This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RR Mon,2461159.6127,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RR Mon 20260429.1127 10.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.90 06:53:36.50 -04:59:47.9
217.62726 -1.79473 galactic Mon Second-epoch detections are separated by 0.5" and 6.9 pix
The object was found in VSX23" BEST-II lra2b_00421
Type: ACV
# Max. Min./Amp. JD0 Period
13.998 CR Y 0.060 CR 1.369000000000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:36.50 -04:59:47.9: 14.12 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:36.50 -04:59:47.9: 14.90 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.49 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 lra2b_00421,2461159.6127,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 lra2b_00421 20260429.1127 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 13.03 06:52:12.49 -00:22:25.6
213.35238 0.00094 galactic Mon Second-epoch detections are separated by 0.4" and 6.9 pix
The object was found in VSX15" Gaia DR3 3113182378515802496
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.720 G 13.740 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:52:12.49 -00:22:25.6: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:12.49 -00:22:25.6: 15.41 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.41 +/- 0.30
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113182378515802496,2461159.6127,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113182378515802496 20260429.1127 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 29.1127 2461159.6127 12.97 06:57:31.65 -00:23:42.1
213.97785 1.17468 galactic Mon Second-epoch detections are separated by 2.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.3747-00.3973 | 06:57:31.65 -00:23:42.1 (user input) | CBH (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:31.65 -00:23:42.1: 13.99 +/- 0.15 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:31.65 -00:23:42.1: 15.57 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.99 +/- 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
ATO J104.3747-00.3973,2461159.6127,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J104.3747-00.3973 20260429.1127 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 29.1127 2461159.6127 12.88 06:55:22.99 -02:18:59.2
215.44313 -0.17893 galactic Mon Second-epoch detections are separated by 1.3" and 6.9 pix
The object was found in VSX 3" Gaia DR3 3105987414941950208
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.170 G 14.200 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:55:22.99 -02:18:59.2: 14.54 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:55:22.99 -02:18:59.2: 15.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105987414941950208,2461159.6127,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105987414941950208 20260429.1127 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 29.1127 2461159.6127 12.81 06:56:38.29 -04:36:28.6
217.62524 -0.94573 galactic Mon Second-epoch detections are separated by 2.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.1586-04.6125 | 06:56:38.29 -04:36:28.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.398+/-0.038 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:56:38.29 -04:36:28.6: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:56:38.29 -04:36:28.6: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104.1586-04.6125,2461159.6127,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J104.1586-04.6125 20260429.1127 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 29.1127 2461159.6127 12.90 07:00:08.49 -00:53:10.0
214.71325 1.53197 galactic Mon Second-epoch detections are separated by 2.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112246281802906624 | 07:00:07.87 -00:52:53.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.369+/-0.081 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:00:08.49 -00:53:10.0: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:00:08.49 -00:53:10.0: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112246281802906624,2461159.6127,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112246281802906624 20260429.1127 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.69 07:05:23.54 -01:12:19.8
215.59774 2.55341 galactic Mon Second-epoch detections are separated by 2.5" and 7.1 pix
The object was found in VSX 2" Gaia DR3 3109509013245659392
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.690 G 13.750 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:23.54 -01:12:19.8: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:23.54 -01:12:19.8: 15.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109509013245659392,2461159.6127,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109509013245659392 20260429.1127 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 29.1127 2461159.6127 12.74 07:02:13.77 -00:39:21.2
214.74682 2.10145 galactic Mon Second-epoch detections are separated by 0.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112607471372279424 | 07:02:13.89 -00:39:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:13.77 -00:39:21.2: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:13.77 -00:39:21.2: 14.89 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.89 +/- 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 3112607471372279424,2461159.6127,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112607471372279424 20260429.1127 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 29.1127 2461159.6127 12.62 07:09:03.94 -01:19:31.7
216.12543 3.31471 galactic Mon Second-epoch detections are separated by 1.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:09:03.94 -01:19:31.7 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:09:03.94 -01:19:31.7: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:09:03.94 -01:19:31.7: 15.36 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461159.6127,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260429.1127 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 29.1127 2461159.6127 12.44 07:02:35.25 -03:37:56.6
217.43559 0.81961 galactic Mon Second-epoch detections are separated by 1.4" and 7.0 pix
The object was found in VSX24" Gaia DR3 3107854935441146240
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.670 G 11.700 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:35.25 -03:37:56.6: 14.57 +/- 0.30 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:35.25 -03:37:56.6: 15.10 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.89 +/- 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 3107854935441146240,2461159.6127,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107854935441146240 20260429.1127 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 29.1127 2461159.6127 12.71 07:05:15.37 +00:02:45.6
214.46767 3.09513 galactic Mon Second-epoch detections are separated by 2.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112750781541980032 | 07:05:17.03 +00:02:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.786+/-0.033 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:15.37 +00:02:45.6: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:15.37 +00:02:45.6: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112750781541980032,2461159.6127,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112750781541980032 20260429.1127 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 29.1127 2461159.6127 12.49 06:57:33.46 -03:31:49.5
216.77109 -0.24992 galactic Mon Second-epoch detections are separated by 2.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.3903-03.5266 | 06:57:33.46 -03:31:49.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:33.46 -03:31:49.5: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:33.46 -03:31:49.5: 15.05 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104.3903-03.5266,2461159.6127,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J104.3903-03.5266 20260429.1127 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.52 06:51:34.73 -01:53:52.3
214.63717 -0.83393 galactic Mon Second-epoch detections are separated by 4.2" and 7.5 pix
The object was found in VSX 6" Gaia DR3 3106258719436766848
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.350 G 14.370 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:51:34.73 -01:53:52.3: 13.46 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:34.73 -01:53:52.3: 14.39 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106258719436766848,2461159.6127,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106258719436766848 20260429.1127 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 29.1127 2461159.6127 12.51 06:55:03.32 +01:02:05.0
212.42323 1.27659 galactic Mon Second-epoch detections are separated by 2.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.7645+01.0325 | 06:55:03.32 +01:02:05.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:55:03.32 +01:02:05.0: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:55:03.32 +01:02:05.0: 13.84 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.7645+01.0325,2461159.6127,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J103.7645+01.0325 20260429.1127 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 29.1127 2461159.6127 12.43 07:16:03.79 -01:38:30.1
217.21194 4.72313 galactic Mon Second-epoch detections are separated by 3.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:16:03.79 -01:38:30.1 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:16:03.79 -01:38:30.1: 14.60 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:16:03.79 -01:38:30.1: 15.36 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461159.6127,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260429.1127 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 29.1127 2461159.6127 12.53 06:53:42.63 -01:01:10.7
214.09844 0.04064 galactic Mon Second-epoch detections are separated by 1.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.4228-01.0262 | 06:53:42.63 -01:01:10.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:42.63 -01:01:10.7: 13.68 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:42.63 -01:01:10.7: 14.02 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4228-01.0262,2461159.6127,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J103.4228-01.0262 20260429.1127 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 29.1127 2461159.6127 12.28 07:02:32.62 -02:31:08.0
216.44039 1.31956 galactic Mon Second-epoch detections are separated by 1.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.6344-02.5144 | 07:02:33.15 -02:30:54.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:32.62 -02:31:08.0: 14.72 +/- 0.33 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:32.62 -02:31:08.0: 15.55 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.72 +/- 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
ATO J105.6344-02.5144,2461159.6127,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J105.6344-02.5144 20260429.1127 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.32 07:13:43.93 -01:35:26.7
216.89791 4.22925 galactic Mon Second-epoch detections are separated by 0.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3108583602413252224 | 07:13:44.38 -01:35:50.2 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A2V (LAMOST DR5) J-Ks=0.143+/-0.041 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:13:43.93 -01:35:26.7: 14.57 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:13:43.93 -01:35:26.7: 15.34 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108583602413252224,2461159.6127,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108583602413252224 20260429.1127 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.46 07:09:05.01 -02:57:19.9
217.57776 2.57078 galactic Mon Second-epoch detections are separated by 3.0" and 7.0 pix
The object was found in VSX 3" Gaia DR3 3107955953073281024
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.800 G 13.830 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:09:05.01 -02:57:19.9: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:09:05.01 -02:57:19.9: 15.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107955953073281024,2461159.6127,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107955953073281024 20260429.1127 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 29.1127 2461159.6127 12.38 06:51:46.27 -05:25:55.8
217.80721 -2.40016 galactic Mon Second-epoch detections are separated by 0.9" and 6.9 pix
The object was found in VSX 2" Gaia DR3 3101909360675940992
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.470 G 13.490 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:51:46.27 -05:25:55.8: 14.76 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:46.27 -05:25:55.8: 15.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101909360675940992,2461159.6127,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101909360675940992 20260429.1127 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.46 07:09:19.83 +00:54:53.6
214.15877 4.39797 galactic Mon Second-epoch detections are separated by 1.1" and 6.6 pix
The object was found in VSX 4" Gaia DR3 3114403553674802304
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.540 G 13.590 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:09:19.83 +00:54:53.6: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:09:19.83 +00:54:53.6: 15.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114403553674802304,2461159.6127,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114403553674802304 20260429.1127 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 29.1127 2461159.6127 12.38 06:59:30.61 -04:05:39.4
217.49517 -0.07424 galactic Mon Second-epoch detections are separated by 1.9" and 6.7 pix
The object was found in VSX 3" Gaia DR3 3101809545632575104
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.710 G 13.730 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:30.61 -04:05:39.4: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:30.61 -04:05:39.4: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101809545632575104,2461159.6127,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101809545632575104 20260429.1127 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.53 06:50:50.92 -02:36:24.6
215.18524 -1.31935 galactic Mon Second-epoch detections are separated by 0.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3105927800794434176 | 06:50:50.10 -02:36:07.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1956ApJS....2..271M LF 9 -03 143
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:50:50.92 -02:36:24.6: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:50:50.92 -02:36:24.6: 13.74 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105927800794434176,2461159.6127,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105927800794434176 20260429.1127 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 29.1127 2461159.6127 12.36 07:08:16.27 -02:14:30.6
216.84980 2.71816 galactic Mon Second-epoch detections are separated by 0.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.0656-02.2522 | 07:08:15.83 -02:14:50.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.674+/-0.033 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:16.27 -02:14:30.6: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:16.27 -02:14:30.6: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.0656-02.2522,2461159.6127,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J107.0656-02.2522 20260429.1127 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.45 06:57:30.10 -00:57:11.9
214.47176 0.91419 galactic Mon Second-epoch detections are separated by 0.7" and 6.7 pix
The object was found in VSX 3" Gaia DR3 3112232984583836928
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.550 G 13.580 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:30.10 -00:57:11.9: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:30.10 -00:57:11.9: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112232984583836928,2461159.6127,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112232984583836928 20260429.1127 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 29.1127 2461159.6127 12.31 07:02:50.56 -03:19:41.4
217.19425 1.01551 galactic Mon Second-epoch detections are separated by 4.2" and 7.4 pix
The object was found in VSX 1" Gaia DR3 3108620917091030272
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.750 G 13.790 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:50.56 -03:19:41.4: 13.47 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:50.56 -03:19:41.4: 15.50 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.47 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108620917091030272,2461159.6127,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108620917091030272 20260429.1127 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 29.1127 2461159.6127 12.38 07:08:29.18 -00:58:27.6
215.74633 3.34682 galactic Mon Second-epoch detections are separated by 1.5" and 6.7 pix
The object was found in VSX 1" Gaia DR3 3109604288498805632
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.490 G 13.520 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:29.18 -00:58:27.6: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:29.18 -00:58:27.6: 15.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109604288498805632,2461159.6127,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109604288498805632 20260429.1127 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.06 07:05:08.38 -04:26:25.2
218.44550 1.01500 galactic Mon Second-epoch detections are separated by 1.5" and 6.7 pix
The object was found in VSX 1" Gaia DR3 3101552603515643008
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.210 G 13.240 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:08.38 -04:26:25.2: 14.28 +/- 0.23 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:08.38 -04:26:25.2: 15.47 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.28 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101552603515643008,2461159.6127,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101552603515643008 20260429.1127 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 29.1127 2461159.6127 12.23 06:59:54.60 -02:15:14.1
215.90384 0.85567 galactic Mon Second-epoch detections are separated by 1.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.9744-02.2632 | 06:59:54.60 -02:15:14.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.386+/-0.031 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:54.60 -02:15:14.1: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:54.60 -02:15:14.1: 15.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104.9744-02.2632,2461159.6127,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J104.9744-02.2632 20260429.1127 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.03 07:13:59.84 -02:51:47.8
218.06100 3.70255 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 | ATO J108.4987-02.8566 | 07:13:59.03 -02:51:29.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 296670 J-Ks=0.278+/-0.031 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:13:59.84 -02:51:47.8: 14.53 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:13:59.84 -02:51:47.8: 15.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.4987-02.8566,2461159.6127,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J108.4987-02.8566 20260429.1127 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.29 07:03:51.10 -03:43:31.4
217.66275 1.05738 galactic Mon Second-epoch detections are separated by 1.0" and 6.8 pix
The object was found in VSX 2" Gaia DR3 3107838541545851008
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.590 G 13.610 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:51.10 -03:43:31.4: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:51.10 -03:43:31.4: 15.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107838541545851008,2461159.6127,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107838541545851008 20260429.1127 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 29.1127 2461159.6127 12.41 07:01:22.61 -00:16:06.1
214.30443 2.08876 galactic Mon Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.3436-00.2691 | 07:01:21.98 -00:16:29.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:22.61 -00:16:06.1: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:22.61 -00:16:06.1: 15.62 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J105.3436-00.2691,2461159.6127,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J105.3436-00.2691 20260429.1127 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 29.1127 2461159.6127 12.05 07:06:41.15 -02:24:48.2
216.82063 2.28757 galactic Mon Second-epoch detections are separated by 2.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.6656-02.4124 | 07:06:41.15 -02:24:48.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:06:41.15 -02:24:48.2: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:06:41.15 -02:24:48.2: 15.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.6656-02.4124,2461159.6127,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J106.6656-02.4124 20260429.1127 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 29.1127 2461159.6127 12.22 07:01:21.74 +02:15:49.7
212.04634 3.23945 galactic Mon Second-epoch detections are separated by 0.2" and 6.8 pix
The object was found in VSX 2" Gaia DR3 3115503000884520448
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.180 G 13.210 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:21.74 +02:15:49.7: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:21.74 +02:15:49.7: 13.50 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115503000884520448,2461159.6127,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115503000884520448 20260429.1127 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.09 07:12:09.81 +01:52:14.8
