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293162_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293162_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:57:18.74 -05:58:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293170_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293170_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293180_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293180_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293200_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293200_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:41:20.95 -01:43:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293203_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293203_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:24:01.98 -02:25:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293205_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293205_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:39:32.27 +03:12:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.794 3127159061087972864 099.88415792470 +03.20149092640 13.6964 13.2339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293219_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293219_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293225_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293225_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293247_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293247_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:29:54.11 +01:22:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293248_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293248_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:38:17.99 -06:45:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.227 3100097640389269248 099.57433748949 -06.75730169050 13.6657 12.8453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293255_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293255_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293266_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293266_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293271_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293271_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:46:20.39 -05:15:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.556 3100651210134669056 101.58485367391 -05.25670435408 13.8422 13.2498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293276_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293276_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293284_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293284_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:40.04 +01:31:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293287_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293287_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 293314_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293314_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:51:42.13 +00:25:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 4.375 3113575453922853632 102.92527875821 +00.42011914305 13.6376 13.1324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293325_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293325_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:43:42.44 -04:26:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.012 3105302487915881984 100.92693219573 -04.44232787110 13.7957 13.3898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293331_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293331_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293332_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293332_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293344_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293344_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:58:50.19 -04:41:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 5.226 3101679906339288704 104.70859973578 -04.68774296413 13.8134 13.3106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293351_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293351_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:44:24.95 -00:04:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293382_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293382_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293384_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293384_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293397_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293397_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:51:56.71 -07:01:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 3.188 3099282180719501440 102.98592632821 -07.02753016354 13.9551 13.2209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293405_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293405_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:57:24.14 -02:57:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.058 3102896172359569152 104.35008263573 -02.95190892558 13.8534 13.3648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293408_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293408_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293427_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293427_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:13:48.14 -03:44:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 4.605 3059615374604845824 108.45015657413 -03.73990071395 13.9207 13.6891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293434_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293434_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293442_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293442_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:04:24.67 -04:44:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 4.358 3101515254479426176 106.10305967209 -04.74501396050 13.8733 13.4014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293446_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293446_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:42.20 -01:42:35.7: 12.60 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:42.20 -01:42:35.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.60 +/- 0.05
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Considering the candidate 293449_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293449_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293450_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293450_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293452_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293452_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293453_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293453_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:28:28.05 -01:46:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 5.787 3117534997152676096 097.11660672041 -01.77414040698 13.9213 13.4771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293474_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293474_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:55:58.74 -01:35:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.239 3112099187762874112 103.99454201873 -01.60068098726 13.8572 13.1918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293492_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293492_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293496_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293496_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:01:39.21 -03:36:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 5.640 3102604733060032000 105.41258550099 -03.60657619637 13.4456 12.2851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293504_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293504_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293509_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293509_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293512_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293512_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:43:55.56 -05:03:59.4: 13.09 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:43:55.56 -05:03:59.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.09 +/- 0.07
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Considering the candidate 293516_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293516_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293521_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293521_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293544_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293544_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:42:30.94 -06:04:20.7: 13.36 +/- 0.09 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:42:30.94 -06:04:20.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.36 +/- 0.09
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Considering the candidate 293545_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293545_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:48:21.02 -03:11:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293547_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293547_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293548_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293548_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:06:14.81 -04:55:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 3.860 3101470827337246464 106.56132619080 -04.92539118273 13.9219 13.2405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293550_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293550_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:39:08.68 -03:48:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.462 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293553_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293553_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:51:34.27 -01:39:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293556_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293556_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293564_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293564_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:24:33.47 -01:26:13.3: 12.77 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:24:33.47 -01:26:13.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.77 +/- 0.07