213.62858 5.46381 galactic CMi Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J108.0443+01.8719 | 07:12:08.56 +01:52:23.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.236+/-0.033 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:09.81 +01:52:14.8: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:09.81 +01:52:14.8: 15.31 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.0443+01.8719,2461159.6127,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J108.0443+01.8719 20260429.1127 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.16 07:12:01.96 -01:11:16.0
216.34348 4.03689 galactic Mon Second-epoch detections are separated by 0.8" and 6.9 pix
The object was found in ASASSN-V 3" ASASSN-V J071201.82-011118.1
Type: EA
MeanMag 12.68 m Amp. 0.27 m Period 3.3076416 d
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:01.96 -01:11:16.0: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:01.96 -01:11:16.0: 15.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461159.6127,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260429.1127 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.09 07:15:49.72 -00:37:02.7
216.27176 5.14169 galactic Mon Second-epoch detections are separated by 2.5" and 7.1 pix
The object was found in VSX16" Gaia DR3 3110157583366513664
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.020 G 14.070 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:15:49.72 -00:37:02.7: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:15:49.72 -00:37:02.7: 15.25 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110157583366513664,2461159.6127,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110157583366513664 20260429.1127 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.07 07:03:14.46 +01:07:06.4
213.28176 3.13601 galactic Mon Second-epoch detections are separated by 2.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.8095+01.1236 | 07:03:14.29 +01:07:25.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:14.46 +01:07:06.4: 14.70 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:14.46 +01:07:06.4: 15.52 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J105.8095+01.1236,2461159.6127,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J105.8095+01.1236 20260429.1127 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.13 07:16:04.59 +00:48:08.0
215.03238 5.84685 galactic Mon Second-epoch detections are separated by 1.1" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J109.0147+00.7974 | 07:16:04.59 +00:48:08.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:16:04.59 +00:48:08.0: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:16:04.59 +00:48:08.0: 15.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J109.0147+00.7974,2461159.6127,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J109.0147+00.7974 20260429.1127 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 29.1127 2461159.6127 12.12 06:50:59.48 -02:47:54.1
215.37203 -1.37488 galactic Mon Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3105904607971898368 | 06:50:58.10 -02:47:57.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.318+/-0.037 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:50:59.48 -02:47:54.1: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:50:59.48 -02:47:54.1: 13.35 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105904607971898368,2461159.6127,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105904607971898368 20260429.1127 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.01 07:08:41.85 +01:18:46.4
213.73113 4.43861 galactic CMi Second-epoch detections are separated by 1.9" and 6.9 pix
The object was found in VSX 9" Gaia DR3 3114481588940149120
Type: ROT
# Max. Min./Amp. JD0 Period
13.690 G 13.710 G G
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:41.85 +01:18:46.4: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:41.85 +01:18:46.4: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114481588940149120,2461159.6127,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114481588940149120 20260429.1127 12.01CV 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 29.1127 2461159.6127 12.15 07:03:36.84 -01:50:14.9
215.95664 1.86909 galactic Mon Second-epoch detections are separated by 1.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.9026-01.8386 | 07:03:36.84 -01:50:14.9 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:36.84 -01:50:14.9: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:36.84 -01:50:14.9: 14.50 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.50 +/- 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
ATO J105.9026-01.8386,2461159.6127,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J105.9026-01.8386 20260429.1127 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.09 07:13:11.69 +01:02:13.4
214.49197 5.31325 galactic Mon Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J108.2988+01.0363 | 07:13:11.08 +01:02:31.0 (Gaia DR3) | SINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=-0.088+/-0.043 (B)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:13:11.69 +01:02:13.4: 14.63 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:13:11.69 +01:02:13.4: 15.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.2988+01.0363,2461159.6127,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J108.2988+01.0363 20260429.1127 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.27 06:46:14.65 +01:13:09.0
211.25474 -0.59937 galactic Mon Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:46:14.65 +01:13:09.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:46:14.65 +01:13:09.0: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:46:14.65 +01:13:09.0: 13.10 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461159.6127,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260429.1127 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 29.1127 2461159.6127 12.12 07:03:40.27 -01:07:51.0
215.33437 2.20497 galactic Mon Second-epoch detections are separated by 1.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3109541277034406144 | 07:03:40.37 -01:07:35.5 (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: G5 (LAMOST DR5) J-Ks=0.245+/-0.038 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:40.27 -01:07:51.0: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:40.27 -01:07:51.0: 15.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3109541277034406144,2461159.6127,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 3109541277034406144 20260429.1127 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.96 07:18:18.05 -00:24:27.9
216.36956 5.78700 galactic Mon Second-epoch detections are separated by 2.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J109.5734-00.4114 | 07:18:18.05 -00:24:27.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.255+/-0.030 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:18:18.05 -00:24:27.9: 14.01 +/- 0.25 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:18:18.05 -00:24:27.9: 15.35 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.01 +/- 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
ATO J109.5734-00.4114,2461159.6127,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J109.5734-00.4114 20260429.1127 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.90 07:12:11.80 -01:59:47.9
217.08257 3.70197 galactic Mon Second-epoch detections are separated by 2.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J108.0562-02.0008 | 07:12:11.98 -02:00:12.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A 1949AnHar.112....1C HD 293581 J-Ks=0.610+/-0.033 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:11.80 -01:59:47.9: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:11.80 -01:59:47.9: 15.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.0562-02.0008,2461159.6127,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J108.0562-02.0008 20260429.1127 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.82 07:16:12.87 -04:06:21.0
219.42141 3.61968 galactic Mon Second-epoch detections are separated by 2.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3059915163320894848 | 07:16:12.88 -04:06:43.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.366+/-0.030 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:16:12.87 -04:06:21.0: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:16:12.87 -04:06:21.0: 15.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059915163320894848,2461159.6127,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059915163320894848 20260429.1127 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.02 07:05:00.18 +01:38:42.9
213.01287 3.76800 galactic Mon Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.2479+01.6428 | 07:05:00.18 +01:38:42.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.035+/-0.037 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:00.18 +01:38:42.9: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:00.18 +01:38:42.9: 14.55 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.55 +/- 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
ATO J106.2479+01.6428,2461159.6127,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J106.2479+01.6428 20260429.1127 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 29.1127 2461159.6127 11.99 06:58:21.76 -00:45:45.5
214.40032 1.19271 galactic Mon Second-epoch detections are separated by 1.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112259952677226112 | 06:58:20.49 -00:45:55.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.199+/-0.035 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:58:21.76 -00:45:45.5: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:21.76 -00:45:45.5: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112259952677226112,2461159.6127,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112259952677226112 20260429.1127 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.02 07:12:26.24 +01:50:34.4
213.68482 5.51204 galactic CMi Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:12:26.24 +01:50:34.4 (user input) | T | P | (position from user input) J-Ks=0.174+/-0.031 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:26.24 +01:50:34.4: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:26.24 +01:50:34.4: 15.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461159.6127,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260429.1127 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 29.1127 2461159.6127 11.91 07:01:01.01 -00:25:44.6
214.40638 1.93533 galactic Mon Second-epoch detections are separated by 0.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.2433-00.4249 | 07:01:01.31 -00:25:23.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0: 1956ApJS....2..271M LF 9 -01 512
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:01.01 -00:25:44.6: 14.28 +/- 0.21 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:01.01 -00:25:44.6: 15.16 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.28 +/- 0.21
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J105.2433-00.4249,2461159.6127,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J105.2433-00.4249 20260429.1127 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.85 06:59:25.68 -01:04:49.7
214.80476 1.28455 galactic Mon Second-epoch detections are separated by 1.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.8632-01.0847 | 06:59:25.72 -01:05:11.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.646+/-0.032 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:25.68 -01:04:49.7: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:25.68 -01:04:49.7: 15.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J104.8632-01.0847,2461159.6127,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J104.8632-01.0847 20260429.1127 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 29.1127 2461159.6127 11.50 07:04:20.85 -04:41:02.1
218.57141 0.72784 galactic Mon Second-epoch detections are separated by 1.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3101541986356735360 | 07:04:20.78 -04:41:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.342+/-0.031 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:04:20.85 -04:41:02.1: 14.52 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:04:20.85 -04:41:02.1: 15.22 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101541986356735360,2461159.6127,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101541986356735360 20260429.1127 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.80 06:59:39.73 -00:40:07.6
214.46510 1.52459 galactic Mon Second-epoch detections are separated by 1.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:59:39.73 -00:40:07.6 (user input) | T | P | (position from user input) J-Ks=0.213+/-0.053 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:39.73 -00:40:07.6: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:39.73 -00:40:07.6: 15.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461159.6127,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260429.1127 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.67 07:06:04.88 -02:19:37.6
216.67463 2.19292 galactic Mon Second-epoch detections are separated by 1.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.5323-02.3310 | 07:06:05.79 -02:19:56.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.680+/-0.033 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:06:04.88 -02:19:37.6: 14.68 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:06:04.88 -02:19:37.6: 15.41 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.5323-02.3310,2461159.6127,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J106.5323-02.3310 20260429.1127 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.61 07:15:10.56 -04:30:19.1
219.65624 3.20536 galactic Mon Second-epoch detections are separated by 2.9" and 7.0 pix
The object was found in VSX15" ASAS J071511-0430.1
Type: SR
# Max. Min./Amp. JD0 Period
8.841 Ic Y 0.304 Ic 2455546.90000 615.000000000000 M7
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:15:10.56 -04:30:19.1: 14.59 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:15:10.56 -04:30:19.1: 15.00 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.00 +/- 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
ASAS J071511-0430.1,2461159.6127,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J071511-0430.1 20260429.1127 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.46 07:08:48.29 +00:19:42.4
214.62183 4.01337 galactic Mon Second-epoch detections are separated by 1.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.2071+00.3441 | 07:08:48.95 +00:20:00.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:48.29 +00:19:42.4: 14.66 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:48.29 +00:19:42.4: 15.51 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.2071+00.3441,2461159.6127,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J107.2071+00.3441 20260429.1127 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.52 07:05:10.46 -00:00:18.8
214.50395 3.05354 galactic Mon Second-epoch detections are separated by 2.7" and 6.4 pix
The object was found in VSX15" ASAS J070510-0000.2
Type: MISC
# Max. Min./Amp. JD0 Period
12.450 V Y 0.190 V 2451920.30000 56.605688000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:10.46 -00:00:18.8: 14.88 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:10.46 -00:00:18.8: 15.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J070510-0000.2,2461159.6127,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J070510-0000.2 20260429.1127 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.43 07:16:13.30 -00:00:45.6
215.77723 5.50626 galactic Mon Second-epoch detections are separated by 1.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3111060630310108928 | 07:16:14.83 -00:00:07.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.114+/-0.038 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:16:13.30 -00:00:45.6: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:16:13.30 -00:00:45.6: 14.50 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.50 +/- 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 3111060630310108928,2461159.6127,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111060630310108928 20260429.1127 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.24 07:11:00.63 -02:53:39.2
217.74465 3.02625 galactic Mon Second-epoch detections are separated by 0.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.7472-02.9052 | 07:11:00.72 -02:54:01.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 1949AnHar.112....1C HD 296558 J-Ks=0.245+/-0.030 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:11:00.63 -02:53:39.2: 14.59 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:11:00.63 -02:53:39.2: 15.35 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.7472-02.9052,2461159.6127,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J107.7472-02.9052 20260429.1127 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 29.1127 2461159.6127 11.04 07:08:43.96 -03:56:11.0
218.40933 2.04222 galactic Mon Second-epoch detections are separated by 1.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.1828-03.9366 | 07:08:44.38 -03:55:56.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.613+/-0.038 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:43.96 -03:56:11.0: 12.69 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:43.96 -03:56:11.0: 15.35 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.69 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1828-03.9366,2461159.6127,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J107.1828-03.9366 20260429.1127 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 10.63 07:14:38.83 -03:56:25.0
219.09333 3.34960 galactic Mon Second-epoch detections are separated by 1.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J108.6673-03.9395 | 07:14:38.63 -03:56:02.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B8 1949AnHar.112....1C HD 296712 J-Ks=0.114+/-0.035 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:14:38.83 -03:56:25.0: 14.44 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:14:38.83 -03:56:25.0: 15.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.6673-03.9395,2461159.6127,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J108.6673-03.9395 20260429.1127 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 9.97 07:17:51.22 -01:41:37.7
217.46511 5.09634 galactic Mon Second-epoch detections are separated by 0.3" and 6.8 pix
The object was found in VSX20" Gaia DR3 3109822923819222400
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.810 G 12.840 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:17:51.22 -01:41:37.7: 14.50 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:17:51.22 -01:41:37.7: 15.39 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109822923819222400,2461159.6127,9.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109822923819222400 20260429.1127 9.97CV 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 29.1127 2461159.6127 10.19 07:03:02.21 +01:23:57.0
213.00819 3.21848 galactic Mon Second-epoch detections are separated by 0.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.7726+01.3967 | 07:03:03.50 +01:23:37.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F2 1949AnHar.112....1C HD 289496 J-Ks=0.144+/-0.029 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:02.21 +01:23:57.0: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:02.21 +01:23:57.0: 15.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J105.7726+01.3967,2461159.6127,10.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J105.7726+01.3967 20260429.1127 10.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 10.68 06:53:07.46 -01:35:07.5
214.53515 -0.34776 galactic Mon Second-epoch detections are separated by 0.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112275315783496832 | 06:53:09.11 -01:35:02.4 (Gaia DR3) | ACV/roAm/ (local) | (local) | Gaia3var=VARIABLE SpType: B5 1956ApJS....2..271M LF 9 -02 253 J-Ks=0.050+/-0.035 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:07.46 -01:35:07.5: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:07.46 -01:35:07.5: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112275315783496832,2461159.6127,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112275315783496832 20260429.1127 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.26 06:52:35.30 -02:12:18.2
215.02560 -0.74947 galactic Mon Second-epoch detections are separated by 2.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3106035656015561472 | 06:52:34.02 -02:12:34.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5V 1956ApJS....2..271M LF 9 -03 206 J-Ks=0.701+/-0.031 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:52:35.30 -02:12:18.2: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:35.30 -02:12:18.2: 14.41 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106035656015561472,2461159.6127,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106035656015561472 20260429.1127 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.38 07:05:25.02 -00:59:48.8
215.41486 2.65431 galactic Mon Second-epoch detections are separated by 1.1" and 6.8 pix
The object was found in VSX19" Gaia DR3 3109568627391618304
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.510 G 14.540 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:25.02 -00:59:48.8: 14.67 +/- 0.34 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:25.02 -00:59:48.8: 15.35 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.67 +/- 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 3109568627391618304,2461159.6127,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109568627391618304 20260429.1127 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 29.1127 2461159.6127 11.51 07:05:30.66 +01:36:36.7
213.10207 3.86507 galactic Mon Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3114643388949636736 | 07:05:31.92 +01:36:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1949AnHar.112....1C HD 289625 J-Ks=0.365+/-0.030 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:30.66 +01:36:36.7: 13.96 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:30.66 +01:36:36.7: 15.38 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.96 +/- 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 3114643388949636736,2461159.6127,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114643388949636736 20260429.1127 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.47 06:57:39.96 -05:17:24.3
218.34915 -1.02917 galactic Mon Second-epoch detections are separated by 2.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3101213782128977280 | 06:57:41.00 -05:17:46.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.769+/-0.032 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:39.96 -05:17:24.3: 14.76 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:39.96 -05:17:24.3: 15.50 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101213782128977280,2461159.6127,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101213782128977280 20260429.1127 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.62 06:49:41.95 -01:43:20.2
214.26677 -1.17198 galactic Mon Second-epoch detections are separated by 2.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.4172-01.7273 | 06:49:40.14 -01:43:12.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.746+/-0.031 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:49:41.95 -01:43:20.2: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:49:41.95 -01:43:20.2: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.4172-01.7273,2461159.6127,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J102.4172-01.7273 20260429.1127 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.80 07:01:24.19 +01:06:08.5
213.08649 2.71978 galactic Mon Second-epoch detections are separated by 1.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113861670543456896 | 07:01:23.17 +01:06:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 1949AnHar.112....1C HD 289505
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:24.19 +01:06:08.5: 13.65 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:24.19 +01:06:08.5: 14.80 +/- 0.21 detection
Forced photometry reference-image weighted average: 13.93 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113861670543456896,2461159.6127,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113861670543456896 20260429.1127 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.76 07:06:24.24 +00:20:29.3
214.33558 3.48534 galactic Mon Second-epoch detections are separated by 0.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3114263159786050944 | 07:06:23.17 +00:20:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A 1949AnHar.112....1C HD 293175
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:06:24.24 +00:20:29.3: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:06:24.24 +00:20:29.3: 13.87 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114263159786050944,2461159.6127,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114263159786050944 20260429.1127 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 29.1127 2461159.6127 11.77 07:12:29.92 +00:35:37.6
214.80815 4.95603 galactic Mon Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:12:29.92 +00:35:37.6 (user input) | T | P | (position from user input) J-Ks=0.501+/-0.034 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:29.92 +00:35:37.6: 14.63 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:29.92 +00:35:37.6: 15.28 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461159.6127,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260429.1127 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.64 07:18:58.87 -05:26:28.5
220.92719 3.61100 galactic Mon Second-epoch detections are separated by 2.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3058400105016706688 | 07:18:58.38 -05:26:58.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:18:58.87 -05:26:28.5: 14.45 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:18:58.87 -05:26:28.5: 15.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3058400105016706688,2461159.6127,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3058400105016706688 20260429.1127 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.09 06:52:07.82 +00:28:19.6
212.59067 0.36933 galactic Mon Second-epoch detections are separated by 0.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113577274989419904 | 06:52:06.22 +00:27:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.411+/-0.062 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:52:07.82 +00:28:19.6: 13.13 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:07.82 +00:28:19.6: 13.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113577274989419904,2461159.6127,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113577274989419904 20260429.1127 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.92 07:01:07.65 -03:14:32.1
216.92192 0.67420 galactic Mon Second-epoch detections are separated by 3.1" and 6.6 pix
The object was found in VSX 3" Gaia DR3 3108634145589904768
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.120 G 13.150 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:07.65 -03:14:32.1: 14.76 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:07.65 -03:14:32.1: 15.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108634145589904768,2461159.6127,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108634145589904768 20260429.1127 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.06 06:56:36.50 +01:00:09.7
212.62872 1.60753 galactic Mon Second-epoch detections are separated by 0.4" and 6.7 pix
The object was found in VSX 2" Gaia DR3 3113810440173047680
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.150 G 13.170 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:56:36.50 +01:00:09.7: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:56:36.50 +01:00:09.7: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113810440173047680,2461159.6127,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113810440173047680 20260429.1127 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 29.1127 2461159.6127 11.90 07:13:48.27 -00:49:58.9
216.23107 4.59316 galactic Mon Second-epoch detections are separated by 1.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3110877252388089856 | 07:13:49.46 -00:50:25.5 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 293673 J-Ks=0.582+/-0.033 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:13:48.27 -00:49:58.9: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:13:48.27 -00:49:58.9: 15.21 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110877252388089856,2461159.6127,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110877252388089856 20260429.1127 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 11.97 07:00:56.86 -03:16:17.9
216.92752 0.62084 galactic Mon Second-epoch detections are separated by 0.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:00:56.86 -03:16:17.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:00:56.86 -03:16:17.9: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:00:56.86 -03:16:17.9: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461159.6127,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260429.1127 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 29.1127 2461159.6127 12.13 06:54:57.35 -01:11:47.8
214.39791 0.23693 galactic Mon Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.7386-01.1974 | 06:54:57.29 -01:11:24.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K2 1956ApJS....2..271M LF 9 -02 349
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:57.35 -01:11:47.8: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:57.35 -01:11:47.8: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.7386-01.1974,2461159.6127,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J103.7386-01.1974 20260429.1127 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 29.1127 2461159.6127 12.13 07:05:49.23 +01:38:16.7
213.11258 3.94658 galactic Mon Second-epoch detections are separated by 1.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.4621+01.6243 | 07:05:50.63 +01:37:57.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.551+/-0.030 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:49.23 +01:38:16.7: 13.44 +/- 0.11 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:49.23 +01:38:16.7: 14.33 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.84 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4621+01.6243,2461159.6127,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J106.4621+01.6243 20260429.1127 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 29.1127 2461159.6127 12.08 07:07:11.50 -02:58:19.4
217.37542 2.14359 galactic Mon Second-epoch detections are separated by 3.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3107988968482458496 | 07:07:08.73 -02:58:28.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:11.50 -02:58:19.4: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:11.50 -02:58:19.4: 15.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107988968482458496,2461159.6127,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260429.1127 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 29.1127 2461159.6127 12.18 06:52:46.18 -01:34:15.9
214.48197 -0.42011 galactic Mon Second-epoch detections are separated by 1.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112286925076234752 | 06:52:44.07 -01:34:23.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8III 1956ApJS....2..271M LF 9 -02 239
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:52:46.18 -01:34:15.9: 14.95 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:46.18 -01:34:15.9: 15.63 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112286925076234752,2461159.6127,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112286925076234752 20260429.1127 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 29.1127 2461159.6127 12.19 06:58:26.75 -00:54:23.5
214.53786 1.14553 galactic Mon Second-epoch detections are separated by 6.4" 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 | Gaia DR3 3112254596859130368 | 06:58:27.93 -00:54:46.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 1956ApJS....2..271M LF 9 -01 427 J-Ks=0.262+/-0.041 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:58:26.75 -00:54:23.5: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:26.75 -00:54:23.5: 14.33 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112254596859130368,2461159.6127,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112254596859130368 20260429.1127 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.25 07:08:12.55 -03:12:26.0
217.70119 2.26129 galactic Mon Second-epoch detections are separated by 1.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:08:12.55 -03:12:26.0 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:12.55 -03:12:26.0: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:12.55 -03:12:26.0: 14.14 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.14 +/- 0.13
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461159.6127,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260429.1127 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 29.1127 2461159.6127 12.24 06:53:58.11 -04:52:50.6
217.56487 -1.66208 galactic Mon Second-epoch detections are separated by 3.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.4899-04.8802 | 06:53:58.11 -04:52:50.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7IIIa 2012A&A...543A.125G CoRoT 110696033
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:58.11 -04:52:50.6: 14.58 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:58.11 -04:52:50.6: 15.29 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.4899-04.8802,2461159.6127,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J103.4899-04.8802 20260429.1127 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.03 07:01:38.39 -04:40:49.5
218.25920 0.12976 galactic Mon Second-epoch detections are separated by 2.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3101715086411523584 | 07:01:37.75 -04:41:16.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1949AnHar.112....1C HD 296156
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:38.39 -04:40:49.5: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:38.39 -04:40:49.5: 15.48 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101715086411523584,2461159.6127,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101715086411523584 20260429.1127 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.29 06:49:33.19 -01:23:29.2
213.95560 -1.05370 galactic Mon Second-epoch detections are separated by 2.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.3878-01.3922 | 06:49:33.19 -01:23:29.2 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:49:33.19 -01:23:29.2: 14.14 +/- 0.19 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:49:33.19 -01:23:29.2: 13.35 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.3878-01.3922,2461159.6127,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260429.1127 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 29.1127 2461159.6127 12.38 06:52:53.69 +01:22:23.8
211.87566 0.95024 galactic Mon Second-epoch detections are separated by 0.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.2259+01.3729 | 06:52:52.05 +01:22:21.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:52:53.69 +01:22:23.8: 14.25 +/- 0.23 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:53.69 +01:22:23.8: 13.59 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.2259+01.3729,2461159.6127,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J103.2259+01.3729 20260429.1127 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.37 07:01:10.32 +00:00:20.0
214.03715 2.16820 galactic Mon Second-epoch detections are separated by 3.8" and 6.2 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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:10.32 +00:00:20.0: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:10.32 +00:00:20.0: 15.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112882349279538816,2461159.6127,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260429.1127 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 29.1127 2461159.6127 12.32 06:57:00.78 +00:17:37.8
213.30599 1.37441 galactic Mon Second-epoch detections are separated by 2.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113688634901420928 | 06:57:00.01 +00:18:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 292824
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:00.78 +00:17:37.8: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:00.78 +00:17:37.8: 15.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113688634901420928,2461159.6127,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113688634901420928 20260429.1127 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.32 07:07:58.75 -00:56:39.1
215.66136 3.24790 galactic Mon Second-epoch detections are separated by 1.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:07:58.75 -00:56:39.1 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:58.75 -00:56:39.1: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:58.75 -00:56:39.1: 14.24 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461159.6127,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260429.1127 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.35 07:01:46.16 +01:19:50.2
212.92481 2.90524 galactic Mon Second-epoch detections are separated by 2.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3115367176839807872 | 07:01:47.56 +01:19:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:46.16 +01:19:50.2: 13.96 +/- 0.17 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:46.16 +01:19:50.2: 15.44 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.96 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115367176839807872,2461159.6127,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115367176839807872 20260429.1127 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.43 06:47:11.21 -02:50:54.0
214.98389 -2.24346 galactic Mon Second-epoch detections are separated by 2.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3106082209159437440 | 06:47:08.75 -02:50:26.8 (Gaia DR3) | ACV/roAm/ (local) | (local) | Gaia3var=VARIABLE SpType: A5 1956ApJS....2..271M LF 9 -03 45
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:47:11.21 -02:50:54.0: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:47:11.21 -02:50:54.0: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106082209159437440,2461159.6127,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106082209159437440 20260429.1127 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 29.1127 2461159.6127 12.32 07:08:02.93 -03:37:52.5
218.05970 2.03097 galactic Mon Second-epoch detections are separated by 1.5" and 6.8 pix
The object was found in VSX 2" Gaia DR3 3107714060519716992
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.580 G 13.600 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:02.93 -03:37:52.5: 14.67 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:02.93 -03:37:52.5: 15.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107714060519716992,2461159.6127,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107714060519716992 20260429.1127 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.57 06:51:43.84 -00:26:00.1
213.35098 -0.13247 galactic Mon Second-epoch detections are separated by 1.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113180901047215360 | 06:51:44.35 -00:25:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1956ApJS....2..271M LF 9 -01 187
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:51:43.84 -00:26:00.1: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:43.84 -00:26:00.1: 14.75 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.17
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113180901047215360,2461159.6127,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113180901047215360 20260429.1127 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.48 06:59:40.54 -00:39:47.2
214.46160 1.53018 galactic Mon Second-epoch detections are separated by 2.6" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112640181842895232 | 06:59:40.85 -00:39:03.3 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:40.54 -00:39:47.2: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:40.54 -00:39:47.2: 15.61 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112640181842895232,2461159.6127,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112640181842895232 20260429.1127 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.40 07:07:25.54 +01:35:35.0
213.33579 4.28327 galactic Mon Second-epoch detections are separated by 1.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.8633+01.6057 | 07:07:25.05 +01:36:00.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:25.54 +01:35:35.0: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:25.54 +01:35:35.0: 15.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.8633+01.6057,2461159.6127,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J106.8633+01.6057 20260429.1127 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 29.1127 2461159.6127 12.46 07:02:02.01 +00:07:45.7
214.02525 2.41634 galactic Mon Second-epoch detections are separated by 3.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.5011+00.1277 | 07:02:01.39 +00:08:10.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1949AnHar.112....1C HD 293049
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:02.01 +00:07:45.7: 14.88 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:02.01 +00:07:45.7: 15.60 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J105.5011+00.1277,2461159.6127,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J105.5011+00.1277 20260429.1127 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 29.1127 2461159.6127 12.55 06:54:48.35 +00:23:18.3
212.97014 0.92646 galactic Mon Second-epoch detections are separated by 4.1" and 6.6 pix
The object was found in VSX 4" ZTF J065448.56+002321.1
Type: EW
# Max. Min./Amp. JD0 Period
14.331 r Y 0.168 r 2458205.63470 0.489308400000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:48.35 +00:23:18.3: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:48.35 +00:23:18.3: 15.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J065448.56+002321.1,2461159.6127,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J065448.56+002321.1 20260429.1127 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 29.1127 2461159.6127 12.34 07:01:07.55 -01:29:23.1
215.36284 1.47510 galactic Mon Second-epoch detections are separated by 1.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3109157130864532480 | 07:01:08.74 -01:29:57.0 (Gaia DR3) | E (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: G8 1956ApJS....2..271M LF 9 -02 601 J-Ks=0.339+/-0.042 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:07.55 -01:29:23.1: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:07.55 -01:29:23.1: 15.42 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109157130864532480,2461159.6127,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109157130864532480 20260429.1127 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 29.1127 2461159.6127 12.47 06:51:24.84 -03:32:35.6
216.08346 -1.62015 galactic Mon Second-epoch detections are separated by 1.3" and 7.0 pix
The object was found in VSX22" BEST-II LRa02a2_21410
Type: EA
# Max. Min./Amp. JD0 Period
16.980 CR Y 0.370 CR 2454435.33000 3.880000000000