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Considering the candidate 293567_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293567_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293621_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293621_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293626_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293626_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:46:57.59 -02:12:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 4.672 3106176389201065728 101.73968461197 -02.20840746904 13.9082 12.8701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293630_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293630_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:30:03.04 +01:18:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 3.870 3120812576892619648 097.51252210072 +01.30787912936 13.6852 12.9897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293633_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293633_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:53:41.45 -00:33:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.582 3112503842401083904 103.42233870049 -00.56409058978 14.0403 13.7266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293644_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293644_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:35:42.03 +03:11:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.618 3130161170208610688 098.92490276050 +03.18629758406 13.7622 13.1813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293651_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293651_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293661_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293661_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293665_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293665_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:43:37.10 -04:25:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293677_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293677_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:28:51.03 +03:09:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293679_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293679_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:46:50.58 +01:18:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.117 3125737976669232256 101.71061901697 +01.30128313633 13.9023 13.1882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293683_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293683_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:54:59.54 -01:03:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.222 3112333791758054272 103.74773607348 -01.05207476769 13.3921 12.4083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293693_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293693_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293708_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293708_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:01:47.16 -01:24:50.4: 13.25 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:01:47.16 -01:24:50.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.25 +/- 0.08
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Considering the candidate 293717_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293717_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:19:27.43 -01:40:46.4: 12.57 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:19:27.43 -01:40:46.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.57 +/- 0.05
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Considering the candidate 293745_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293745_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:36:32.37 -03:35:55.2: 12.93 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:36:32.37 -03:35:55.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.93 +/- 0.06
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Considering the candidate 293757_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293757_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:11:01.90 +00:03:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.948 3111202810908018432 107.75743753981 +00.06395802188 13.6799 13.2216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293770_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293770_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293794_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293794_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293796_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293796_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:06:37.20 -04:38:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.200 3101496459701712640 106.65476195883 -04.63532880131 13.6813 13.0848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293827_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293827_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293829_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293829_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:35:10.45 -00:43:21.1: 13.52 +/- 0.11 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:35:10.45 -00:43:21.1: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.52 +/- 0.11
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Considering the candidate 293848_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293848_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:04:05.02 -02:22:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.476 3108833221613004800 106.02064200889 -02.37978674497 13.9010 13.5534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293886_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293886_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293887_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293887_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:59:49.90 -06:00:35.5: 12.69 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:59:49.90 -06:00:35.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.69 +/- 0.06
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Considering the candidate 293914_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293914_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293945_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293945_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 293957_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 293957_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:52:27.35 -05:52:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293979_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 293979_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294006_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294006_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:46:58.42 +01:29:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.506 3125767182446332672 101.74323261975 +01.48735629924 14.0034 13.4904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294008_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294008_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294020_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294020_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 07:02:32.41 -00:13:10.3: 12.60 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 07:02:32.41 -00:13:10.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.60 +/- 0.04
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Considering the candidate 294053_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294053_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294094_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294094_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294108_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294108_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294114_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294114_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:50:36.99 -01:46:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294146_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294146_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:02:01.06 -00:33:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.702 3112656021682569600 105.50481814040 -00.56507854051 13.8943 13.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294173_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294173_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294174_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294174_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:03:39.67 -00:16:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.602 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294186_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294186_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294191_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294191_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294192_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294192_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:02:01.33 -00:36:15.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 294193_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294193_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294206_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294206_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:28:11.73 +01:54:29.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 294229_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294229_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:57:35.59 +01:13:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 4.081 3113913996123980800 104.39787524035 +01.23033451357 14.0646 13.7846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294241_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294241_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294242_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294242_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294262_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294262_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294269_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294269_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294283_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294283_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:03:46.91 -01:04:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.412 3109553199868724224 105.94499944489 -01.08113492279 14.0995 13.5489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294291_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294291_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:14:47.06 +01:57:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294296_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294296_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:38:53.46 -00:49:15.2: 13.36 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:38:53.46 -00:49:15.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.36 +/- 0.08
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Considering the candidate 294304_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294304_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:47:16.39 +00:24:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.114 3113526280838415360 101.81809096502 +00.41023256005 14.1704 13.5996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294307_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294307_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294362_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294362_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294373_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294373_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:32:57.43 -02:23:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.334 3117243768307728000 098.23916846949 -02.38794555937 14.2908 12.8599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294424_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294424_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:46:18.40 -02:26:01.3: 13.15 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:46:18.40 -02:26:01.3: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.15 +/- 0.06
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Considering the candidate 294493_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294493_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:37:05.68 +03:07:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 4.671 3130145334667135232 099.27333575975 +03.13107873566 14.1676 13.5769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294510_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294510_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:54:03.40 +02:06:11.7: 12.71 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:54:03.40 +02:06:11.7: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.71 +/- 0.05