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:51:24.84 -03:32:35.6: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:24.84 -03:32:35.6: 14.20 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 LRa02a2_21410,2461159.6127,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 LRa02a2_21410 20260429.1127 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 29.1127 2461159.6127 12.68 06:48:35.72 -00:00:04.6
212.60900 -0.63305 galactic Mon Second-epoch detections are separated by 1.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113451174747949312 | 06:48:35.04 +00:00:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1949AnHar.112....1C HD 292414 J-Ks=0.536+/-0.072 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:48:35.72 -00:00:04.6: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:48:35.72 -00:00:04.6: 13.39 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113451174747949312,2461159.6127,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113451174747949312 20260429.1127 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 29.1127 2461159.6127 12.62 06:55:36.32 -01:20:46.1
214.60503 0.31317 galactic Mon Second-epoch detections are separated by 1.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112125060645731072 | 06:55:37.26 -01:21:05.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:55:36.32 -01:20:46.1: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:55:36.32 -01:20:46.1: 15.49 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112125060645731072,2461159.6127,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112125060645731072 20260429.1127 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 29.1127 2461159.6127 12.46 06:58:22.85 -04:38:15.2
217.84982 -0.57287 galactic Mon Second-epoch detections are separated by 1.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3101684166946863104 | 06:58:22.21 -04:37:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:58:22.85 -04:38:15.2: 14.70 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:22.85 -04:38:15.2: 15.05 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.05 +/- 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 3101684166946863104,2461159.6127,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101684166946863104 20260429.1127 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 29.1127 2461159.6127 12.84 07:02:49.62 -03:11:40.1
217.07358 1.07325 galactic Mon Second-epoch detections are separated by 3.3" and 6.7 pix
The object was found in VSX 2" Gaia DR3 3108625826231054976
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.980 G 14.010 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:49.62 -03:11:40.1: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:49.62 -03:11:40.1: 15.56 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108625826231054976,2461159.6127,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108625826231054976 20260429.1127 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 29.1127 2461159.6127 12.69 06:58:24.63 -03:02:35.3
216.43480 0.16198 galactic Mon Second-epoch detections are separated by 1.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3102885172944943488 | 06:58:26.11 -03:02:13.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9 1956ApJS....2..271M LF 9 -03 415
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:58:24.63 -03:02:35.3: 14.29 +/- 0.22 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:24.63 -03:02:35.3: 15.33 +/- 0.36 detection
Forced photometry reference-image weighted average: 14.58 +/- 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 3102885172944943488,2461159.6127,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102885172944943488 20260429.1127 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 29.1127 2461159.6127 12.81 06:51:17.46 -02:53:48.6
215.49381 -1.35312 galactic Mon Second-epoch detections are separated by 2.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3105855610985039744 | 06:51:16.04 -02:54:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.925+/-0.044 (M)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:51:17.46 -02:53:48.6: 13.51 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:17.46 -02:53:48.6: 14.39 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105855610985039744,2461159.6127,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105855610985039744 20260429.1127 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 29.1127 2461159.6127 12.73 07:00:55.05 -03:04:10.5
216.74438 0.70656 galactic Mon Second-epoch detections are separated by 0.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3108690216381698304 | 07:00:56.90 -03:03:39.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 1949AnHar.112....1C HD 295921
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:00:55.05 -03:04:10.5: 14.63 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:00:55.05 -03:04:10.5: 15.29 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.29 +/- 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
Gaia DR3 3108690216381698304,2461159.6127,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108690216381698304 20260429.1127 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 29.1127 2461159.6127 12.88 06:48:53.21 +01:49:29.8
211.01698 0.26469 galactic Mon Second-epoch detections are separated by 2.0" and 6.5 pix
The object was found in VSX 3" Gaia DR3 3126153111029053568
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.860 G 13.900 G F
The object was found in astcheck.391 Ingeborg 495 286 571 16.2 -0 0
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:48:53.21 +01:49:29.8: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:48:53.21 +01:49:29.8: 13.67 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.67 +/- 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 3126153111029053568,2461159.6127,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126153111029053568 20260429.1127 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 29.1127 2461159.6127 12.92 06:49:37.18 -02:17:20.0
214.76225 -1.44780 galactic Mon Second-epoch detections are separated by 1.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.4066-02.2885 | 06:49:37.58 -02:16:51.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B5 1949AnHar.112....1C HD 292508
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:49:37.18 -02:17:20.0: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:49:37.18 -02:17:20.0: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.4066-02.2885,2461159.6127,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J102.4066-02.2885 20260429.1127 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 29.1127 2461159.6127 13.06 06:51:34.31 -01:39:23.8
214.42162 -0.72552 galactic Mon Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.9043-01.6544 | 06:51:34.96 -01:38:50.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0: 1956ApJS....2..271M LF 9 -02 199
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:51:34.31 -01:39:23.8: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:34.31 -01:39:23.8: 15.46 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J102.9043-01.6544,2461159.6127,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J102.9043-01.6544 20260429.1127 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 29.1127 2461159.6127 13.27 06:54:26.43 +00:45:45.7
212.59534 1.01581 galactic Mon Second-epoch detections are separated by 2.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113778687474978304 | 06:54:24.47 +00:45:50.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:26.43 +00:45:45.7: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:26.43 +00:45:45.7: 15.57 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113778687474978304,2461159.6127,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113778687474978304 20260429.1127 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AK Mon,2461159.6127,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AK Mon 20260429.1127 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461120.60986138 21.03.2026 02:38:02.023 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
First image: 2461120.60986138 21.03.2026 02:38:02.023 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Last image: 2461159.61294988 29.04.2026 02:42:28.870 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.94
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: 6 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): 29298
Objects passed selection criteria: 29176
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 21024.2
Average stars matched: 20581.5 (97.8941 %)
Memory usage VmPeak: 133820 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 28 21:44:54 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: 2461120.60986138 21.03.2026 02:38:02.023 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
First image: 2461120.60986138 21.03.2026 02:38:02.023 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Last image: 2461159.61294988 29.04.2026 02:42:28.870 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 392
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
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: 59 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): 180985
Objects passed selection criteria: 180661
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 146070
Average stars matched: 141588 (96.9323 %)
Memory usage VmPeak: 2154572 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 28 21:48:58 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/TTUQ2b1x1/TTUQ2_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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.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: 2461159.61239023
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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits'
wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Image size: 921.1'x633.5' 15.4(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.77"/pix along the X axis and 5.95"/pix along the Y axis
Image center: 06:51:17.088 -01:58:30.73 J2000 4789.000 3195.000
###################################
The image scale is 5.77"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:31.626 -01:58:29.66 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:17.088 -01:58:30.73
Second-epoch image center 06:51:31.626 -01:58:29.66
Angular distance between the image centers 0.0605 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:31.645 -01:59:10.06 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:17.088 -01:58:30.73
Second-epoch image center 06:51:31.645 -01:59:10.06
Angular distance between the image centers 0.0616 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 06:51:31.626 -01:58:29.66
Second-epoch second image center 06:51:31.645 -01:59:10.06
Angular distance between the image centers 0.01122 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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.6quHQbctFP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.E8Mic0MQ9K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits &> /tmp/tmp.N45yRnZHxl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits &> /tmp/tmp.TaOlKbflzs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits) and catalog (wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat) found
'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat' -> 'wcsmag.cat'
Read 36541 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9458 to 110.5184 deg, Dec -7.3465 to +3.3006 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 94.9458 to 110.5184 deg, Dec -7.3465 to 3.3006 deg
Loaded 23388 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): 309 out of 336 total matches.
Matched with Tycho-2 336 out of 36541 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.830495
a=0.000000 b=1.000000 c=22.830495
From vast_summary.log: estimated ref. image limiting mag.: -7.94
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36541 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9458 to 110.5184 deg, Dec -7.3465 to +3.3006 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 94.9458 to 110.5184 deg, Dec -7.3465 to 3.3006 deg
Loaded 23388 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): 309 out of 336 total matches.
Matched with Tycho-2 336 out of 36541 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (aperture=6.4)
Read 36462 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9286 to 110.5255 deg, Dec -7.3103 to +3.2986 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 94.9286 to 110.5255 deg, Dec -7.3103 to 3.2986 deg
Loaded 23325 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): 2099 out of 2264 total matches.
Matched with Tycho-2 2264 out of 36462 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.5 pix Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
2.4 pix wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.5 pix wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Limiting magnitude estimates:
14.9 mag. Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
14.9 mag. Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
13.8 mag. fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
13.9 mag. fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.0 (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.6quHQbctFP (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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits' -> 'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3925, passed=36541
Got 36541 stars (including 32595 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 36541 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 921.1'
Seting catalog search parameters based on the expected field of view 921.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012793 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010234 (36.8 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 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 436 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 320 matched stars entering correct_measured_positions(), 244 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 319 matched stars entering correct_measured_positions(), 9295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.07"
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 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 469 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 374 matched stars entering correct_measured_positions(), 9331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.04"
Accuracy estimation diagnostic: 371 matched stars entering correct_measured_positions(), 11803 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.95"
Excluding outliers - 371 stars left (next iteration limit 350)
The image catalog is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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.E8Mic0MQ9K (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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.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-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3920, passed=36462
Got 36462 stars (including 32518 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 36462 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.5'
Seting catalog search parameters based on the expected field of view 924.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012840 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010272 (37.0 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 634 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 574 matched stars entering correct_measured_positions(), 509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 574 matched stars entering correct_measured_positions(), 17673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.15"
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 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 682 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 641 matched stars entering correct_measured_positions(), 17690 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.07"
Accuracy estimation diagnostic: 640 matched stars entering correct_measured_positions(), 19306 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.84"
Excluding outliers - 640 stars left (next iteration limit 631)
The image catalog is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.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.N45yRnZHxl (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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1077, passed=12597
Got 12597 stars (including 11515 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 12597 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 12194 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 12190 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 12191 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 919 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.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.TaOlKbflzs (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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1278, passed=13898
Got 13898 stars (including 12608 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 13898 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 468 (Dec -7.3 to 3.4)
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: 930 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 13574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
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 468 (Dec -7.3 to 3.4)
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: 930 matched stars entering correct_measured_positions(), 13572 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 13572 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.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-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out06854.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51582_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 51582_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:10:16.93 +01:29:55.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51585_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 51585_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:17.06 +01:47:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51586_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 51586_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:27.21 -03:06:41.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51636_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 51636_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:43.89 +00:27:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.41, MAG_FAINT_SEARCH_LIMIT=11.39)GAIADR2_OUTPUT=# 3.167 3113576720930987264 102.93221130906 +00.46345044461 11.3198 11.1541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06854_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 06854_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:17:30.99 +01:05:37.9
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Image size: 921.1'x633.5' 15.4(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.77"/pix along the X axis and 5.95"/pix along the Y axis
Image center: 06:51:17.088 -01:58:30.73 J2000 4789.000 3195.000
###################################
The image scale is 5.77"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:31.626 -01:58:29.66 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:17.088 -01:58:30.73
Second-epoch image center 06:51:31.626 -01:58:29.66
Angular distance between the image centers 0.0605 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
Image size: 937.4'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:31.645 -01:59:10.06 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:17.088 -01:58:30.73
Second-epoch image center 06:51:31.645 -01:59:10.06
Angular distance between the image centers 0.0616 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 06:51:31.626 -01:58:29.66
Second-epoch second image center 06:51:31.645 -01:59:10.06
Angular distance between the image centers 0.01122 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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.4hq3ichybq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.ADqrJ49aGs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits &> /tmp/tmp.E7YLyz5OmA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits &> /tmp/tmp.F2LZKfAP30
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits) and catalog (wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat) found
'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat' -> 'wcsmag.cat'
Read 220722 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9439 to 110.5351 deg, Dec -7.3473 to +3.3081 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 94.9439 to 110.5351 deg, Dec -7.3473 to 3.3081 deg
Loaded 23446 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): 371 out of 484 total matches.
Matched with Tycho-2 484 out of 220722 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.868254
a=0.000000 b=1.000000 c=21.868254
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.20
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 220722 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9439 to 110.5351 deg, Dec -7.3473 to +3.3081 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 94.9439 to 110.5351 deg, Dec -7.3473 to 3.3081 deg
Loaded 23446 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): 371 out of 484 total matches.
Matched with Tycho-2 484 out of 220722 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (aperture=5.0)
Read 220494 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 94.9245 to 110.5311 deg, Dec -7.3125 to +3.2993 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 94.9245 to 110.5311 deg, Dec -7.3125 to 3.2993 deg
Loaded 23349 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): 1804 out of 2528 total matches.