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Considering the candidate 294514_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294514_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294558_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294558_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:57.55 -00:25:32.4: 12.91 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:57.55 -00:25:32.4: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.91 +/- 0.06
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Considering the candidate 294575_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294575_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294609_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294609_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:04:37.17 -00:12:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 2.648 3112719140521623424 106.15520020739 -00.20290985339 14.3165 13.7542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294626_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294626_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294632_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294632_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:39:10.95 +01:59:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294657_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294657_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294664_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294664_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:30:07.22 -02:39:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.417 3117217616247602048 097.52997534566 -02.66519300427 14.0065 13.4404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294712_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294712_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294729_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294729_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294752_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294752_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 294759_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294759_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294787_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294787_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294816_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294816_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:05:22.94 -02:34:18.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
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Considering the candidate 294826_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294826_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:54:21.50 +00:49:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.148 3113967223658900992 103.58919358203 +00.82223515243 14.0185 13.0309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294840_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294840_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294862_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294862_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 294941_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 294941_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:39:16.32 -02:19:47.2: 12.58 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:39:16.32 -02:19:47.2: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 12.58 +/- 0.04
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Considering the candidate 294974_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 294974_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 295000_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 295000_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 295003_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 295003_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:44:38.22 -02:01:18.5: 13.55 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:44:38.22 -02:01:18.5: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.55 +/- 0.10
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Considering the candidate 295021_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 295021_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:10:30.28 -02:04:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.859 3108448431201789056 107.62570513900 -02.08424527252 14.3357 13.5762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295022_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 295022_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:38:38.88 +01:56:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.772 3126723723203857536 099.66166226243 +01.94146807612 14.3399 13.7153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295047_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 295047_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 295053_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 295053_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 295059_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 295059_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 295074_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 295074_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:51:32.64 +03:04:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.384 3126543437655686784 102.88541336288 +03.06712667176 14.4822 13.9993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295080_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 295080_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 295085_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 295085_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:59:43.68 -02:37:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 4.111 3108906996270577408 104.93142633250 -02.63195994644 14.3673 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295089_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 295089_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 295097_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 295097_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 295120_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 295120_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 295133_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 295133_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 295169_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 295169_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:56:18.90 -01:29:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.906 3112107537179160576 104.07850173421 -01.49152845560 14.5073 13.6510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295193_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 295193_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:46:27.13 -01:10:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.449 3107158321806080256 101.61235032124 -01.18301329268 14.2770 13.1905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295196_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 295196_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:05:42.67 -00:34:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.874 3109686683154789760 106.42698614471 -00.57206031659 14.5432 13.7302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295206_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 295206_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits at 06:48:29.06 +02:23:58.0: 13.21 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits at 06:48:29.06 +02:23:58.0: 99.00 +/- 99.00 edge
Forced photometry reference-image weighted average: 13.21 +/- 0.08
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Considering the candidate 295222_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 295222_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
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Considering the candidate 295225_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 295225_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295231_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
Preparing report for the candidate 295231_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09353_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 09353_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:03:53.11 -06:53:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129229_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 129229_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:19:38.79 -02:00:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 246364_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:17:31.09 +01:05:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 121122_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:09:13.70 -02:21:30.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65114_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 65114_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:27:01.31 -04:35:41.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228912_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 228912_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 06:50:00.74 +01:46:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 2.168 3126143833899577984 102.50251175252 +01.77583767395 10.7644 9.3430 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024
The candidate 199360_fd_Mon-02-Q1b1x1_2026-04-21_21-48-00_20.00sec_-4.90C_LIGHTs_0024 did not pass the final checks
**** FOUND 07:08:45.33 +00:41:48.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 15s
make_report_in_HTML.sh TOTAL: 522s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:42:47.89 +00:54:51.1
06:50:44.10 +02:07:58.8
06:54:46.98 -00:19:00.4
07:01:27.97 -01:55:22.4
06:44:49.32 +00:56:57.0
06:54:45.18 +00:31:42.1
06:50:18.58 -02:39:12.8
07:05:41.85 +00:52:59.6
07:07:15.65 +02:10:16.5
06:48:43.92 -01:08:00.6
07:06:19.07 +01:07:44.0
07:02:21.27 -00:52:48.4
06:44:14.43 +00:14:39.1
06:58:51.85 +02:39:10.6
07:03:28.03 -02:23:33.0
07:11:04.84 +01:22:10.1
06:51:10.24 -02:40:54.9
07:05:19.87 -03:25:08.8
07:10:54.83 -04:19:14.2
06:48:23.40 -02:03:32.1
07:08:47.34 -00:37:50.4
06:41:26.71 +02:47:59.4
06:54:39.89 +01:28:19.3
06:50:34.33 -01:55:04.8
06:58:53.75 +01:26:59.9
06:46:20.75 +02:44:05.4
06:54:34.58 -00:15:47.7
07:01:04.13 -04:48:06.3
07:08:44.96 -01:27:55.0
06:59:42.31 -02:10:51.3
06:58:57.70 -01:46:05.7
07:08:17.23 -04:56:00.7
07:02:23.56 -01:34:41.4
07:01:41.15 +00:06:33.1
07:09:51.76 -03:51:26.7
07:21:05.85 +00:28:16.8
07:12:54.81 -06:36:46.4
06:41:58.53 +02:45:41.9
07:10:40.40 +01:18:15.9
06:53:46.16 -00:14:32.9
07:06:51.27 -02:03:50.2
07:15:39.63 -00:49:27.4
07:18:48.75 -01:43:46.8
07:11:13.37 -06:42:51.7
07:13:31.55 -03:31:14.3
07:13:11.35 -00:08:48.2
07:11:55.42 -04:52:53.2
07:05:20.10 -02:51:43.7
06:42:34.69 -00:18:24.7
06:47:08.81 -00:14:49.7
07:12:55.87 +02:30:42.5
07:12:17.08 -02:10:59.6
07:10:29.07 +01:45:55.0
06:37:16.16 +03:08:58.0
07:21:45.83 -00:10:00.7
07:03:11.50 +01:23:07.0
07:06:11.43 -02:51:26.0
07:09:59.80 +01:25:47.9
07:09:22.87 +01:06:33.4
06:57:55.21 -04:37:47.0
07:14:02.20 -01:05:37.5
06:51:10.58 +01:06:02.7
07:03:25.16 -05:00:41.6
06:46:13.93 +00:50:43.7
07:17:44.49 -01:00:25.8
07:07:24.36 +02:31:25.8
07:08:48.82 -03:43:07.6
06:47:18.07 +00:57:53.1
07:11:44.15 -02:16:15.2
07:14:12.70 -04:31:50.9
07:04:35.25 +02:44:55.5
06:35:07.51 -03:03:03.7
06:59:30.41 +00:22:08.5
07:13:32.85 +00:13:15.9
06:43:52.81 +01:17:52.0
06:53:55.11 +02:25:33.1
06:58:57.06 -03:00:41.3
07:10:56.81 -04:18:47.7
07:04:22.03 -05:00:12.5
07:18:05.03 -01:25:38.0