Matched with Tycho-2 2528 out of 220494 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 315 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.4 pix Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
2.3 pix fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
2.3 pix wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.4 pix wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Limiting magnitude estimates:
14.2 mag. Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
14.2 mag. Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
13.1 mag. fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
13.2 mag. fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.6 (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.4hq3ichybq (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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits' -> 'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=38776, passed=220694
Got 220694 stars (including 181701 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 220694 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 921.1'
Seting catalog search parameters based on the expected field of view 921.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012793 (46.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010234 (36.8 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 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 418 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 311 matched stars entering correct_measured_positions(), 233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.15"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 307 matched stars entering correct_measured_positions(), 49872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.33"
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 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 451 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 367 matched stars entering correct_measured_positions(), 49901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.32"
Accuracy estimation diagnostic: 364 matched stars entering correct_measured_positions(), 64427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.21"
Excluding outliers - 364 stars left (next iteration limit 337)
The image catalog is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.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.ADqrJ49aGs (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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.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-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=38902, passed=220472
Got 220472 stars (including 181352 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 220472 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.5'
Seting catalog search parameters based on the expected field of view 924.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012840 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010272 (37.0 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 633 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 556 matched stars entering correct_measured_positions(), 490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.15"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 554 matched stars entering correct_measured_positions(), 100492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.72"
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 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 668 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 620 matched stars entering correct_measured_positions(), 100512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.71"
Accuracy estimation diagnostic: 619 matched stars entering correct_measured_positions(), 116714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.90"
Excluding outliers - 619 stars left (next iteration limit 609)
The image catalog is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.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.E7YLyz5OmA (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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=9042, passed=102694
Got 102694 stars (including 93545 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 102694 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 99939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 99939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 99939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 922 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.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.F2LZKfAP30 (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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=10507, passed=113036
Got 113036 stars (including 102413 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 113036 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 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 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 110705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 110702 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 110700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 923 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.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-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-41-40_20.00sec_-4.90C_LIGHT_0020.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.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_2026-04-28_CI_Mon-02-Q2b1x1_214314_TTUQ2b1x1_300242_5T9QiSto/wcs_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021.fits
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out246444.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246631.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246656.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246659.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246677.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246708.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246743.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246752.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out247648.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out248034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out247628.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out129332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246438.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out246502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248047.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 280s
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: 79s
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Considering the candidate 246438_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246438_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246442_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246442_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246444_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246444_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:55:34.92 -03:51:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.926 3102547043057746176 103.89516294362 -03.85569390586 13.8935 13.3553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246453_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246453_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:58:59.29 -01:25:18.6: 13.33 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:59.29 -01:25:18.6: 13.11 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.04
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Considering the candidate 246454_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246454_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:41.59 -01:02:04.7: 14.17 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:41.59 -01:02:04.7: 13.29 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
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Considering the candidate 246460_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246460_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246461_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246461_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246462_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246462_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246465_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246465_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246467_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246467_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:17.21 -00:29:48.4: 11.67 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:17.21 -00:29:48.4: 12.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.03 +/- 0.01
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Considering the candidate 246474_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246474_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:02.90 -02:37:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.444 3108918021446066560 104.76186466960 -02.61869835104 13.8699 13.3939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246477_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246477_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:18:24.43 +01:34:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 4.355 3111877391353331200 109.60277358536 +01.56957046220 13.3338 12.6662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246484_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246484_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:42:59.45 -00:24:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.126 3119455401588618496 100.74732956184 -00.41078656802 13.8492 13.2626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246487_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246487_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:55:52.03 -00:57:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.374 3112427873020082304 103.96604863601 -00.96298805966 13.6983 12.9359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246489_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246489_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246497_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246497_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246499_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246499_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:15:54.52 -00:50:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 2.837 3110149444409507456 108.97638845846 -00.83454229676 13.4745 12.9937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246502_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246502_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246512_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246512_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246517_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246517_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246518_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246518_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:05:19.33 -01:29:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.517 3109468056438096000 106.33034015352 -01.48790042039 13.5034 12.6642 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 246519_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246519_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:44.70 -03:53:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 2.151 3101831256687593728 105.68604330241 -03.89400517000 13.3060 12.9603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246521_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246521_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:05:38.50 -03:16:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 2.908 3107883110426703488 106.40991401759 -03.26888291942 13.3133 12.9423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246522_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246522_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:55:05.07 -01:02:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.076 3112333899136721408 103.77089108376 -01.04932192669 13.4551 12.7464 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 246525_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246525_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:06.61 +00:28:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 3.141 3113392007278549888 103.27695675982 +00.46879719149 13.5732 13.0519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246530_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246530_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246531_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246531_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246532_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246532_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246535_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246535_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:17:10.63 -04:16:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.092 3059711100832943616 109.29405056817 -04.27541791002 13.0768 12.1579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246536_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246536_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246537_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246537_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:05:49.73 +01:33:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.977 3114733102226564608 106.45677691624 +01.55902096947 13.5132 13.0159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246541_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246541_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246549_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246549_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246553_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246553_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:27.30 -01:29:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.785 3106335066773835264 102.86322551194 -01.49193002968 13.3529 12.3988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246554_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246554_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:33.16 +02:06:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246555_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246555_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:09:13.74 +01:24:58.6: 12.90 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:09:13.74 +01:24:58.6: 15.46 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.90 +/- 0.07
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Considering the candidate 246556_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246556_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246557_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246557_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 246559_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246559_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:39.20 -00:21:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.254 3109664456700761600 107.16306297148 -00.36135835888 13.1910 12.3130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246560_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246560_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246562_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246562_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246565_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246565_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:44:16.57 -00:10:04.4: 14.24 +/- 0.21 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:16.57 -00:10:04.4: 12.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.03
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Considering the candidate 246569_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246569_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246570_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246570_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246576_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246576_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:10:06.52 -05:42:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.298 3053144301998173952 107.52731439341 -05.70202379804 12.9303 12.4197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246578_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246578_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246582_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246582_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:58:53.97 +00:32:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 2.642 3112971822037304448 104.72483387692 +00.53662840684 13.2525 12.4300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246583_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246583_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246584_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246584_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:06.27 -02:04:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.742 3106231162926784256 102.77580301690 -02.08169042820 13.3129 12.8657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246585_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246585_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246588_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246588_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:52.64 -00:06:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 2.400 3113333694502694016 103.21920072535 -00.10273675864 13.1280 12.2459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246595_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246595_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:06:33.48 -02:33:38.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)
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Considering the candidate 246597_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246597_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:06.99 +01:29:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 5.694 3114681661400627968 106.77870860938 +01.48264087515 13.3404 12.6380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246604_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246604_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246605_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246605_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:49:16.59 +01:46:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.534 3126140157407667328 102.31874322026 +01.77582510479 13.2369 12.8437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246606_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246606_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:07.29 +02:07:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246607_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246607_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:45.98 +01:52:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246608_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246608_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246609_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246609_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:58.81 -02:58:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 2.622 3107963993251302912 106.99440881430 -02.97752881737 12.9544 12.4417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246612_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246612_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246615_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246615_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:05:01.42 +01:48:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.641 3114755436055724928 106.25598204354 +01.81022333530 13.0723 12.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246617_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246617_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246620_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246620_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:08.90 +00:19:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.985 3113375033568592256 103.53660221403 +00.31943571180 13.1145 12.2753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246624_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246624_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:51:28.97 +01:57:03.4: 13.87 +/- 0.16 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:28.97 +01:57:03.4: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.04
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Considering the candidate 246625_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246625_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246626_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246626_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246629_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246629_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:42.76 +02:18:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246631_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246631_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:01.30 -01:37:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 3.411 3106285382592168960 103.00494216818 -01.61926474040 13.1404 12.6260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246633_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246633_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:57:07.32 +00:11:06.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)
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Considering the candidate 246635_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246635_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:22.78 +00:47:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.290 3114352426386304384 106.84475170251 +00.79641349732 13.2005 12.4883 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 246636_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246636_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:35.61 -03:12:28.6: 10.72 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:35.61 -03:12:28.6: 15.53 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.72 +/- 0.01
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Considering the candidate 246637_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246637_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246639_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246639_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:40:33.17 +01:52:24.9: 14.87 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:40:33.17 +01:52:24.9: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.03
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Considering the candidate 246640_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246640_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246642_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246642_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:13:09.25 +00:52:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.605 3111397905500984320 108.28854184748 +00.87385961036 13.1711 12.4219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246644_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246644_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246645_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246645_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246649_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246649_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246650_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246650_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:26.21 +01:38:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 3.592 3115403838680806016 105.85881404359 +01.64175011941 13.1156 12.2747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246651_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246651_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246652_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246652_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246655_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246655_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:37:29.75 +01:45:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246656_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246656_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:33.14 +00:32:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 3.342 3114294122208651008 107.13787303785 +00.53631806316 13.1529 12.4015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246657_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246657_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:43:43.94 -01:42:12.6: 14.92 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:43.94 -01:42:12.6: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.03
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Considering the candidate 246658_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246658_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:54.54 -05:18:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 2.690 3101952447785931648 102.22673217314 -05.31126321634 12.9501 12.3869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246659_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246659_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:03.17 -00:37:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.579 3113194232625197056 102.51282878943 -00.62797430687 13.1829 12.7117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246660_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246660_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:06:42.26 -03:09:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 2.521 3107979111536590592 106.67588059035 -03.15417042601 13.0043 12.3122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246661_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246661_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246664_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246664_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246671_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246671_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246676_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246676_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:02.45 +01:07:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246677_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246677_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:17:38.33 +01:13:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.045 3111755968334593536 109.41025479268 +01.21751632338 12.8697 12.1561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246678_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246678_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246682_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246682_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246683_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246683_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246687_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246687_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246688_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246688_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:08.24 -05:53:01.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 246691_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246691_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:42:58.25 +02:07:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 2.562 3126780382412815744 100.74233929542 +02.12628035814 13.0041 12.3850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246693_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246693_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:32.01 -00:25:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.615 3119372697696534784 100.13273373346 -00.42928554201 12.8212 11.9990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246695_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246695_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:58.93 -00:19:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 2.071 3113267723803628032 103.49523763159 -00.32101610671 12.7027 11.7159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246696_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246696_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246697_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246697_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246698_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246698_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246700_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246700_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:26.60 +01:01:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 2.911 3113672412805244544 102.61053048368 +01.02430569162 12.2346 11.0584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246702_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246702_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246703_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246703_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246704_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246704_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:13.40 -00:19:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246705_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246705_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:37.18 -04:14:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 2.983 3101747972982311552 105.40574746029 -04.24506783820 12.7532 12.0169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246706_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246706_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246708_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246708_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:07.00 -01:27:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 3.461 3112284318034616192 103.52878928410 -01.46702302221 12.8078 12.2175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246710_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246710_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:09.54 -00:31:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 1.937 3109654664175447040 107.03933749885 -00.53365091178 12.7814 12.0137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246711_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246711_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246712_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246712_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:10:32.38 +02:01:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.067 3115091160759117056 107.63445348678 +02.02860480844 12.8638 12.0750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246713_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246713_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:49.73 +01:05:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 1.926 3114600881653061376 105.95718131582 +01.09466021958 12.6217 12.1501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246716_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246716_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:16.52 -05:08:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 2.765 3101410075013963264 105.56849423180 -05.14018986688 12.1954 11.2080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246718_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246718_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246719_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246719_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:56:24.06 +01:22:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.392 3114102218772312704 104.10002976772 +01.37115075284 12.7076 11.9544 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 246723_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246723_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246724_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246724_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246726_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246726_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:59.70 +00:10:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 2.059 3119546935930633600 100.24843993955 +00.16765835915 12.7899 12.3203 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246727_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246727_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:37:33.19 +00:36:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 1.637 3119819408654913152 099.38863803077 +00.60489964142 12.7958 12.2404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246728_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246728_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246730_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246730_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:00.75 +01:40:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.985 3115395244446320512 105.50309509202 +01.66881056532 12.6269 12.1565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246735_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246735_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246739_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246739_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:04:15.68 -02:22:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246740_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246740_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:12:40.35 +01:01:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246741_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246741_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:09:21.34 +02:14:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 3.277 3115156963958576256 107.33847751877 +02.23567456553 12.4681 12.0482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246742_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246742_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:03.23 -02:17:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 1.592 3108998320154606464 104.76311203704 -02.29796996872 12.4004 11.6148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246743_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246743_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:12:11.63 +00:30:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.859 3111363988141876864 108.04845873087 +00.50334469064 12.3696 11.7618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246744_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246744_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246746_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246746_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246748_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246748_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:46:26.29 +00:44:10.7: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:46:26.29 +00:44:10.7: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
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Considering the candidate 246750_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246750_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:12:39.28 -02:45:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 1.763 3108170594059818752 108.16354020929 -02.75847317301 12.1337 11.5651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246751_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246751_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246752_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246752_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:55:15.03 -00:55:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 2.570 3112431991889463424 103.81260449157 -00.91865812326 12.2315 11.3893 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 246754_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246754_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:11:39.57 -00:56:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 1.677 3109383424102195072 107.91479278939 -00.94259728715 12.2917 11.8590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246759_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246759_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:10:59.23 -03:55:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246760_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246760_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:57:05.71 +01:24:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 1.910 3114108059926391040 104.27346090126 +01.41316855347 12.1037 11.3783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246761_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246761_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:16.82 +02:09:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246762_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246762_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:35.68 +01:46:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246763_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246763_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246765_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246765_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:09:33.51 -03:59:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 0.673 3107642386103795456 107.38961875804 -03.98679803136 12.1264 11.3871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246767_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246767_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246769_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246769_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:05:16.02 -02:53:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 0.405 3108002059542766720 106.31665080241 -02.88660911930 12.2073 11.4382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246770_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246770_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:47:13.00 +00:51:25.2: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:47:13.00 +00:51:25.2: 11.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.01
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Considering the candidate 246771_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246771_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:55:15.60 -00:47:21.6: 10.08 +/- 0.00 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:55:15.60 -00:47:21.6: 15.59 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.08 +/- 0.00
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Considering the candidate 246772_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246772_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:44.42 +00:30:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246775_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246775_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:14:24.39 +01:15:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246778_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246778_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:05.78 -03:49:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 1.543 3102714546783212672 103.52372089919 -03.83109116491 11.8165 11.5615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246779_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246779_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246780_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246780_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:43.71 -02:23:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 2.127 3106589466276044672 100.18250785556 -02.38467256388 11.8484 11.4176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246781_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246781_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:52:52.48 -02:58:21.5: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:52.48 -02:58:21.5: 11.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.01
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Considering the candidate 246784_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246784_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246786_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246786_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:24.70 -05:22:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246787_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246787_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:10:17.03 +01:29:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246789_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246789_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:17.13 +01:47:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246873_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246873_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246954_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 246954_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 246983_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 246983_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:37.25 +00:26:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247030_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247030_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:11.42 -00:35:54.1: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:11.42 -00:35:54.1: 11.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.36 +/- 0.01
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Considering the candidate 247039_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247039_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:47:13.75 +01:33:06.4: 14.22 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:47:13.75 +01:33:06.4: 12.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.02
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Considering the candidate 247049_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247049_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:10.65 +01:53:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247101_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247101_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247102_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247102_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247147_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247147_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:00:37.52 -01:51:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 3.105 3109109680066395904 105.15642782143 -01.86277396635 12.3871 11.5938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247149_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247149_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:24.18 -01:27:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247173_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247173_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:47:44.09 +00:29:29.3: 13.72 +/- 0.13 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:47:44.09 +00:29:29.3: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.02
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Considering the candidate 247176_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247176_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247182_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247182_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247186_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247186_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247206_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247206_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:25.56 -05:17:27.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247215_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247215_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:05.68 +01:48:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247222_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247222_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:00.76 -04:14:53.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247231_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247231_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:45:27.68 +00:57:44.0: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:45:27.68 +00:57:44.0: 12.53 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
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Considering the candidate 247236_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247236_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:12:13.18 +00:47:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247277_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247277_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:32.72 -01:21:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247291_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247291_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:06:17.27 +02:00:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.993 3114765366020010752 106.57169428469 +02.00384672606 12.7577 12.3595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247292_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247292_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:36:41.08 -05:13:22.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247295_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247295_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247297_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247297_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:05:52.47 -01:02:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247298_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247298_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:08.23 -04:35:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247311_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247311_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:52.71 -01:19:05.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247314_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247314_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:17:28.54 -00:24:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247316_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247316_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:39:00.31 +01:56:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247327_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247327_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:50.87 -02:31:49.1: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:50.87 -02:31:49.1: 11.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.21 +/- 0.01
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Considering the candidate 247330_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247330_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:04:32.41 +01:08:09.3: 12.29 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:04:32.41 +01:08:09.3: 15.37 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.29 +/- 0.04
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Considering the candidate 247335_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247335_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247345_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247345_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:34:14.59 -04:53:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247353_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247353_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247354_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247354_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:56:49.22 -03:40:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247367_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247367_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:19.89 +01:31:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 4.472 3125766220373632256 101.83212084767 +01.53059619715 12.9717 12.4642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247369_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247369_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247379_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247379_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:10:20.77 -04:14:37.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247387_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247387_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:16.66 +02:11:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247395_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247395_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247396_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247396_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:55:49.99 -01:35:05.6: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:55:49.99 -01:35:05.6: 11.87 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
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Considering the candidate 247399_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247399_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:04.69 -02:56:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 4.685 3105853961717706752 102.76849306617 -02.94368947578 12.8768 12.1348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247417_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247417_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:44.45 -00:31:37.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247421_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247421_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247427_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247427_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247438_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247438_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:44:15.57 -03:26:22.7: 11.70 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:15.57 -03:26:22.7: 13.62 +/- 0.06 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.02