07:06:54.73 -04:13:50.9
06:57:47.71 -01:31:06.6
06:50:49.70 -01:13:40.1
07:04:04.45 -04:33:46.2
07:04:15.81 -02:22:57.8
07:06:21.62 -03:11:42.1
06:45:04.86 +02:50:46.6
06:54:34.45 -00:35:21.9
07:03:52.81 +00:49:49.1
07:06:44.66 -01:25:53.0
06:51:33.03 +00:27:11.7
07:15:44.02 -06:38:23.5
07:07:54.34 -01:34:49.4
07:04:10.78 -03:14:37.7
07:08:35.59 +01:46:44.6
06:58:08.42 -01:38:50.9
06:40:30.47 -01:04:41.8
06:44:27.28 +02:30:55.6
07:16:34.06 -05:05:58.8
07:17:39.14 -03:44:20.4
07:05:08.67 -01:31:32.2
07:01:19.14 -03:06:44.5
07:03:47.20 -03:20:28.7
07:19:20.29 -00:18:57.8
06:44:33.37 -01:39:38.0
07:04:54.49 +00:11:36.7
07:13:04.82 -05:12:25.0
06:57:11.89 -03:58:11.9
07:05:12.13 -03:19:36.1
06:56:45.22 +00:46:34.7
07:15:57.87 -01:33:34.6
06:34:11.01 -00:21:48.1
06:49:33.18 -01:23:30.6
07:07:11.27 -02:58:19.6
06:40:18.01 +00:18:22.2
07:18:50.15 -05:15:16.1
07:04:34.96 -05:56:28.7
06:44:31.61 +00:07:34.9
07:10:37.59 -04:15:16.7
07:05:14.48 +00:02:11.1
07:20:50.47 -00:51:22.9
07:07:06.96 +01:40:01.4
06:43:50.92 +01:35:54.7
06:40:25.65 +00:56:10.4
06:58:49.25 -01:06:25.7
07:01:10.31 +00:00:19.8
07:07:33.28 -03:25:30.2
07:14:45.40 -01:22:48.0
07:15:26.09 -01:11:22.4
06:43:51.57 +02:08:02.0
06:59:40.39 -00:39:46.1
06:54:15.99 -00:38:32.4
07:01:49.13 -03:26:18.3
07:17:38.21 -05:59:16.4
07:09:38.12 +00:33:56.3
06:59:33.92 -01:45:36.8
07:12:11.46 -02:24:18.5
06:56:49.08 +00:46:31.9
06:43:47.33 +01:14:22.1
07:03:36.79 +02:37:09.4
06:49:56.15 -02:40:54.4
07:03:04.50 -01:18:36.8
06:49:53.06 +02:30:13.8
07:17:41.28 +00:07:01.5
07:19:55.70 -00:15:42.1
07:21:06.34 -03:15:03.8
07:11:45.32 -05:40:07.9
07:04:10.39 -03:43:26.5
06:55:03.24 -01:02:49.4
07:07:00.71 -00:52:19.9
07:01:42.98 -06:22:07.2
07:10:02.75 -02:32:02.1
07:04:16.78 -03:01:36.9
06:58:03.74 -00:47:07.7
06:42:44.33 +01:39:57.4
06:54:43.78 -02:41:19.4
07:01:22.76 -05:01:09.1
06:57:12.28 -03:57:43.6
07:13:29.25 -03:39:20.6
07:08:30.77 +01:18:17.8
06:20:54.16 -03:20:44.0
07:14:03.49 -00:18:23.3
06:45:39.07 +02:45:23.2
06:54:39.48 +02:38:02.2
07:05:20.28 +02:45:52.5
07:21:25.31 -03:35:02.6
07:04:51.59 -02:12:03.8
06:51:18.29 -01:23:07.0
07:08:04.47 -01:43:39.9
06:44:56.78 +01:18:45.2
06:50:59.49 +00:13:41.2
06:37:33.36 +01:24:38.3
06:54:59.82 +00:10:52.0
06:37:27.06 -02:40:37.8
06:28:32.48 -00:56:46.0
06:46:45.89 -00:18:52.0
06:49:07.30 -01:40:16.7
06:47:23.74 +01:25:44.4
06:35:47.89 +00:35:26.6
06:25:54.91 -00:53:16.5
06:59:45.84 -03:24:18.8
06:43:45.74 +00:35:16.0
07:08:43.12 +01:18:06.7
07:07:40.48 -03:15:05.8
06:45:33.69 -00:26:17.2
06:50:49.64 +02:42:35.2
06:50:09.69 -03:29:03.2
06:44:50.75 +01:05:47.0
06:47:41.10 +00:31:32.3
06:38:52.44 +01:12:25.3
07:09:21.65 +01:07:26.5
06:53:02.86 +01:17:30.2
07:20:48.79 -00:38:29.4
06:40:19.45 +00:59:57.5
07:03:16.47 -02:05:55.1
07:06:54.21 +02:10:49.3
07:04:11.58 -04:39:48.8
06:50:34.27 -02:44:32.3
07:17:47.06 -06:57:41.9
06:47:10.25 +02:54:03.4
06:51:11.56 -02:22:08.7
06:58:42.35 -04:00:08.5
06:55:11.83 +00:56:25.3
06:47:19.81 +01:08:22.4
06:45:17.60 +00:43:39.8
06:30:04.32 +01:18:38.3
06:49:09.00 -01:39:01.6
06:43:05.05 -02:53:58.0
06:51:28.37 -00:06:29.0
07:20:51.30 -01:01:32.3
06:35:00.97 -02:07:00.6
07:01:56.30 -04:37:28.1
07:21:14.17 +01:37:58.6
06:57:16.81 -02:44:41.2
06:55:15.83 +01:54:59.5
06:42:59.41 +00:50:08.3
07:18:56.81 -01:17:53.1
07:01:59.53 +00:49:51.0
06:44:27.84 +03:07:19.1
06:44:36.42 -00:34:42.3
06:47:07.42 +01:46:46.4
06:46:21.39 +02:10:55.9
07:08:00.99 -01:31:56.9
06:45:46.33 +01:57:40.7
06:52:07.48 +01:07:57.9
06:39:39.98 +00:06:19.3
########### Completed Mon-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:42:47.89 +00:54:51.1
06:50:44.10 +02:07:58.8
06:54:46.98 -00:19:00.4
07:01:27.97 -01:55:22.4
06:44:49.32 +00:56:57.0
06:54:45.18 +00:31:42.1
06:50:18.58 -02:39:12.8
07:05:41.85 +00:52:59.6
07:07:15.65 +02:10:16.5
06:48:43.92 -01:08:00.6
07:06:19.07 +01:07:44.0
07:02:21.27 -00:52:48.4
06:44:14.43 +00:14:39.1
06:58:51.85 +02:39:10.6
07:03:28.03 -02:23:33.0
07:11:04.84 +01:22:10.1
06:51:10.24 -02:40:54.9
07:05:19.87 -03:25:08.8
07:10:54.83 -04:19:14.2
06:48:23.40 -02:03:32.1
07:08:47.34 -00:37:50.4
06:41:26.71 +02:47:59.4
06:54:39.89 +01:28:19.3
06:50:34.33 -01:55:04.8
06:58:53.75 +01:26:59.9
06:46:20.75 +02:44:05.4
06:54:34.58 -00:15:47.7
07:01:04.13 -04:48:06.3
07:08:44.96 -01:27:55.0
06:59:42.31 -02:10:51.3
06:58:57.70 -01:46:05.7
07:08:17.23 -04:56:00.7
07:02:23.56 -01:34:41.4
07:01:41.15 +00:06:33.1
07:09:51.76 -03:51:26.7
07:21:05.85 +00:28:16.8
07:12:54.81 -06:36:46.4
06:41:58.53 +02:45:41.9
07:10:40.40 +01:18:15.9
06:53:46.16 -00:14:32.9
07:06:51.27 -02:03:50.2
07:15:39.63 -00:49:27.4
07:18:48.75 -01:43:46.8
07:11:13.37 -06:42:51.7
07:13:31.55 -03:31:14.3
07:13:11.35 -00:08:48.2
07:11:55.42 -04:52:53.2
07:05:20.10 -02:51:43.7
06:42:34.69 -00:18:24.7
06:47:08.81 -00:14:49.7
07:12:55.87 +02:30:42.5
07:12:17.08 -02:10:59.6
07:10:29.07 +01:45:55.0
06:37:16.16 +03:08:58.0
07:21:45.83 -00:10:00.7
07:03:11.50 +01:23:07.0
07:06:11.43 -02:51:26.0
07:09:59.80 +01:25:47.9
07:09:22.87 +01:06:33.4
06:57:55.21 -04:37:47.0
07:14:02.20 -01:05:37.5
06:51:10.58 +01:06:02.7
07:03:25.16 -05:00:41.6
06:46:13.93 +00:50:43.7
07:17:44.49 -01:00:25.8
07:07:24.36 +02:31:25.8
07:08:48.82 -03:43:07.6
06:47:18.07 +00:57:53.1
07:11:44.15 -02:16:15.2
07:14:12.70 -04:31:50.9
07:04:35.25 +02:44:55.5
06:35:07.51 -03:03:03.7
06:59:30.41 +00:22:08.5
07:13:32.85 +00:13:15.9
06:43:52.81 +01:17:52.0
06:53:55.11 +02:25:33.1
06:58:57.06 -03:00:41.3
07:10:56.81 -04:18:47.7
07:04:22.03 -05:00:12.5
07:18:05.03 -01:25:38.0
07:06:54.73 -04:13:50.9
06:57:47.71 -01:31:06.6
06:50:49.70 -01:13:40.1
07:04:04.45 -04:33:46.2
07:04:15.81 -02:22:57.8
07:06:21.62 -03:11:42.1
06:45:04.86 +02:50:46.6
06:54:34.45 -00:35:21.9
07:03:52.81 +00:49:49.1
07:06:44.66 -01:25:53.0
06:51:33.03 +00:27:11.7
07:15:44.02 -06:38:23.5
07:07:54.34 -01:34:49.4
07:04:10.78 -03:14:37.7
07:08:35.59 +01:46:44.6
06:58:08.42 -01:38:50.9
06:40:30.47 -01:04:41.8
06:44:27.28 +02:30:55.6
07:16:34.06 -05:05:58.8
07:17:39.14 -03:44:20.4
07:05:08.67 -01:31:32.2
07:01:19.14 -03:06:44.5
07:03:47.20 -03:20:28.7
07:19:20.29 -00:18:57.8
06:44:33.37 -01:39:38.0
07:04:54.49 +00:11:36.7
07:13:04.82 -05:12:25.0
06:57:11.89 -03:58:11.9
07:05:12.13 -03:19:36.1
06:56:45.22 +00:46:34.7
07:15:57.87 -01:33:34.6
06:34:11.01 -00:21:48.1
06:49:33.18 -01:23:30.6
07:07:11.27 -02:58:19.6
06:40:18.01 +00:18:22.2
07:18:50.15 -05:15:16.1
07:04:34.96 -05:56:28.7
06:44:31.61 +00:07:34.9
07:10:37.59 -04:15:16.7
07:05:14.48 +00:02:11.1
07:20:50.47 -00:51:22.9
07:07:06.96 +01:40:01.4
06:43:50.92 +01:35:54.7
06:40:25.65 +00:56:10.4
06:58:49.25 -01:06:25.7
07:01:10.31 +00:00:19.8
07:07:33.28 -03:25:30.2
07:14:45.40 -01:22:48.0
07:15:26.09 -01:11:22.4
06:43:51.57 +02:08:02.0
06:59:40.39 -00:39:46.1
06:54:15.99 -00:38:32.4
07:01:49.13 -03:26:18.3
07:17:38.21 -05:59:16.4
07:09:38.12 +00:33:56.3
06:59:33.92 -01:45:36.8
07:12:11.46 -02:24:18.5
06:56:49.08 +00:46:31.9
06:43:47.33 +01:14:22.1
07:03:36.79 +02:37:09.4
06:49:56.15 -02:40:54.4
07:03:04.50 -01:18:36.8
06:49:53.06 +02:30:13.8
07:17:41.28 +00:07:01.5
07:19:55.70 -00:15:42.1
07:21:06.34 -03:15:03.8
07:11:45.32 -05:40:07.9
07:04:10.39 -03:43:26.5
06:55:03.24 -01:02:49.4
07:07:00.71 -00:52:19.9
07:01:42.98 -06:22:07.2
07:10:02.75 -02:32:02.1
07:04:16.78 -03:01:36.9
06:58:03.74 -00:47:07.7
06:42:44.33 +01:39:57.4
06:54:43.78 -02:41:19.4
07:01:22.76 -05:01:09.1
06:57:12.28 -03:57:43.6
07:13:29.25 -03:39:20.6
07:08:30.77 +01:18:17.8
06:20:54.16 -03:20:44.0
07:14:03.49 -00:18:23.3
06:45:39.07 +02:45:23.2
06:54:39.48 +02:38:02.2
07:05:20.28 +02:45:52.5
07:21:25.31 -03:35:02.6
07:04:51.59 -02:12:03.8
06:51:18.29 -01:23:07.0
07:08:04.47 -01:43:39.9
06:44:56.78 +01:18:45.2
06:50:59.49 +00:13:41.2
06:37:33.36 +01:24:38.3
06:54:59.82 +00:10:52.0
06:37:27.06 -02:40:37.8
06:28:32.48 -00:56:46.0
06:46:45.89 -00:18:52.0
06:49:07.30 -01:40:16.7
06:47:23.74 +01:25:44.4
06:35:47.89 +00:35:26.6
06:25:54.91 -00:53:16.5
06:59:45.84 -03:24:18.8
06:43:45.74 +00:35:16.0
07:08:43.12 +01:18:06.7
07:07:40.48 -03:15:05.8
06:45:33.69 -00:26:17.2
06:50:49.64 +02:42:35.2
06:50:09.69 -03:29:03.2
06:44:50.75 +01:05:47.0
06:47:41.10 +00:31:32.3
06:38:52.44 +01:12:25.3
07:09:21.65 +01:07:26.5
06:53:02.86 +01:17:30.2
07:20:48.79 -00:38:29.4
06:40:19.45 +00:59:57.5
07:03:16.47 -02:05:55.1
07:06:54.21 +02:10:49.3
07:04:11.58 -04:39:48.8
06:50:34.27 -02:44:32.3
07:17:47.06 -06:57:41.9
06:47:10.25 +02:54:03.4
06:51:11.56 -02:22:08.7
06:58:42.35 -04:00:08.5
06:55:11.83 +00:56:25.3
06:47:19.81 +01:08:22.4
06:45:17.60 +00:43:39.8
06:30:04.32 +01:18:38.3
06:49:09.00 -01:39:01.6
06:43:05.05 -02:53:58.0
06:51:28.37 -00:06:29.0
07:20:51.30 -01:01:32.3
06:35:00.97 -02:07:00.6
07:01:56.30 -04:37:28.1
07:21:14.17 +01:37:58.6
06:57:16.81 -02:44:41.2
06:55:15.83 +01:54:59.5
06:42:59.41 +00:50:08.3
07:18:56.81 -01:17:53.1
07:01:59.53 +00:49:51.0
06:44:27.84 +03:07:19.1
06:44:36.42 -00:34:42.3
06:47:07.42 +01:46:46.4
06:46:21.39 +02:10:55.9
07:08:00.99 -01:31:56.9
06:45:46.33 +01:57:40.7
06:52:07.48 +01:07:57.9
06:39:39.98 +00:06:19.3
###################################################################################
06:42:47.89 +00:54:51.1 -- not an asteroid (will add it to exclusion list)
06:50:44.10 +02:07:58.8 -- not an asteroid (will add it to exclusion list)
06:54:46.98 -00:19:00.4 -- not an asteroid (will add it to exclusion list)
07:01:27.97 -01:55:22.4 -- not an asteroid (will add it to exclusion list)
06:44:49.32 +00:56:57.0 -- not an asteroid (will add it to exclusion list)
06:54:45.18 +00:31:42.1 -- not an asteroid (will add it to exclusion list)
06:50:18.58 -02:39:12.8 -- not an asteroid (will add it to exclusion list)
07:05:41.85 +00:52:59.6 -- not an asteroid (will add it to exclusion list)
07:07:15.65 +02:10:16.5 -- not an asteroid (will add it to exclusion list)
06:48:43.92 -01:08:00.6 -- not an asteroid (will add it to exclusion list)
07:06:19.07 +01:07:44.0 -- not an asteroid (will add it to exclusion list)
07:02:21.27 -00:52:48.4 -- not an asteroid (will add it to exclusion list)
06:44:14.43 +00:14:39.1 -- not an asteroid (will add it to exclusion list)
06:58:51.85 +02:39:10.6 -- not an asteroid (will add it to exclusion list)
07:03:28.03 -02:23:33.0 -- not an asteroid (will add it to exclusion list)
07:11:04.84 +01:22:10.1 -- not an asteroid (will add it to exclusion list)
06:51:10.24 -02:40:54.9 -- not an asteroid (will add it to exclusion list)
07:05:19.87 -03:25:08.8 -- not an asteroid (will add it to exclusion list)
07:10:54.83 -04:19:14.2 -- not an asteroid (will add it to exclusion list)
06:48:23.40 -02:03:32.1 -- not an asteroid (will add it to exclusion list)
07:08:47.34 -00:37:50.4 -- not an asteroid (will add it to exclusion list)
06:41:26.71 +02:47:59.4 -- not an asteroid (will add it to exclusion list)
06:54:39.89 +01:28:19.3 -- not an asteroid (will add it to exclusion list)
06:50:34.33 -01:55:04.8 -- not an asteroid (will add it to exclusion list)
06:58:53.75 +01:26:59.9 -- not an asteroid (will add it to exclusion list)
06:46:20.75 +02:44:05.4 -- not an asteroid (will add it to exclusion list)
06:54:34.58 -00:15:47.7 -- not an asteroid (will add it to exclusion list)
07:01:04.13 -04:48:06.3 -- not an asteroid (will add it to exclusion list)
07:08:44.96 -01:27:55.0 -- not an asteroid (will add it to exclusion list)
06:59:42.31 -02:10:51.3 -- not an asteroid (will add it to exclusion list)
06:58:57.70 -01:46:05.7 -- not an asteroid (will add it to exclusion list)
07:08:17.23 -04:56:00.7 -- not an asteroid (will add it to exclusion list)
07:02:23.56 -01:34:41.4 -- not an asteroid (will add it to exclusion list)
07:01:41.15 +00:06:33.1 -- not an asteroid (will add it to exclusion list)
07:09:51.76 -03:51:26.7 -- not an asteroid (will add it to exclusion list)
07:21:05.85 +00:28:16.8 -- not an asteroid (will add it to exclusion list)
07:12:54.81 -06:36:46.4 -- not an asteroid (will add it to exclusion list)
06:41:58.53 +02:45:41.9 -- not an asteroid (will add it to exclusion list)
07:10:40.40 +01:18:15.9 -- not an asteroid (will add it to exclusion list)
06:53:46.16 -00:14:32.9 -- not an asteroid (will add it to exclusion list)
07:06:51.27 -02:03:50.2 -- not an asteroid (will add it to exclusion list)
07:15:39.63 -00:49:27.4 -- not an asteroid (will add it to exclusion list)
07:18:48.75 -01:43:46.8 -- not an asteroid (will add it to exclusion list)
07:11:13.37 -06:42:51.7 -- not an asteroid (will add it to exclusion list)
07:13:31.55 -03:31:14.3 -- not an asteroid (will add it to exclusion list)
07:13:11.35 -00:08:48.2 -- not an asteroid (will add it to exclusion list)
07:11:55.42 -04:52:53.2 -- not an asteroid (will add it to exclusion list)
07:05:20.10 -02:51:43.7 -- not an asteroid (will add it to exclusion list)
06:42:34.69 -00:18:24.7 -- not an asteroid (will add it to exclusion list)
06:47:08.81 -00:14:49.7 -- not an asteroid (will add it to exclusion list)
07:12:55.87 +02:30:42.5 -- not an asteroid (will add it to exclusion list)
07:12:17.08 -02:10:59.6 -- not an asteroid (will add it to exclusion list)
07:10:29.07 +01:45:55.0 -- not an asteroid (will add it to exclusion list)
06:37:16.16 +03:08:58.0 -- not an asteroid (will add it to exclusion list)
07:21:45.83 -00:10:00.7 -- not an asteroid (will add it to exclusion list)
07:03:11.50 +01:23:07.0 -- not an asteroid (will add it to exclusion list)
07:06:11.43 -02:51:26.0 -- not an asteroid (will add it to exclusion list)
07:09:59.80 +01:25:47.9 -- not an asteroid (will add it to exclusion list)
07:09:22.87 +01:06:33.4 -- not an asteroid (will add it to exclusion list)
06:57:55.21 -04:37:47.0 -- not an asteroid (will add it to exclusion list)
07:14:02.20 -01:05:37.5 -- not an asteroid (will add it to exclusion list)
06:51:10.58 +01:06:02.7 -- not an asteroid (will add it to exclusion list)
07:03:25.16 -05:00:41.6 -- not an asteroid (will add it to exclusion list)
06:46:13.93 +00:50:43.7 -- not an asteroid (will add it to exclusion list)
07:17:44.49 -01:00:25.8 -- not an asteroid (will add it to exclusion list)
07:07:24.36 +02:31:25.8 -- not an asteroid (will add it to exclusion list)
07:08:48.82 -03:43:07.6 -- not an asteroid (will add it to exclusion list)
06:47:18.07 +00:57:53.1 -- not an asteroid (will add it to exclusion list)
07:11:44.15 -02:16:15.2 -- not an asteroid (will add it to exclusion list)
07:14:12.70 -04:31:50.9 -- not an asteroid (will add it to exclusion list)
07:04:35.25 +02:44:55.5 -- not an asteroid (will add it to exclusion list)
06:35:07.51 -03:03:03.7 -- not an asteroid (will add it to exclusion list)
06:59:30.41 +00:22:08.5 -- not an asteroid (will add it to exclusion list)
07:13:32.85 +00:13:15.9 -- not an asteroid (will add it to exclusion list)
06:43:52.81 +01:17:52.0 -- not an asteroid (will add it to exclusion list)
06:53:55.11 +02:25:33.1 -- not an asteroid (will add it to exclusion list)
06:58:57.06 -03:00:41.3 -- not an asteroid (will add it to exclusion list)
07:10:56.81 -04:18:47.7 -- not an asteroid (will add it to exclusion list)
07:04:22.03 -05:00:12.5 -- not an asteroid (will add it to exclusion list)
07:18:05.03 -01:25:38.0 -- not an asteroid (will add it to exclusion list)
07:06:54.73 -04:13:50.9 -- not an asteroid (will add it to exclusion list)
06:57:47.71 -01:31:06.6 -- not an asteroid (will add it to exclusion list)
06:50:49.70 -01:13:40.1 -- not an asteroid (will add it to exclusion list)
07:04:04.45 -04:33:46.2 -- not an asteroid (will add it to exclusion list)
07:04:15.81 -02:22:57.8 -- not an asteroid (will add it to exclusion list)
07:06:21.62 -03:11:42.1 -- not an asteroid (will add it to exclusion list)
06:45:04.86 +02:50:46.6 -- not an asteroid (will add it to exclusion list)
06:54:34.45 -00:35:21.9 -- not an asteroid (will add it to exclusion list)
07:03:52.81 +00:49:49.1 -- not an asteroid (will add it to exclusion list)
07:06:44.66 -01:25:53.0 -- not an asteroid (will add it to exclusion list)
06:51:33.03 +00:27:11.7 -- not an asteroid (will add it to exclusion list)
07:15:44.02 -06:38:23.5 -- not an asteroid (will add it to exclusion list)
07:07:54.34 -01:34:49.4 -- not an asteroid (will add it to exclusion list)
07:04:10.78 -03:14:37.7 -- not an asteroid (will add it to exclusion list)
07:08:35.59 +01:46:44.6 -- not an asteroid (will add it to exclusion list)
06:58:08.42 -01:38:50.9 -- not an asteroid (will add it to exclusion list)
06:40:30.47 -01:04:41.8 -- not an asteroid (will add it to exclusion list)
06:44:27.28 +02:30:55.6 -- not an asteroid (will add it to exclusion list)
07:16:34.06 -05:05:58.8 -- not an asteroid (will add it to exclusion list)
07:17:39.14 -03:44:20.4 -- not an asteroid (will add it to exclusion list)
07:05:08.67 -01:31:32.2 -- not an asteroid (will add it to exclusion list)
07:01:19.14 -03:06:44.5 -- not an asteroid (will add it to exclusion list)
07:03:47.20 -03:20:28.7 -- not an asteroid (will add it to exclusion list)
07:19:20.29 -00:18:57.8 -- not an asteroid (will add it to exclusion list)
06:44:33.37 -01:39:38.0 -- not an asteroid (will add it to exclusion list)
07:04:54.49 +00:11:36.7 -- not an asteroid (will add it to exclusion list)
07:13:04.82 -05:12:25.0 -- not an asteroid (will add it to exclusion list)
06:57:11.89 -03:58:11.9 -- not an asteroid (will add it to exclusion list)
07:05:12.13 -03:19:36.1 -- not an asteroid (will add it to exclusion list)
06:56:45.22 +00:46:34.7 -- not an asteroid (will add it to exclusion list)
07:15:57.87 -01:33:34.6 -- not an asteroid (will add it to exclusion list)
06:34:11.01 -00:21:48.1 -- not an asteroid (will add it to exclusion list)
06:49:33.18 -01:23:30.6 -- not an asteroid (will add it to exclusion list)
07:07:11.27 -02:58:19.6 -- not an asteroid (will add it to exclusion list)
06:40:18.01 +00:18:22.2 -- not an asteroid (will add it to exclusion list)
07:18:50.15 -05:15:16.1 -- not an asteroid (will add it to exclusion list)
07:04:34.96 -05:56:28.7 -- not an asteroid (will add it to exclusion list)
06:44:31.61 +00:07:34.9 -- not an asteroid (will add it to exclusion list)
07:10:37.59 -04:15:16.7 -- not an asteroid (will add it to exclusion list)
07:05:14.48 +00:02:11.1 -- not an asteroid (will add it to exclusion list)
07:20:50.47 -00:51:22.9 -- not an asteroid (will add it to exclusion list)
07:07:06.96 +01:40:01.4 -- not an asteroid (will add it to exclusion list)
06:43:50.92 +01:35:54.7 -- not an asteroid (will add it to exclusion list)
06:40:25.65 +00:56:10.4 -- not an asteroid (will add it to exclusion list)
06:58:49.25 -01:06:25.7 -- not an asteroid (will add it to exclusion list)
07:01:10.31 +00:00:19.8 -- not an asteroid (will add it to exclusion list)
07:07:33.28 -03:25:30.2 -- not an asteroid (will add it to exclusion list)
07:14:45.40 -01:22:48.0 -- not an asteroid (will add it to exclusion list)
07:15:26.09 -01:11:22.4 -- not an asteroid (will add it to exclusion list)
06:43:51.57 +02:08:02.0 -- not an asteroid (will add it to exclusion list)
06:59:40.39 -00:39:46.1 -- not an asteroid (will add it to exclusion list)
06:54:15.99 -00:38:32.4 -- not an asteroid (will add it to exclusion list)
07:01:49.13 -03:26:18.3 -- not an asteroid (will add it to exclusion list)
07:17:38.21 -05:59:16.4 -- not an asteroid (will add it to exclusion list)
07:09:38.12 +00:33:56.3 -- not an asteroid (will add it to exclusion list)
06:59:33.92 -01:45:36.8 -- not an asteroid (will add it to exclusion list)
07:12:11.46 -02:24:18.5 -- not an asteroid (will add it to exclusion list)
06:56:49.08 +00:46:31.9 -- not an asteroid (will add it to exclusion list)
06:43:47.33 +01:14:22.1 -- not an asteroid (will add it to exclusion list)
07:03:36.79 +02:37:09.4 -- not an asteroid (will add it to exclusion list)
06:49:56.15 -02:40:54.4 -- not an asteroid (will add it to exclusion list)
07:03:04.50 -01:18:36.8 -- not an asteroid (will add it to exclusion list)
06:49:53.06 +02:30:13.8 -- not an asteroid (will add it to exclusion list)
07:17:41.28 +00:07:01.5 -- not an asteroid (will add it to exclusion list)
07:19:55.70 -00:15:42.1 -- not an asteroid (will add it to exclusion list)
07:21:06.34 -03:15:03.8 -- not an asteroid (will add it to exclusion list)
07:11:45.32 -05:40:07.9 -- not an asteroid (will add it to exclusion list)
07:04:10.39 -03:43:26.5 -- not an asteroid (will add it to exclusion list)
06:55:03.24 -01:02:49.4 -- not an asteroid (will add it to exclusion list)
07:07:00.71 -00:52:19.9 -- not an asteroid (will add it to exclusion list)
07:01:42.98 -06:22:07.2 -- not an asteroid (will add it to exclusion list)
07:10:02.75 -02:32:02.1 -- not an asteroid (will add it to exclusion list)
07:04:16.78 -03:01:36.9 -- not an asteroid (will add it to exclusion list)
06:58:03.74 -00:47:07.7 -- not an asteroid (will add it to exclusion list)
06:42:44.33 +01:39:57.4 -- not an asteroid (will add it to exclusion list)
06:54:43.78 -02:41:19.4 -- not an asteroid (will add it to exclusion list)
07:01:22.76 -05:01:09.1 -- not an asteroid (will add it to exclusion list)
06:57:12.28 -03:57:43.6 -- not an asteroid (will add it to exclusion list)
07:13:29.25 -03:39:20.6 -- not an asteroid (will add it to exclusion list)
07:08:30.77 +01:18:17.8 -- not an asteroid (will add it to exclusion list)
06:20:54.16 -03:20:44.0 -- not an asteroid (will add it to exclusion list)
07:14:03.49 -00:18:23.3 -- not an asteroid (will add it to exclusion list)
06:45:39.07 +02:45:23.2 -- not an asteroid (will add it to exclusion list)
06:54:39.48 +02:38:02.2 -- not an asteroid (will add it to exclusion list)
07:05:20.28 +02:45:52.5 -- not an asteroid (will add it to exclusion list)
07:21:25.31 -03:35:02.6 -- not an asteroid (will add it to exclusion list)
07:04:51.59 -02:12:03.8 -- not an asteroid (will add it to exclusion list)
06:51:18.29 -01:23:07.0 -- not an asteroid (will add it to exclusion list)
07:08:04.47 -01:43:39.9 -- not an asteroid (will add it to exclusion list)
06:44:56.78 +01:18:45.2 -- not an asteroid (will add it to exclusion list)
06:50:59.49 +00:13:41.2 -- not an asteroid (will add it to exclusion list)
06:37:33.36 +01:24:38.3 -- not an asteroid (will add it to exclusion list)
06:54:59.82 +00:10:52.0 -- not an asteroid (will add it to exclusion list)
06:37:27.06 -02:40:37.8 -- not an asteroid (will add it to exclusion list)
06:28:32.48 -00:56:46.0 -- not an asteroid (will add it to exclusion list)
06:46:45.89 -00:18:52.0 -- not an asteroid (will add it to exclusion list)
06:49:07.30 -01:40:16.7 -- not an asteroid (will add it to exclusion list)
06:47:23.74 +01:25:44.4 -- not an asteroid (will add it to exclusion list)
06:35:47.89 +00:35:26.6 -- not an asteroid (will add it to exclusion list)
06:25:54.91 -00:53:16.5 -- not an asteroid (will add it to exclusion list)
06:59:45.84 -03:24:18.8 -- not an asteroid (will add it to exclusion list)
06:43:45.74 +00:35:16.0 -- not an asteroid (will add it to exclusion list)
07:08:43.12 +01:18:06.7 -- not an asteroid (will add it to exclusion list)
07:07:40.48 -03:15:05.8 -- not an asteroid (will add it to exclusion list)
06:45:33.69 -00:26:17.2 -- not an asteroid (will add it to exclusion list)
06:50:49.64 +02:42:35.2 -- not an asteroid (will add it to exclusion list)
06:50:09.69 -03:29:03.2 -- not an asteroid (will add it to exclusion list)
06:44:50.75 +01:05:47.0 -- not an asteroid (will add it to exclusion list)
06:47:41.10 +00:31:32.3 -- not an asteroid (will add it to exclusion list)
06:38:52.44 +01:12:25.3 -- asteroid (will NOT add it to exclusion list)
07:09:21.65 +01:07:26.5 -- not an asteroid (will add it to exclusion list)
06:53:02.86 +01:17:30.2 -- not an asteroid (will add it to exclusion list)