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Considering the candidate 247441_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247441_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:44:33.78 -01:39:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247442_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247442_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:13.55 +02:02:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247445_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247445_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247447_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247447_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247448_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247448_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:51.29 -01:46:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 1.931 3109234234118285952 107.21394667394 -01.77617496224 13.0380 12.3331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247451_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247451_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247460_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247460_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:09:37.60 -01:22:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.999 3109339379218885888 107.40665275024 -01.37683283674 13.0624 12.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247471_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247471_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:15:27.16 -00:49:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247472_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247472_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:41:30.12 +00:57:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 2.128 3125804325323474944 100.37578011780 +00.96206277387 13.1485 12.7058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247476_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247476_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:00:06.67 -02:51:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247478_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247478_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247480_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247480_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247485_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247485_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247486_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247486_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:10:16.02 -02:20:54.2: 11.84 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:10:16.02 -02:20:54.2: 13.45 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.27 +/- 0.03
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Considering the candidate 247487_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247487_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:39.47 +02:11:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247499_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247499_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247503_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247503_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:39:44.30 +00:57:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 5.738 3119848820590668032 099.93359793985 +00.95608028773 12.8460 11.9304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247507_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247507_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:09.52 -05:52:27.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247509_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247509_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:13.70 +01:34:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.818 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247515_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247515_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 247517_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247517_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:30.13 -04:07:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247521_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247521_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:00:21.41 -05:50:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.565 3100935640049817728 105.08895116582 -05.84376213725 12.7701 11.8846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247533_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247533_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247536_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247536_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:50.17 +00:16:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.627 3112948006440304640 104.95896919067 +00.27146844100 13.2300 12.8150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247538_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247538_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:51.30 -01:22:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247539_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247539_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:25.91 -01:17:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.583 3107094447052075136 101.85775483899 -01.29002878528 13.2204 12.7533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247544_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247544_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247546_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247546_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:37:58.56 -01:25:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247552_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247552_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247554_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247554_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:56:27.57 +00:06:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.832 3113677261828133888 104.11429280310 +00.10422085836 13.1732 12.4789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247559_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247559_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:00.63 -02:52:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247567_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247567_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:15:41.91 -03:23:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 2.743 3060026248353746688 108.92463740659 -03.39203949534 12.8586 11.9322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247569_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247569_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:28.98 -00:00:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247575_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247575_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247577_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247577_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:04.82 -01:02:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 3.196 3107346681891637888 101.26967865935 -01.04031808691 13.2059 12.6723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247597_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247597_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:05.72 +00:15:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 3.311 3113554112226157568 102.52351755616 +00.25513630730 13.0221 12.1110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247599_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247599_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247603_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247603_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:26.28 +02:03:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247604_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247604_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:45.44 -01:43:47.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247624_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247624_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247628_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247628_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:35.26 -01:19:40.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)
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Considering the candidate 247630_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247630_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:44:31.63 +00:07:37.1: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:31.63 +00:07:37.1: 13.13 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.05
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Considering the candidate 247633_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247633_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:11.80 +01:50:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247637_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247637_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:57.39 -03:04:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247643_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247643_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:25.70 -05:20:08.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247648_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247648_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:12:18.77 +00:29:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.735 3111363167805876992 108.07802448996 +00.48541087422 12.9942 12.1878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247654_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247654_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247657_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247657_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:35:16.46 -04:45:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247665_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247665_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247670_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247670_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:11:28.43 -00:18:59.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247671_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247671_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:00.69 +00:23:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 3.998 3119568410766803968 100.75309723994 +00.39363410704 13.2345 12.5585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247672_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247672_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247673_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247673_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:39.65 -04:37:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247680_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247680_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:07.34 -01:52:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247683_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247683_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247686_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247686_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247688_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247688_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:18.33 +01:32:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 5.007 3125769175311132288 101.82503425206 +01.53365566575 13.0807 12.1097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247691_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247691_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:43:50.56 -01:04:06.6: 14.98 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:50.56 -01:04:06.6: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.03
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Considering the candidate 247699_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247699_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247703_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247703_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:48:16.64 -01:48:38.2: 10.97 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:48:16.64 -01:48:38.2: 13.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 11.10 +/- 0.01
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Considering the candidate 247705_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247705_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:58:39.12 -04:20:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 3.928 3101710349067118720 104.66302468638 -04.33867408529 13.0563 12.0264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247707_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247707_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:04:20.72 -00:08:22.0: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:04:20.72 -00:08:22.0: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.04
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Considering the candidate 247708_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247708_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:15.20 -05:59:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247711_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247711_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:44:36.20 +01:45:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247727_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247727_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247728_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247728_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247732_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247732_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247736_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247736_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247741_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247741_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247742_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247742_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:23.10 -01:59:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 2.477 3106212776163414144 101.84609672672 -01.99519846415 13.3080 12.7592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247752_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247752_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:01.00 -03:20:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247753_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247753_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247760_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247760_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:47:04.07 -03:46:14.1: 10.72 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:47:04.07 -03:46:14.1: 14.44 +/- 0.15 detection
Forced photometry reference-image weighted average: 10.73 +/- 0.01
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Considering the candidate 247763_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247763_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:07.39 -03:02:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.626 3105838465475537920 103.03011982126 -03.03664024423 13.3838 12.5115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247767_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247767_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:11.94 +01:45:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247769_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247769_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:06.13 -00:02:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 2.727 3107483330569016576 101.27521621046 -00.04654528542 13.5111 12.9685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247773_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247773_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:11:26.70 -01:03:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 5.244 3109380129868098176 107.86006082161 -01.05220251966 13.3067 12.8199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247783_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247783_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:22.90 -06:08:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.131 3052874406254774656 105.34484077065 -06.13892768243 13.2836 12.7701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247788_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247788_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:23.97 +01:48:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247790_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247790_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:37.50 -00:31:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 4.664 3112646160437322112 104.90516011811 -00.52192288748 13.4503 12.5426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247794_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247794_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:52.97 -04:47:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.607 3101629122646359040 104.96985275355 -04.79110958798 13.3251 12.7714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247804_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247804_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247806_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247806_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:15.36 -01:41:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 3.080 3109119408172694912 105.31457972897 -01.68746275311 13.5274 12.5235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247807_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247807_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:17:26.12 +01:37:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.026 3111920547185261696 109.35876621578 +01.62744516688 13.1980 12.9185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247810_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247810_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:55.12 -02:23:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 2.667 3106018510504636160 103.22925868247 -02.38539636749 13.5296 12.9702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247813_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247813_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247834_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247834_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247858_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247858_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:41:47.08 -00:16:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.595 3119468149051361920 100.44582555146 -00.27157940447 13.7130 13.3699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247865_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247865_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:19.52 -03:20:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.219 3108619920658643968 105.58111518078 -03.34490994692 13.4942 12.9329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247872_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247872_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247874_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247874_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:39:58.56 -01:44:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.105 3106839811330382464 099.99353216035 -01.74109541440 13.4396 12.9835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247878_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247878_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:16:56.03 -05:22:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247891_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247891_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247892_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247892_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:46:29.68 -00:12:58.0: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:46:29.68 -00:12:58.0: 13.38 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.05
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Considering the candidate 247905_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247905_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:26.57 +00:47:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 3.777 3113601086287321216 103.11008331811 +00.78771273287 13.7467 13.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247906_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247906_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:55.09 +01:18:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.739 3125843495425360640 100.97899243064 +01.29945169565 13.6672 13.2128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247938_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247938_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:00.28 -00:27:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 5.705 3112649836929196672 105.25161924724 -00.46612989853 13.7232 13.2855 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247944_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247944_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:37.27 +00:28:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 4.110 3113532877908279936 101.90503476239 +00.48169308884 13.6277 13.1530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247945_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247945_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247954_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247954_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:59.65 -02:44:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 3.569 3105945972795426816 103.49787131933 -02.73864765651 13.4074 12.4613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247956_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247956_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:32.37 -05:17:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.257 3101401244562695680 105.38457775638 -05.28896930257 12.4362 11.2755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247962_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247962_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247964_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 247964_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 247997_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 247997_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:56:40.66 -02:50:20.5: 14.79 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:56:40.66 -02:50:20.5: 10.09 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.09 +/- 0.00
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Considering the candidate 248001_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 248001_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:44:24.93 -00:04:49.3: 9.76 +/- 0.00 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:24.93 -00:04:49.3: 13.76 +/- 0.08 detection
Forced photometry reference-image weighted average: 9.77 +/- 0.00
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Considering the candidate 248002_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 248002_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 248013_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 248013_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:45:54.72 +00:18:11.2: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:45:54.72 +00:18:11.2: 13.55 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.05
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Considering the candidate 248014_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 248014_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:06:39.77 -02:47:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.620 3108029448552969984 106.66546376749 -02.79246343920 13.7321 12.9686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248026_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 248026_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 248028_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 248028_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:28.70 -01:01:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.557 3107173165213600896 101.86916799478 -01.02454829849 12.9061 10.7625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248034_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 248034_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:59.57 -01:03:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 4.044 3112333791758054272 103.74773607348 -01.05207476769 13.3921 12.4083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248047_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 248047_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
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Considering the candidate 37203_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
The candidate 37203_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021 did not pass the final checks
**** FOUND 07:17:30.92 +01:05:36.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 129332_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
Preparing report for the candidate 129332_fd_Mon-02-Q2b1x1_2026-04-28_21-42-28_20.00sec_-5.00C_LIGHT_0021
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 366s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:17:30.99 +01:05:37.9
07:12:49.76 -03:03:25.8
06:53:36.50 -04:59:47.9
06:52:12.49 -00:22:25.6
06:57:31.65 -00:23:42.1
06:55:22.99 -02:18:59.2
06:56:38.29 -04:36:28.6
07:00:08.49 -00:53:10.0
07:05:23.54 -01:12:19.8
07:02:13.77 -00:39:21.2
07:09:03.94 -01:19:31.7
07:02:35.25 -03:37:56.6
07:05:15.37 +00:02:45.6
06:57:33.46 -03:31:49.5
06:51:34.73 -01:53:52.3
06:55:03.32 +01:02:05.0
07:16:03.79 -01:38:30.1
06:53:42.63 -01:01:10.7
07:02:32.62 -02:31:08.0
07:13:43.93 -01:35:26.7
07:09:05.01 -02:57:19.9
06:51:46.27 -05:25:55.8
07:09:19.83 +00:54:53.6
06:59:30.61 -04:05:39.4
06:50:50.92 -02:36:24.6
07:08:16.27 -02:14:30.6
06:57:30.10 -00:57:11.9
07:02:50.56 -03:19:41.4
07:08:29.18 -00:58:27.6
07:05:08.38 -04:26:25.2
06:59:54.60 -02:15:14.1
07:13:59.84 -02:51:47.8
07:03:51.10 -03:43:31.4
07:01:22.61 -00:16:06.1
07:06:41.15 -02:24:48.2
07:01:21.74 +02:15:49.7
07:12:09.81 +01:52:14.8
07:12:01.96 -01:11:16.0
07:15:49.72 -00:37:02.7
07:03:14.46 +01:07:06.4
07:16:04.59 +00:48:08.0
06:50:59.48 -02:47:54.1
07:08:41.85 +01:18:46.4
07:03:36.84 -01:50:14.9
07:13:11.69 +01:02:13.4
06:46:14.65 +01:13:09.0
07:03:40.27 -01:07:51.0
07:18:18.05 -00:24:27.9
07:12:11.80 -01:59:47.9
07:16:12.87 -04:06:21.0