07:20:48.79 -00:38:29.4 -- not an asteroid (will add it to exclusion list)
06:40:19.45 +00:59:57.5 -- not an asteroid (will add it to exclusion list)
07:03:16.47 -02:05:55.1 -- not an asteroid (will add it to exclusion list)
07:06:54.21 +02:10:49.3 -- not an asteroid (will add it to exclusion list)
07:04:11.58 -04:39:48.8 -- not an asteroid (will add it to exclusion list)
06:50:34.27 -02:44:32.3 -- not an asteroid (will add it to exclusion list)
07:17:47.06 -06:57:41.9 -- not an asteroid (will add it to exclusion list)
06:47:10.25 +02:54:03.4 -- not an asteroid (will add it to exclusion list)
06:51:11.56 -02:22:08.7 -- not an asteroid (will add it to exclusion list)
06:58:42.35 -04:00:08.5 -- not an asteroid (will add it to exclusion list)
06:55:11.83 +00:56:25.3 -- not an asteroid (will add it to exclusion list)
06:47:19.81 +01:08:22.4 -- not an asteroid (will add it to exclusion list)
06:45:17.60 +00:43:39.8 -- not an asteroid (will add it to exclusion list)
06:30:04.32 +01:18:38.3 -- not an asteroid (will add it to exclusion list)
06:49:09.00 -01:39:01.6 -- not an asteroid (will add it to exclusion list)
06:43:05.05 -02:53:58.0 -- not an asteroid (will add it to exclusion list)
06:51:28.37 -00:06:29.0 -- not an asteroid (will add it to exclusion list)
07:20:51.30 -01:01:32.3 -- not an asteroid (will add it to exclusion list)
06:35:00.97 -02:07:00.6 -- not an asteroid (will add it to exclusion list)
07:01:56.30 -04:37:28.1 -- not an asteroid (will add it to exclusion list)
07:21:14.17 +01:37:58.6 -- not an asteroid (will add it to exclusion list)
06:57:16.81 -02:44:41.2 -- not an asteroid (will add it to exclusion list)
06:55:15.83 +01:54:59.5 -- not an asteroid (will add it to exclusion list)
06:42:59.41 +00:50:08.3 -- not an asteroid (will add it to exclusion list)
07:18:56.81 -01:17:53.1 -- not an asteroid (will add it to exclusion list)
07:01:59.53 +00:49:51.0 -- not an asteroid (will add it to exclusion list)
06:44:27.84 +03:07:19.1 -- not an asteroid (will add it to exclusion list)
06:44:36.42 -00:34:42.3 -- not an asteroid (will add it to exclusion list)
06:47:07.42 +01:46:46.4 -- not an asteroid (will add it to exclusion list)
06:46:21.39 +02:10:55.9 -- not an asteroid (will add it to exclusion list)
07:08:00.99 -01:31:56.9 -- not an asteroid (will add it to exclusion list)
06:45:46.33 +01:57:40.7 -- not an asteroid (will add it to exclusion list)
06:52:07.48 +01:07:57.9 -- not an asteroid (will add it to exclusion list)
06:39:39.98 +00:06:19.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:20:54.16 -03:20:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:54.91 -00:53:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:32.48 -00:56:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:04.32 +01:18:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:11.01 -00:21:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:00.97 -02:07:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:07.51 -03:03:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:47.89 +00:35:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:16.16 +03:08:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:27.06 -02:40:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:33.36 +01:24:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:39.98 +00:06:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:18.01 +00:18:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:19.45 +00:59:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:25.65 +00:56:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:30.47 -01:04:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:26.71 +02:47:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:58.53 +02:45:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:34.69 -00:18:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:44.33 +01:39:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:47.89 +00:54:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:59.41 +00:50:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:05.05 -02:53:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:45.74 +00:35:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:47.33 +01:14:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:50.92 +01:35:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:51.57 +02:08:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:52.81 +01:17:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:14.43 +00:14:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:27.28 +02:30:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:27.84 +03:07:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:31.61 +00:07:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:33.37 -01:39:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:36.42 -00:34:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:49.32 +00:56:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:50.75 +01:05:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:56.78 +01:18:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:04.86 +02:50:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:17.60 +00:43:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:33.69 -00:26:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:39.07 +02:45:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:46.33 +01:57:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:13.93 +00:50:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:20.75 +02:44:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:21.39 +02:10:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:45.89 -00:18:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:07.42 +01:46:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:08.81 -00:14:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:10.25 +02:54:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:18.07 +00:57:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:19.81 +01:08:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:23.74 +01:25:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:41.10 +00:31:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:23.40 -02:03:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:43.92 -01:08:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.30 -01:40:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:09.00 -01:39:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:33.18 -01:23:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:53.06 +02:30:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.15 -02:40:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:09.69 -03:29:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:18.58 -02:39:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:34.27 -02:44:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:34.33 -01:55:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:44.10 +02:07:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:49.64 +02:42:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:49.70 -01:13:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:59.49 +00:13:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.24 -02:40:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.58 +01:06:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:11.56 -02:22:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:18.29 -01:23:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:28.37 -00:06:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:33.03 +00:27:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:07.48 +01:07:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:02.86 +01:17:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:46.16 -00:14:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:55.11 +02:25:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:15.99 -00:38:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:34.45 -00:35:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:34.58 -00:15:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:39.48 +02:38:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:39.89 +01:28:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:43.78 -02:41:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:45.18 +00:31:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:46.98 -00:19:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:59.82 +00:10:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:03.24 -01:02:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:11.83 +00:56:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:15.83 +01:54:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:45.22 +00:46:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:49.08 +00:46:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:11.89 -03:58:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:12.28 -03:57:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:16.81 -02:44:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:47.71 -01:31:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:55.21 -04:37:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:03.74 -00:47:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:08.42 -01:38:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:42.35 -04:00:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:49.25 -01:06:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:51.85 +02:39:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:53.75 +01:26:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:57.06 -03:00:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:57.70 -01:46:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:30.41 +00:22:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:33.92 -01:45:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:40.39 -00:39:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:42.31 -02:10:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:45.84 -03:24:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:04.13 -04:48:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:10.31 +00:00:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:19.14 -03:06:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:22.76 -05:01:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:27.97 -01:55:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:41.15 +00:06:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:42.98 -06:22:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:49.13 -03:26:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:56.30 -04:37:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:59.53 +00:49:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:21.27 -00:52:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:23.56 -01:34:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:04.50 -01:18:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:11.50 +01:23:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:16.47 -02:05:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:25.16 -05:00:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:28.03 -02:23:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:36.79 +02:37:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:47.20 -03:20:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:52.81 +00:49:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:04.45 -04:33:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:10.39 -03:43:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:10.78 -03:14:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:11.58 -04:39:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:15.81 -02:22:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.78 -03:01:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:22.03 -05:00:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:34.96 -05:56:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:35.25 +02:44:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:51.59 -02:12:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:54.49 +00:11:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:08.67 -01:31:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:12.13 -03:19:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:14.48 +00:02:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:19.87 -03:25:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:20.10 -02:51:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:20.28 +02:45:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:41.85 +00:52:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:11.43 -02:51:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:19.07 +01:07:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:21.62 -03:11:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:44.66 -01:25:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:51.27 -02:03:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:54.21 +02:10:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:54.73 -04:13:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:00.71 -00:52:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:06.96 +01:40:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:11.27 -02:58:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:15.65 +02:10:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:24.36 +02:31:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:33.28 -03:25:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:40.48 -03:15:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:54.34 -01:34:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:00.99 -01:31:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:04.47 -01:43:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:17.23 -04:56:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:30.77 +01:18:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:35.59 +01:46:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.12 +01:18:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:44.96 -01:27:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:47.34 -00:37:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:48.82 -03:43:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:21.65 +01:07:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:22.87 +01:06:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:38.12 +00:33:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:51.76 -03:51:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:59.80 +01:25:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:02.75 -02:32:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:29.07 +01:45:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:37.59 -04:15:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:40.40 +01:18:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:54.83 -04:19:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:56.81 -04:18:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:04.84 +01:22:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:13.37 -06:42:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:44.15 -02:16:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:45.32 -05:40:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:55.42 -04:52:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:11.46 -02:24:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:17.08 -02:10:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:54.81 -06:36:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:55.87 +02:30:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:04.82 -05:12:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:11.35 -00:08:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:29.25 -03:39:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:31.55 -03:31:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:32.85 +00:13:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:02.20 -01:05:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:03.49 -00:18:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:12.70 -04:31:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:45.40 -01:22:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:26.09 -01:11:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:39.63 -00:49:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:44.02 -06:38:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:57.87 -01:33:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:34.06 -05:05:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:38.21 -05:59:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:39.14 -03:44:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:41.28 +00:07:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:44.49 -01:00:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:47.06 -06:57:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:05.03 -01:25:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:48.75 -01:43:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:50.15 -05:15:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:56.81 -01:17:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:20.29 -00:18:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:55.70 -00:15:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:48.79 -00:38:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:50.47 -00:51:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:51.30 -01:01:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:05.85 +00:28:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:06.34 -03:15:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:14.17 +01:37:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:25.31 -03:35:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:45.83 -00:10:00.7 -- 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)
06:20:54.16 -03:20:44.0 -- not a known variable star
06:25:54.91 -00:53:16.5 -- not a known variable star
06:28:32.48 -00:56:46.0 -- not a known variable star
06:30:04.32 +01:18:38.3 -- a known variable star
06:34:11.01 -00:21:48.1 -- not a known variable star
06:35:00.97 -02:07:00.6 -- not a known variable star
06:35:07.51 -03:03:03.7 -- not a known variable star
06:35:47.89 +00:35:26.6 -- not a known variable star
06:37:16.16 +03:08:58.0 -- not a known variable star
06:37:27.06 -02:40:37.8 -- not a known variable star
06:37:33.36 +01:24:38.3 -- not a known variable star
06:39:39.98 +00:06:19.3 -- not a known variable star
06:40:18.01 +00:18:22.2 -- a known variable star
06:40:19.45 +00:59:57.5 -- not a known variable star
06:40:25.65 +00:56:10.4 -- not a known variable star
06:40:30.47 -01:04:41.8 -- a known variable star
06:41:26.71 +02:47:59.4 -- not a known variable star
06:41:58.53 +02:45:41.9 -- not a known variable star
06:42:34.69 -00:18:24.7 -- not a known variable star
06:42:44.33 +01:39:57.4 -- not a known variable star
06:42:47.89 +00:54:51.1 -- a known variable star
06:42:59.41 +00:50:08.3 -- not a known variable star
06:43:05.05 -02:53:58.0 -- a known variable star
06:43:45.74 +00:35:16.0 -- not a known variable star
06:43:47.33 +01:14:22.1 -- not a known variable star
06:43:50.92 +01:35:54.7 -- not a known variable star
06:43:51.57 +02:08:02.0 -- not a known variable star
06:43:52.81 +01:17:52.0 -- not a known variable star
06:44:14.43 +00:14:39.1 -- not a known variable star
06:44:27.28 +02:30:55.6 -- not a known variable star
06:44:27.84 +03:07:19.1 -- not a known variable star
06:44:31.61 +00:07:34.9 -- not a known variable star
06:44:33.37 -01:39:38.0 -- not a known variable star
06:44:36.42 -00:34:42.3 -- not a known variable star
06:44:49.32 +00:56:57.0 -- not a known variable star
06:44:50.75 +01:05:47.0 -- not a known variable star
06:44:56.78 +01:18:45.2 -- not a known variable star
06:45:04.86 +02:50:46.6 -- not a known variable star
06:45:17.60 +00:43:39.8 -- not a known variable star
06:45:33.69 -00:26:17.2 -- a known variable star
06:45:39.07 +02:45:23.2 -- a known variable star
06:45:46.33 +01:57:40.7 -- not a known variable star
06:46:13.93 +00:50:43.7 -- not a known variable star
06:46:20.75 +02:44:05.4 -- a known variable star
06:46:21.39 +02:10:55.9 -- not a known variable star
06:46:45.89 -00:18:52.0 -- not a known variable star
06:47:07.42 +01:46:46.4 -- not a known variable star
06:47:08.81 -00:14:49.7 -- not a known variable star
06:47:10.25 +02:54:03.4 -- not a known variable star
06:47:18.07 +00:57:53.1 -- not a known variable star
06:47:19.81 +01:08:22.4 -- not a known variable star
06:47:23.74 +01:25:44.4 -- a known variable star
06:47:41.10 +00:31:32.3 -- not a known variable star
06:48:23.40 -02:03:32.1 -- not a known variable star
06:48:43.92 -01:08:00.6 -- a known variable star
06:49:07.30 -01:40:16.7 -- not a known variable star
06:49:09.00 -01:39:01.6 -- not a known variable star
06:49:33.18 -01:23:30.6 -- not a known variable star
06:49:53.06 +02:30:13.8 -- a known variable star
06:49:56.15 -02:40:54.4 -- not a known variable star
06:50:09.69 -03:29:03.2 -- a known variable star
06:50:18.58 -02:39:12.8 -- not a known variable star
06:50:34.27 -02:44:32.3 -- not a known variable star
06:50:34.33 -01:55:04.8 -- not a known variable star
06:50:44.10 +02:07:58.8 -- not a known variable star
06:50:49.64 +02:42:35.2 -- not a known variable star
06:50:49.70 -01:13:40.1 -- not a known variable star
06:50:59.49 +00:13:41.2 -- not a known variable star
06:51:10.24 -02:40:54.9 -- not a known variable star
06:51:10.58 +01:06:02.7 -- not a known variable star
06:51:11.56 -02:22:08.7 -- not a known variable star
06:51:18.29 -01:23:07.0 -- a known variable star
06:51:28.37 -00:06:29.0 -- not a known variable star
06:51:33.03 +00:27:11.7 -- a known variable star
06:52:07.48 +01:07:57.9 -- not a known variable star
06:53:02.86 +01:17:30.2 -- a known variable star
06:53:46.16 -00:14:32.9 -- not a known variable star
06:53:55.11 +02:25:33.1 -- a known variable star
06:54:15.99 -00:38:32.4 -- not a known variable star
06:54:34.45 -00:35:21.9 -- not a known variable star
06:54:34.58 -00:15:47.7 -- a known variable star
06:54:39.48 +02:38:02.2 -- not a known variable star
06:54:39.89 +01:28:19.3 -- a known variable star
06:54:43.78 -02:41:19.4 -- not a known variable star
06:54:45.18 +00:31:42.1 -- not a known variable star
06:54:46.98 -00:19:00.4 -- a known variable star
06:54:59.82 +00:10:52.0 -- not a known variable star
06:55:03.24 -01:02:49.4 -- not a known variable star
06:55:11.83 +00:56:25.3 -- not a known variable star
06:55:15.83 +01:54:59.5 -- not a known variable star
06:56:45.22 +00:46:34.7 -- not a known variable star
06:56:49.08 +00:46:31.9 -- not a known variable star
06:57:11.89 -03:58:11.9 -- not a known variable star
06:57:12.28 -03:57:43.6 -- not a known variable star
06:57:16.81 -02:44:41.2 -- not a known variable star
06:57:47.71 -01:31:06.6 -- a known variable star
06:57:55.21 -04:37:47.0 -- a known variable star
06:58:03.74 -00:47:07.7 -- not a known variable star
06:58:08.42 -01:38:50.9 -- not a known variable star
06:58:42.35 -04:00:08.5 -- not a known variable star
06:58:49.25 -01:06:25.7 -- a known variable star
06:58:51.85 +02:39:10.6 -- not a known variable star
06:58:53.75 +01:26:59.9 -- a known variable star
06:58:57.06 -03:00:41.3 -- not a known variable star
06:58:57.70 -01:46:05.7 -- not a known variable star
06:59:30.41 +00:22:08.5 -- not a known variable star
06:59:33.92 -01:45:36.8 -- not a known variable star
06:59:40.39 -00:39:46.1 -- not a known variable star
06:59:42.31 -02:10:51.3 -- a known variable star
06:59:45.84 -03:24:18.8 -- not a known variable star
07:01:04.13 -04:48:06.3 -- a known variable star
07:01:10.31 +00:00:19.8 -- a known variable star
07:01:19.14 -03:06:44.5 -- not a known variable star
07:01:22.76 -05:01:09.1 -- not a known variable star
07:01:27.97 -01:55:22.4 -- not a known variable star
07:01:41.15 +00:06:33.1 -- a known variable star
07:01:42.98 -06:22:07.2 -- a known variable star
07:01:49.13 -03:26:18.3 -- not a known variable star
07:01:56.30 -04:37:28.1 -- not a known variable star
07:01:59.53 +00:49:51.0 -- not a known variable star
07:02:21.27 -00:52:48.4 -- not a known variable star
07:02:23.56 -01:34:41.4 -- not a known variable star
07:03:04.50 -01:18:36.8 -- not a known variable star
07:03:11.50 +01:23:07.0 -- a known variable star
07:03:16.47 -02:05:55.1 -- not a known variable star
07:03:25.16 -05:00:41.6 -- a known variable star
07:03:28.03 -02:23:33.0 -- not a known variable star
07:03:36.79 +02:37:09.4 -- a known variable star
07:03:47.20 -03:20:28.7 -- not a known variable star
07:03:52.81 +00:49:49.1 -- not a known variable star
07:04:04.45 -04:33:46.2 -- not a known variable star
07:04:10.39 -03:43:26.5 -- not a known variable star
07:04:10.78 -03:14:37.7 -- not a known variable star
07:04:11.58 -04:39:48.8 -- not a known variable star
07:04:15.81 -02:22:57.8 -- not a known variable star
07:04:16.78 -03:01:36.9 -- not a known variable star
07:04:22.03 -05:00:12.5 -- not a known variable star
07:04:34.96 -05:56:28.7 -- a known variable star
07:04:35.25 +02:44:55.5 -- a known variable star
07:04:51.59 -02:12:03.8 -- not a known variable star
07:04:54.49 +00:11:36.7 -- not a known variable star
07:05:08.67 -01:31:32.2 -- not a known variable star
07:05:12.13 -03:19:36.1 -- not a known variable star
07:05:14.48 +00:02:11.1 -- not a known variable star
07:05:19.87 -03:25:08.8 -- a known variable star
07:05:20.10 -02:51:43.7 -- a known variable star
07:05:20.28 +02:45:52.5 -- not a known variable star
07:05:41.85 +00:52:59.6 -- a known variable star
07:06:11.43 -02:51:26.0 -- not a known variable star
07:06:19.07 +01:07:44.0 -- not a known variable star
07:06:21.62 -03:11:42.1 -- a known variable star
07:06:44.66 -01:25:53.0 -- not a known variable star
07:06:51.27 -02:03:50.2 -- a known variable star
07:06:54.21 +02:10:49.3 -- a known variable star
07:06:54.73 -04:13:50.9 -- not a known variable star
07:07:00.71 -00:52:19.9 -- not a known variable star
07:07:06.96 +01:40:01.4 -- not a known variable star
07:07:11.27 -02:58:19.6 -- not a known variable star
07:07:15.65 +02:10:16.5 -- not a known variable star
07:07:24.36 +02:31:25.8 -- not a known variable star
07:07:33.28 -03:25:30.2 -- a known variable star
07:07:40.48 -03:15:05.8 -- a known variable star
07:07:54.34 -01:34:49.4 -- a known variable star
07:08:00.99 -01:31:56.9 -- not a known variable star
07:08:04.47 -01:43:39.9 -- not a known variable star
07:08:17.23 -04:56:00.7 -- a known variable star
07:08:30.77 +01:18:17.8 -- not a known variable star
07:08:35.59 +01:46:44.6 -- not a known variable star
07:08:43.12 +01:18:06.7 -- a known variable star
07:08:44.96 -01:27:55.0 -- not a known variable star
07:08:47.34 -00:37:50.4 -- not a known variable star
07:08:48.82 -03:43:07.6 -- not a known variable star
07:09:21.65 +01:07:26.5 -- a known variable star
07:09:22.87 +01:06:33.4 -- not a known variable star
07:09:38.12 +00:33:56.3 -- not a known variable star
07:09:51.76 -03:51:26.7 -- not a known variable star
07:09:59.80 +01:25:47.9 -- not a known variable star
07:10:02.75 -02:32:02.1 -- not a known variable star
07:10:29.07 +01:45:55.0 -- not a known variable star
07:10:37.59 -04:15:16.7 -- not a known variable star
07:10:40.40 +01:18:15.9 -- not a known variable star
07:10:54.83 -04:19:14.2 -- not a known variable star
07:10:56.81 -04:18:47.7 -- not a known variable star
07:11:04.84 +01:22:10.1 -- not a known variable star
07:11:13.37 -06:42:51.7 -- a known variable star
07:11:44.15 -02:16:15.2 -- not a known variable star
07:11:45.32 -05:40:07.9 -- not a known variable star
07:11:55.42 -04:52:53.2 -- a known variable star
07:12:11.46 -02:24:18.5 -- not a known variable star
07:12:17.08 -02:10:59.6 -- not a known variable star
07:12:54.81 -06:36:46.4 -- a known variable star
07:12:55.87 +02:30:42.5 -- not a known variable star
07:13:04.82 -05:12:25.0 -- a known variable star
07:13:11.35 -00:08:48.2 -- a known variable star
07:13:29.25 -03:39:20.6 -- not a known variable star
07:13:31.55 -03:31:14.3 -- not a known variable star
07:13:32.85 +00:13:15.9 -- a known variable star
07:14:02.20 -01:05:37.5 -- not a known variable star
07:14:03.49 -00:18:23.3 -- not a known variable star
07:14:12.70 -04:31:50.9 -- a known variable star
07:14:45.40 -01:22:48.0 -- not a known variable star
07:15:26.09 -01:11:22.4 -- not a known variable star
07:15:39.63 -00:49:27.4 -- not a known variable star
07:15:44.02 -06:38:23.5 -- not a known variable star
07:15:57.87 -01:33:34.6 -- a known variable star
07:16:34.06 -05:05:58.8 -- a known variable star
07:17:38.21 -05:59:16.4 -- not a known variable star
07:17:39.14 -03:44:20.4 -- a known variable star
07:17:41.28 +00:07:01.5 -- not a known variable star
07:17:44.49 -01:00:25.8 -- not a known variable star
07:17:47.06 -06:57:41.9 -- a known variable star
07:18:05.03 -01:25:38.0 -- not a known variable star
07:18:48.75 -01:43:46.8 -- not a known variable star
07:18:50.15 -05:15:16.1 -- not a known variable star
07:18:56.81 -01:17:53.1 -- a known variable star
07:19:20.29 -00:18:57.8 -- a known variable star
07:19:55.70 -00:15:42.1 -- not a known variable star
07:20:48.79 -00:38:29.4 -- not a known variable star
07:20:50.47 -00:51:22.9 -- a known variable star
07:20:51.30 -01:01:32.3 -- not a known variable star
07:21:05.85 +00:28:16.8 -- not a known variable star
07:21:06.34 -03:15:03.8 -- not a known variable star
07:21:14.17 +01:37:58.6 -- not a known variable star
07:21:25.31 -03:35:02.6 -- a known variable star
07:21:45.83 -00:10:00.7 -- not a known variable star
Found 165 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
225 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 225 (excluding asteroids and hot pixels, 165 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)2461152.61609425 -observatory V36
00:41:23.48 +01:39:41.9 Mercury (-0.2mag)
03:38:53.58 +19:59:57.3 Venus (-3.9mag)
00:35:11.26 +02:45:57.6 Mars (1.2mag)
07:15:36.30 +22:41:13.5 Jupiter (-2.1mag)
00:31:52.63 +01:05:42.2 Saturn (0.9mag)
03:49:00.97 +19:51:40.7 Uranus (5.8mag)
00:11:37.48 -00:10:26.7 Neptune (7.8mag)
20:33:59.10 -22:53:01.1 Pluto (14.5mag)
06:21:59.68 +27:34:14.9 Moon (-9.7mag)
-rw-r--r-- 1 apache apache 362 Apr 21 23:25 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461152.61609425:
07:15:40.58 +22:41:02.0 Io (5.8mag)
07:15:24.49 +22:41:39.6 Europa (5.9mag)
07:15:54.08 +22:40:38.2 Ganymede (5.4mag)
07:15:15.92 +22:41:48.9 Callisto (6.6mag)
07:18:39.32 +22:26:09.7 Himalia (15.4mag)
07:15:37.36 +22:41:08.8 Thebe (16.3mag)
07:18:57.86 +22:56:28.1 Elara (17.3mag)
07:14:54.08 +23:18:01.8 Pasiphae (17.4mag)
07:23:47.40 +22:39:48.1 Carme (18.6mag)
00:31:46.84 +01:05:41.3 Titan (8.8mag)
00:31:58.41 +01:05:43.7 Rhea (10.1mag)
00:31:24.75 +01:04:53.6 Iapetus (11.5mag)
00:31:41.86 +01:05:58.8 Hyperion (14.8mag)
00:33:24.48 +01:13:49.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 21 23:25 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461152.61609425:
16:02:57.26 -20:11:34.3 JWST
17:04:26.90 +43:58:42.2 Chandra
07:53:06.01 -35:08:27.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 21 23:25 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461152.61609425 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
05:29:55.43 +30:49:47.8 18.0mag P/2009 WX51 (Catalina)
18:54:05.68 -29:09:08.8 13.8mag P/2010 H2 (Vales)
05:11:17.17 -69:23:00.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:52.07 +31:28:53.6 17.3mag C/2017 K2 (PANSTARRS)
17:29:38.45 +11:15:36.9 17.6mag C/2021 G2 (ATLAS)
23:11:42.86 +29:28:54.0 17.1mag C/2022 E2 (ATLAS)
04:36:26.19 +26:11:57.8 16.1mag C/2022 N2 (PANSTARRS)
09:04:58.74 +32:01:52.8 16.3mag C/2022 QE78 (ATLAS)
08:32:12.01 +00:28:24.1 17.4mag C/2022 R6 (PANSTARRS)
18:52:04.02 +19:02:05.8 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:38:33.57 -11:25:52.9 17.5mag P/2023 B1 (PANSTARRS)
09:05:06.06 -10:55:51.8 17.7mag C/2023 F3 (ATLAS)
21:59:55.72 +63:16:49.7 17.6mag C/2023 H5 (Lemmon)
19:13:17.22 -03:51:16.6 14.1mag C/2023 R1 (PANSTARRS)
21:12:54.18 +86:46:14.3 17.8mag C/2023 X2 (Lemmon)
06:21:14.87 +63:30:00.2 17.2mag C/2024 A1 (ATLAS)
05:25:58.30 +20:09:52.3 11.4mag C/2024 E1 (Wierzchos)
16:15:08.59 +07:23:04.1 17.3mag C/2024 G6 (ATLAS)
20:22:15.78 +16:58:02.8 14.5mag C/2024 J3 (ATLAS)
03:31:56.74 -21:28:37.2 16.3mag C/2024 T5 (ATLAS)
05:22:01.14 +43:49:10.3 17.7mag C/2025 J1 (Borisov)
13:13:58.40 +48:47:46.0 15.5mag C/2025 L1 (ATLAS)
03:35:13.41 -27:12:11.0 17.9mag C/2025 Q3 (ATLAS)
01:03:40.06 +14:18:26.6 7.8mag C/2025 R3 (PANSTARRS)
12:51:31.08 +03:22:07.1 17.4mag C/2025 Y1 (ATLAS)
04:09:51.49 +02:07:52.4 14.8mag C/2026 A1 (MAPS)
00:16:28.74 +38:16:29.9 14.8mag C/2026 B2 (Sun-Gao)
18:54:48.40 -09:23:08.0 11.5mag 10P/Tempel
14:51:57.84 +02:31:00.7 14.5mag 24P/Schaumasse
11:01:20.87 -01:20:31.1 15.7mag 29P/Schwassmann-Wachmann
10:37:44.63 -03:39:07.0 17.0mag 43P/Wolf-Harrington
01:58:10.02 +18:31:07.9 17.3mag 47P/Ashbrook-Jackson
07:22:19.61 +35:40:36.4 17.0mag 63P/Wild
23:36:44.00 -10:43:51.2 15.7mag 65P/Gunn
04:19:53.87 +23:16:52.5 15.9mag 76P/West-Kohoutek-Ikemura
01:19:11.51 +09:25:07.8 14.3mag 78P/Gehrels
23:21:09.89 -07:34:57.4 14.7mag 88P/Howell
02:27:57.79 +22:13:33.7 15.1mag 93P/Lovas
05:06:36.83 +32:35:33.2 16.1mag 123P/West-Hartley
08:36:00.50 +35:32:47.6 16.2mag 124P/Mrkos
02:42:44.50 +15:02:26.9 16.4mag 128P/Shoemaker-Holt
02:59:35.03 +15:12:57.0 17.5mag 131P/Mueller
01:58:45.73 +15:12:00.2 10.5mag 141P/Machholz
02:06:42.10 +07:08:20.9 10.5mag 141P-A/Machholz
00:49:25.35 +02:53:37.5 12.1mag 141P-D/Machholz
02:37:19.60 +08:52:34.0 17.9mag 141P-I/Machholz
01:19:31.42 +01:33:46.0 15.0mag 162P/SidingSpring
14:40:41.66 +00:29:40.4 17.8mag 210P/Christensen
21:55:49.68 -09:59:26.1 17.8mag 218P/LINEAR
17:17:23.70 -13:11:10.3 16.1mag 235P/LINEAR
05:47:50.77 +35:06:50.4 16.8mag 240P/NEAT
07:41:44.30 -04:32:06.0 17.8mag 242P/Spahr
22:32:12.94 -19:17:23.4 17.7mag 260P/McNaught
02:10:52.93 +21:59:15.4 17.9mag 295P/LINEAR
15:40:02.72 +07:22:14.7 17.5mag 391P/Kowalski
07:36:46.08 +21:22:23.8 17.7mag 450P/LONEOS
05:44:56.81 +44:40:32.2 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 21 23:25 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 21 23:25 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:06:16.602 -06:52:59.29 AT 2026jpa 2026-04-13.89 19.276
06:42:32.732 -34:30:04.15 AT 2026joz 2026-04-14.77 18.707
13:06:33.339 -08:24:24.46 AT 2026joy 2026-04-14.02 19.307
21:07:11.613 -12:36:56.09 AT 2026jox 2026-04-14.14 18.849
05:34:42.408 -28:21:31.62 AT 2026jow 2026-04-14.74 18.902
12:30:54.108 -14:11:53.07 AT 2026jov 2026-04-14.03 19.309
05:52:53.155 -34:43:22.49 AT 2026jou 2026-04-14.75 19.398
05:40:18.921 -24:52:33.50 AT 2026jot 2026-04-14.77 18.65
15:53:02.304 +04:30:53.21 AT 2026jos 2026-04-14.09 19.566
11:19:37.053 +36:36:59.54 AT 2026jor 2026-04-11.94 20.14
08:17:15.784 +16:04:01.41 AT 2026joq 2026-04-11.86 19.95
15:52:58.319 -17:01:02.93 AT 2026jop 2026-04-09.53 19.69
09:28:29.338 +17:46:10.46 AT 2026joo 2026-04-11.90 19.1
14:08:31.151 +20:01:29.32 AT 2026jon 2026-04-08.02 19.9
08:15:22.510 -21:29:08.39 AT 2026jom 2026-04-12.37 19.76
12:13:11.990 +05:30:27.70 AT 2026jol 2026-04-08.25 16.6
09:57:55.902 +03:33:01.27 AT 2026jok 2026-03-06.10 21.72
15:47:58.800 -16:07:43.45 AT 2026joj 2026-04-10.44 20.1583
09:57:44.859 +01:08:42.73 AT 2026joi 2026-04-06.02 22.85
14:40:55.647 +05:24:36.73 SN 2026joh 2026-04-14.03 17.708
-rw-r--r-- 1 apache apache 30K Apr 21 23:25 tns_transients_list.txt