07:05:00.18 +01:38:42.9
06:58:21.76 -00:45:45.5
07:12:26.24 +01:50:34.4
07:01:01.01 -00:25:44.6
06:59:25.68 -01:04:49.7
07:04:20.85 -04:41:02.1
06:59:39.73 -00:40:07.6
07:06:04.88 -02:19:37.6
07:15:10.56 -04:30:19.1
07:08:48.29 +00:19:42.4
07:05:10.46 -00:00:18.8
07:16:13.30 -00:00:45.6
07:11:00.63 -02:53:39.2
07:08:43.96 -03:56:11.0
07:14:38.83 -03:56:25.0
07:17:51.22 -01:41:37.7
07:03:02.21 +01:23:57.0
06:53:07.46 -01:35:07.5
06:52:35.30 -02:12:18.2
07:05:25.02 -00:59:48.8
07:05:30.66 +01:36:36.7
06:57:39.96 -05:17:24.3
06:49:41.95 -01:43:20.2
07:01:24.19 +01:06:08.5
07:06:24.24 +00:20:29.3
07:12:29.92 +00:35:37.6
07:18:58.87 -05:26:28.5
06:52:07.82 +00:28:19.6
07:01:07.65 -03:14:32.1
06:56:36.50 +01:00:09.7
07:13:48.27 -00:49:58.9
07:00:56.86 -03:16:17.9
06:54:57.35 -01:11:47.8
07:05:49.23 +01:38:16.7
07:07:11.50 -02:58:19.4
06:52:46.18 -01:34:15.9
06:58:26.75 -00:54:23.5
07:08:12.55 -03:12:26.0
06:53:58.11 -04:52:50.6
07:01:38.39 -04:40:49.5
06:49:33.19 -01:23:29.2
06:52:53.69 +01:22:23.8
07:01:10.32 +00:00:20.0
06:57:00.78 +00:17:37.8
07:07:58.75 -00:56:39.1
07:01:46.16 +01:19:50.2
06:47:11.21 -02:50:54.0
07:08:02.93 -03:37:52.5
06:51:43.84 -00:26:00.1
06:59:40.54 -00:39:47.2
07:07:25.54 +01:35:35.0
07:02:02.01 +00:07:45.7
06:54:48.35 +00:23:18.3
07:01:07.55 -01:29:23.1
06:51:24.84 -03:32:35.6
06:48:35.72 -00:00:04.6
06:55:36.32 -01:20:46.1
06:58:22.85 -04:38:15.2
07:02:49.62 -03:11:40.1
06:58:24.63 -03:02:35.3
06:51:17.46 -02:53:48.6
07:00:55.05 -03:04:10.5
06:48:53.21 +01:49:29.8
06:49:37.18 -02:17:20.0
06:51:34.31 -01:39:23.8
06:54:26.43 +00:45:45.7
########### Completed Mon-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
07:17:30.99 +01:05:37.9
06:53:36.50 -04:59:47.9
06:52:12.49 -00:22:25.6
06:57:31.65 -00:23:42.1
06:55:22.99 -02:18:59.2
06:56:38.29 -04:36:28.6
07:00:08.49 -00:53:10.0
07:05:23.54 -01:12:19.8
07:02:13.77 -00:39:21.2
07:09:03.94 -01:19:31.7
07:02:35.25 -03:37:56.6
07:05:15.37 +00:02:45.6
06:57:33.46 -03:31:49.5
06:51:34.73 -01:53:52.3
06:55:03.32 +01:02:05.0
07:16:03.79 -01:38:30.1
06:53:42.63 -01:01:10.7
07:02:32.62 -02:31:08.0
07:13:43.93 -01:35:26.7
07:09:05.01 -02:57:19.9
06:51:46.27 -05:25:55.8
07:09:19.83 +00:54:53.6
06:59:30.61 -04:05:39.4
06:50:50.92 -02:36:24.6
07:08:16.27 -02:14:30.6
06:57:30.10 -00:57:11.9
07:02:50.56 -03:19:41.4
07:08:29.18 -00:58:27.6
07:05:08.38 -04:26:25.2
06:59:54.60 -02:15:14.1
07:13:59.84 -02:51:47.8
07:03:51.10 -03:43:31.4
07:01:22.61 -00:16:06.1
07:06:41.15 -02:24:48.2
07:01:21.74 +02:15:49.7
07:12:09.81 +01:52:14.8
07:12:01.96 -01:11:16.0
07:15:49.72 -00:37:02.7
07:03:14.46 +01:07:06.4
07:16:04.59 +00:48:08.0
06:50:59.48 -02:47:54.1
07:08:41.85 +01:18:46.4
07:03:36.84 -01:50:14.9
07:13:11.69 +01:02:13.4
06:46:14.65 +01:13:09.0
07:03:40.27 -01:07:51.0
07:18:18.05 -00:24:27.9
07:12:11.80 -01:59:47.9
07:16:12.87 -04:06:21.0
07:05:00.18 +01:38:42.9
06:58:21.76 -00:45:45.5
07:12:26.24 +01:50:34.4
07:01:01.01 -00:25:44.6
06:59:25.68 -01:04:49.7
07:04:20.85 -04:41:02.1
06:59:39.73 -00:40:07.6
07:06:04.88 -02:19:37.6
07:15:10.56 -04:30:19.1
07:08:48.29 +00:19:42.4
07:05:10.46 -00:00:18.8
07:16:13.30 -00:00:45.6
07:11:00.63 -02:53:39.2
07:08:43.96 -03:56:11.0
07:14:38.83 -03:56:25.0
07:17:51.22 -01:41:37.7
07:03:02.21 +01:23:57.0
06:53:07.46 -01:35:07.5
06:52:35.30 -02:12:18.2
07:05:25.02 -00:59:48.8
07:05:30.66 +01:36:36.7
06:57:39.96 -05:17:24.3
06:49:41.95 -01:43:20.2
07:01:24.19 +01:06:08.5
07:06:24.24 +00:20:29.3
07:12:29.92 +00:35:37.6
07:18:58.87 -05:26:28.5
06:52:07.82 +00:28:19.6
07:01:07.65 -03:14:32.1
06:56:36.50 +01:00:09.7
07:13:48.27 -00:49:58.9
07:00:56.86 -03:16:17.9
06:54:57.35 -01:11:47.8
07:05:49.23 +01:38:16.7
07:07:11.50 -02:58:19.4
06:52:46.18 -01:34:15.9
06:58:26.75 -00:54:23.5
07:08:12.55 -03:12:26.0
06:53:58.11 -04:52:50.6
07:01:38.39 -04:40:49.5
06:49:33.19 -01:23:29.2
06:52:53.69 +01:22:23.8
07:01:10.32 +00:00:20.0
06:57:00.78 +00:17:37.8
07:07:58.75 -00:56:39.1
07:01:46.16 +01:19:50.2
06:47:11.21 -02:50:54.0
07:08:02.93 -03:37:52.5
06:51:43.84 -00:26:00.1
06:59:40.54 -00:39:47.2
07:07:25.54 +01:35:35.0
07:02:02.01 +00:07:45.7
06:54:48.35 +00:23:18.3
07:01:07.55 -01:29:23.1
06:51:24.84 -03:32:35.6
06:48:35.72 -00:00:04.6
06:55:36.32 -01:20:46.1
06:58:22.85 -04:38:15.2
07:02:49.62 -03:11:40.1
06:58:24.63 -03:02:35.3
06:51:17.46 -02:53:48.6
07:00:55.05 -03:04:10.5
06:48:53.21 +01:49:29.8
06:49:37.18 -02:17:20.0
06:51:34.31 -01:39:23.8
06:54:26.43 +00:45:45.7
07:12:49.76 -03:03:25.8
###################################################################################
07:17:30.99 +01:05:37.9 -- not an asteroid (will add it to exclusion list)
06:53:36.50 -04:59:47.9 -- not an asteroid (will add it to exclusion list)
06:52:12.49 -00:22:25.6 -- not an asteroid (will add it to exclusion list)
06:57:31.65 -00:23:42.1 -- not an asteroid (will add it to exclusion list)
06:55:22.99 -02:18:59.2 -- not an asteroid (will add it to exclusion list)
06:56:38.29 -04:36:28.6 -- not an asteroid (will add it to exclusion list)
07:00:08.49 -00:53:10.0 -- not an asteroid (will add it to exclusion list)
07:05:23.54 -01:12:19.8 -- not an asteroid (will add it to exclusion list)
07:02:13.77 -00:39:21.2 -- not an asteroid (will add it to exclusion list)
07:09:03.94 -01:19:31.7 -- not an asteroid (will add it to exclusion list)
07:02:35.25 -03:37:56.6 -- not an asteroid (will add it to exclusion list)
07:05:15.37 +00:02:45.6 -- not an asteroid (will add it to exclusion list)
06:57:33.46 -03:31:49.5 -- not an asteroid (will add it to exclusion list)
06:51:34.73 -01:53:52.3 -- not an asteroid (will add it to exclusion list)
06:55:03.32 +01:02:05.0 -- not an asteroid (will add it to exclusion list)
07:16:03.79 -01:38:30.1 -- not an asteroid (will add it to exclusion list)
06:53:42.63 -01:01:10.7 -- not an asteroid (will add it to exclusion list)
07:02:32.62 -02:31:08.0 -- not an asteroid (will add it to exclusion list)
07:13:43.93 -01:35:26.7 -- not an asteroid (will add it to exclusion list)
07:09:05.01 -02:57:19.9 -- not an asteroid (will add it to exclusion list)
06:51:46.27 -05:25:55.8 -- not an asteroid (will add it to exclusion list)
07:09:19.83 +00:54:53.6 -- not an asteroid (will add it to exclusion list)
06:59:30.61 -04:05:39.4 -- not an asteroid (will add it to exclusion list)
06:50:50.92 -02:36:24.6 -- not an asteroid (will add it to exclusion list)
07:08:16.27 -02:14:30.6 -- not an asteroid (will add it to exclusion list)
06:57:30.10 -00:57:11.9 -- not an asteroid (will add it to exclusion list)
07:02:50.56 -03:19:41.4 -- not an asteroid (will add it to exclusion list)
07:08:29.18 -00:58:27.6 -- not an asteroid (will add it to exclusion list)
07:05:08.38 -04:26:25.2 -- not an asteroid (will add it to exclusion list)
06:59:54.60 -02:15:14.1 -- not an asteroid (will add it to exclusion list)
07:13:59.84 -02:51:47.8 -- not an asteroid (will add it to exclusion list)
07:03:51.10 -03:43:31.4 -- not an asteroid (will add it to exclusion list)
07:01:22.61 -00:16:06.1 -- not an asteroid (will add it to exclusion list)
07:06:41.15 -02:24:48.2 -- not an asteroid (will add it to exclusion list)
07:01:21.74 +02:15:49.7 -- not an asteroid (will add it to exclusion list)
07:12:09.81 +01:52:14.8 -- not an asteroid (will add it to exclusion list)
07:12:01.96 -01:11:16.0 -- not an asteroid (will add it to exclusion list)
07:15:49.72 -00:37:02.7 -- not an asteroid (will add it to exclusion list)
07:03:14.46 +01:07:06.4 -- not an asteroid (will add it to exclusion list)
07:16:04.59 +00:48:08.0 -- not an asteroid (will add it to exclusion list)
06:50:59.48 -02:47:54.1 -- not an asteroid (will add it to exclusion list)
07:08:41.85 +01:18:46.4 -- not an asteroid (will add it to exclusion list)
07:03:36.84 -01:50:14.9 -- not an asteroid (will add it to exclusion list)
07:13:11.69 +01:02:13.4 -- not an asteroid (will add it to exclusion list)
06:46:14.65 +01:13:09.0 -- not an asteroid (will add it to exclusion list)
07:03:40.27 -01:07:51.0 -- not an asteroid (will add it to exclusion list)
07:18:18.05 -00:24:27.9 -- not an asteroid (will add it to exclusion list)
07:12:11.80 -01:59:47.9 -- not an asteroid (will add it to exclusion list)
07:16:12.87 -04:06:21.0 -- not an asteroid (will add it to exclusion list)
07:05:00.18 +01:38:42.9 -- not an asteroid (will add it to exclusion list)
06:58:21.76 -00:45:45.5 -- not an asteroid (will add it to exclusion list)
07:12:26.24 +01:50:34.4 -- not an asteroid (will add it to exclusion list)
07:01:01.01 -00:25:44.6 -- not an asteroid (will add it to exclusion list)
06:59:25.68 -01:04:49.7 -- not an asteroid (will add it to exclusion list)
07:04:20.85 -04:41:02.1 -- not an asteroid (will add it to exclusion list)
06:59:39.73 -00:40:07.6 -- not an asteroid (will add it to exclusion list)
07:06:04.88 -02:19:37.6 -- not an asteroid (will add it to exclusion list)
07:15:10.56 -04:30:19.1 -- not an asteroid (will add it to exclusion list)
07:08:48.29 +00:19:42.4 -- not an asteroid (will add it to exclusion list)
07:05:10.46 -00:00:18.8 -- not an asteroid (will add it to exclusion list)
07:16:13.30 -00:00:45.6 -- not an asteroid (will add it to exclusion list)
07:11:00.63 -02:53:39.2 -- not an asteroid (will add it to exclusion list)
07:08:43.96 -03:56:11.0 -- not an asteroid (will add it to exclusion list)
07:14:38.83 -03:56:25.0 -- not an asteroid (will add it to exclusion list)
07:17:51.22 -01:41:37.7 -- not an asteroid (will add it to exclusion list)
07:03:02.21 +01:23:57.0 -- not an asteroid (will add it to exclusion list)
06:53:07.46 -01:35:07.5 -- not an asteroid (will add it to exclusion list)
06:52:35.30 -02:12:18.2 -- not an asteroid (will add it to exclusion list)
07:05:25.02 -00:59:48.8 -- not an asteroid (will add it to exclusion list)
07:05:30.66 +01:36:36.7 -- not an asteroid (will add it to exclusion list)
06:57:39.96 -05:17:24.3 -- not an asteroid (will add it to exclusion list)
06:49:41.95 -01:43:20.2 -- not an asteroid (will add it to exclusion list)
07:01:24.19 +01:06:08.5 -- not an asteroid (will add it to exclusion list)
07:06:24.24 +00:20:29.3 -- not an asteroid (will add it to exclusion list)
07:12:29.92 +00:35:37.6 -- not an asteroid (will add it to exclusion list)
07:18:58.87 -05:26:28.5 -- not an asteroid (will add it to exclusion list)
06:52:07.82 +00:28:19.6 -- not an asteroid (will add it to exclusion list)
07:01:07.65 -03:14:32.1 -- not an asteroid (will add it to exclusion list)
06:56:36.50 +01:00:09.7 -- not an asteroid (will add it to exclusion list)
07:13:48.27 -00:49:58.9 -- not an asteroid (will add it to exclusion list)
07:00:56.86 -03:16:17.9 -- not an asteroid (will add it to exclusion list)
06:54:57.35 -01:11:47.8 -- not an asteroid (will add it to exclusion list)
07:05:49.23 +01:38:16.7 -- not an asteroid (will add it to exclusion list)
07:07:11.50 -02:58:19.4 -- not an asteroid (will add it to exclusion list)
06:52:46.18 -01:34:15.9 -- not an asteroid (will add it to exclusion list)
06:58:26.75 -00:54:23.5 -- not an asteroid (will add it to exclusion list)
07:08:12.55 -03:12:26.0 -- not an asteroid (will add it to exclusion list)
06:53:58.11 -04:52:50.6 -- not an asteroid (will add it to exclusion list)
07:01:38.39 -04:40:49.5 -- not an asteroid (will add it to exclusion list)
06:49:33.19 -01:23:29.2 -- not an asteroid (will add it to exclusion list)
06:52:53.69 +01:22:23.8 -- not an asteroid (will add it to exclusion list)
07:01:10.32 +00:00:20.0 -- not an asteroid (will add it to exclusion list)
06:57:00.78 +00:17:37.8 -- not an asteroid (will add it to exclusion list)
07:07:58.75 -00:56:39.1 -- not an asteroid (will add it to exclusion list)
07:01:46.16 +01:19:50.2 -- not an asteroid (will add it to exclusion list)
06:47:11.21 -02:50:54.0 -- not an asteroid (will add it to exclusion list)
07:08:02.93 -03:37:52.5 -- not an asteroid (will add it to exclusion list)
06:51:43.84 -00:26:00.1 -- not an asteroid (will add it to exclusion list)
06:59:40.54 -00:39:47.2 -- not an asteroid (will add it to exclusion list)
07:07:25.54 +01:35:35.0 -- not an asteroid (will add it to exclusion list)
07:02:02.01 +00:07:45.7 -- not an asteroid (will add it to exclusion list)
06:54:48.35 +00:23:18.3 -- not an asteroid (will add it to exclusion list)
07:01:07.55 -01:29:23.1 -- not an asteroid (will add it to exclusion list)
06:51:24.84 -03:32:35.6 -- not an asteroid (will add it to exclusion list)
06:48:35.72 -00:00:04.6 -- not an asteroid (will add it to exclusion list)
06:55:36.32 -01:20:46.1 -- not an asteroid (will add it to exclusion list)
06:58:22.85 -04:38:15.2 -- not an asteroid (will add it to exclusion list)
07:02:49.62 -03:11:40.1 -- not an asteroid (will add it to exclusion list)
06:58:24.63 -03:02:35.3 -- not an asteroid (will add it to exclusion list)
06:51:17.46 -02:53:48.6 -- not an asteroid (will add it to exclusion list)
07:00:55.05 -03:04:10.5 -- not an asteroid (will add it to exclusion list)
06:48:53.21 +01:49:29.8 -- asteroid (will NOT add it to exclusion list)
06:49:37.18 -02:17:20.0 -- not an asteroid (will add it to exclusion list)
06:51:34.31 -01:39:23.8 -- not an asteroid (will add it to exclusion list)
06:54:26.43 +00:45:45.7 -- not an asteroid (will add it to exclusion list)
07:12:49.76 -03:03:25.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:46:14.65 +01:13:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:11.21 -02:50:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:35.72 -00:00:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:33.19 -01:23:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:37.18 -02:17:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:41.95 -01:43:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:50.92 -02:36:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:59.48 -02:47:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:17.46 -02:53:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:24.84 -03:32:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:34.31 -01:39:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:34.73 -01:53:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:43.84 -00:26:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:46.27 -05:25:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:07.82 +00:28:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:12.49 -00:22:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:35.30 -02:12:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:46.18 -01:34:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:53.69 +01:22:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:07.46 -01:35:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:36.50 -04:59:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:42.63 -01:01:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:58.11 -04:52:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:26.43 +00:45:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:48.35 +00:23:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:57.35 -01:11:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:03.32 +01:02:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:22.99 -02:18:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:36.32 -01:20:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:36.50 +01:00:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:38.29 -04:36:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:00.78 +00:17:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:30.10 -00:57:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:31.65 -00:23:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:33.46 -03:31:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:39.96 -05:17:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:21.76 -00:45:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:22.85 -04:38:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:24.63 -03:02:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:26.75 -00:54:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:25.68 -01:04:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:30.61 -04:05:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:39.73 -00:40:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:40.54 -00:39:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:54.60 -02:15:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:08.49 -00:53:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:55.05 -03:04:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:56.86 -03:16:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:01.01 -00:25:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:07.55 -01:29:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:07.65 -03:14:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:10.32 +00:00:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:21.74 +02:15:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:22.61 -00:16:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:24.19 +01:06:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:38.39 -04:40:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:46.16 +01:19:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:02.01 +00:07:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:13.77 -00:39:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:32.62 -02:31:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:35.25 -03:37:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:49.62 -03:11:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:50.56 -03:19:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:02.21 +01:23:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:14.46 +01:07:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:36.84 -01:50:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:40.27 -01:07:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:51.10 -03:43:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:20.85 -04:41:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:00.18 +01:38:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:08.38 -04:26:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:10.46 -00:00:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:15.37 +00:02:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:23.54 -01:12:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:25.02 -00:59:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:30.66 +01:36:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:49.23 +01:38:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:04.88 -02:19:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:24.24 +00:20:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:41.15 -02:24:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:11.50 -02:58:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:25.54 +01:35:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:58.75 -00:56:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:02.93 -03:37:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:12.55 -03:12:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:16.27 -02:14:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:29.18 -00:58:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:41.85 +01:18:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.96 -03:56:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:48.29 +00:19:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:03.94 -01:19:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:05.01 -02:57:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:19.83 +00:54:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:00.63 -02:53:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:01.96 -01:11:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:09.81 +01:52:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:11.80 -01:59:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:26.24 +01:50:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:29.92 +00:35:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:49.76 -03:03:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:11.69 +01:02:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:43.93 -01:35:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:48.27 -00:49:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:59.84 -02:51:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:38.83 -03:56:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:10.56 -04:30:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:49.72 -00:37:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:03.79 -01:38:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:04.59 +00:48:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:12.87 -04:06:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:13.30 -00:00:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:30.99 +01:05:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:51.22 -01:41:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:18.05 -00:24:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:58.87 -05:26:28.5 -- 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)
06:46:14.65 +01:13:09.0 -- not a known variable star
06:47:11.21 -02:50:54.0 -- not a known variable star
06:48:35.72 -00:00:04.6 -- not a known variable star
06:49:33.19 -01:23:29.2 -- not a known variable star
06:49:37.18 -02:17:20.0 -- not a known variable star
06:49:41.95 -01:43:20.2 -- not a known variable star
06:50:50.92 -02:36:24.6 -- not a known variable star
06:50:59.48 -02:47:54.1 -- not a known variable star
06:51:17.46 -02:53:48.6 -- not a known variable star
06:51:24.84 -03:32:35.6 -- a known variable star
06:51:34.31 -01:39:23.8 -- not a known variable star
06:51:34.73 -01:53:52.3 -- a known variable star
06:51:43.84 -00:26:00.1 -- not a known variable star
06:51:46.27 -05:25:55.8 -- a known variable star
06:52:07.82 +00:28:19.6 -- not a known variable star
06:52:12.49 -00:22:25.6 -- a known variable star
06:52:35.30 -02:12:18.2 -- not a known variable star
06:52:46.18 -01:34:15.9 -- not a known variable star
06:52:53.69 +01:22:23.8 -- not a known variable star
06:53:07.46 -01:35:07.5 -- not a known variable star
06:53:36.50 -04:59:47.9 -- a known variable star
06:53:42.63 -01:01:10.7 -- not a known variable star
06:53:58.11 -04:52:50.6 -- not a known variable star
06:54:26.43 +00:45:45.7 -- not a known variable star
06:54:48.35 +00:23:18.3 -- a known variable star
06:54:57.35 -01:11:47.8 -- not a known variable star
06:55:03.32 +01:02:05.0 -- not a known variable star
06:55:22.99 -02:18:59.2 -- a known variable star
06:55:36.32 -01:20:46.1 -- not a known variable star
06:56:36.50 +01:00:09.7 -- a known variable star
06:56:38.29 -04:36:28.6 -- not a known variable star
06:57:00.78 +00:17:37.8 -- not a known variable star
06:57:30.10 -00:57:11.9 -- a known variable star
06:57:31.65 -00:23:42.1 -- not a known variable star
06:57:33.46 -03:31:49.5 -- not a known variable star
06:57:39.96 -05:17:24.3 -- not a known variable star
06:58:21.76 -00:45:45.5 -- not a known variable star
06:58:22.85 -04:38:15.2 -- not a known variable star
06:58:24.63 -03:02:35.3 -- not a known variable star
06:58:26.75 -00:54:23.5 -- not a known variable star
06:59:25.68 -01:04:49.7 -- not a known variable star
06:59:30.61 -04:05:39.4 -- a known variable star
06:59:39.73 -00:40:07.6 -- not a known variable star
06:59:40.54 -00:39:47.2 -- not a known variable star
06:59:54.60 -02:15:14.1 -- not a known variable star
07:00:08.49 -00:53:10.0 -- not a known variable star
07:00:55.05 -03:04:10.5 -- not a known variable star
07:00:56.86 -03:16:17.9 -- not a known variable star
07:01:01.01 -00:25:44.6 -- not a known variable star
07:01:07.55 -01:29:23.1 -- not a known variable star
07:01:07.65 -03:14:32.1 -- a known variable star
07:01:10.32 +00:00:20.0 -- a known variable star
07:01:21.74 +02:15:49.7 -- a known variable star
07:01:22.61 -00:16:06.1 -- not a known variable star
07:01:24.19 +01:06:08.5 -- not a known variable star
07:01:38.39 -04:40:49.5 -- not a known variable star
07:01:46.16 +01:19:50.2 -- not a known variable star
07:02:02.01 +00:07:45.7 -- not a known variable star
07:02:13.77 -00:39:21.2 -- not a known variable star
07:02:32.62 -02:31:08.0 -- not a known variable star
07:02:35.25 -03:37:56.6 -- a known variable star
07:02:49.62 -03:11:40.1 -- a known variable star
07:02:50.56 -03:19:41.4 -- a known variable star
07:03:02.21 +01:23:57.0 -- not a known variable star
07:03:14.46 +01:07:06.4 -- not a known variable star
07:03:36.84 -01:50:14.9 -- not a known variable star
07:03:40.27 -01:07:51.0 -- not a known variable star
07:03:51.10 -03:43:31.4 -- a known variable star
07:04:20.85 -04:41:02.1 -- not a known variable star
07:05:00.18 +01:38:42.9 -- not a known variable star
07:05:08.38 -04:26:25.2 -- a known variable star
07:05:10.46 -00:00:18.8 -- a known variable star
07:05:15.37 +00:02:45.6 -- not a known variable star
07:05:23.54 -01:12:19.8 -- a known variable star
07:05:25.02 -00:59:48.8 -- a known variable star
07:05:30.66 +01:36:36.7 -- not a known variable star
07:05:49.23 +01:38:16.7 -- not a known variable star
07:06:04.88 -02:19:37.6 -- not a known variable star
07:06:24.24 +00:20:29.3 -- not a known variable star
07:06:41.15 -02:24:48.2 -- not a known variable star
07:07:11.50 -02:58:19.4 -- not a known variable star
07:07:25.54 +01:35:35.0 -- not a known variable star
07:07:58.75 -00:56:39.1 -- not a known variable star
07:08:02.93 -03:37:52.5 -- a known variable star
07:08:12.55 -03:12:26.0 -- not a known variable star
07:08:16.27 -02:14:30.6 -- not a known variable star
07:08:29.18 -00:58:27.6 -- a known variable star
07:08:41.85 +01:18:46.4 -- a known variable star
07:08:43.96 -03:56:11.0 -- not a known variable star
07:08:48.29 +00:19:42.4 -- not a known variable star
07:09:03.94 -01:19:31.7 -- not a known variable star
07:09:05.01 -02:57:19.9 -- a known variable star
07:09:19.83 +00:54:53.6 -- a known variable star
07:11:00.63 -02:53:39.2 -- not a known variable star
07:12:01.96 -01:11:16.0 -- a known variable star
07:12:09.81 +01:52:14.8 -- not a known variable star
07:12:11.80 -01:59:47.9 -- not a known variable star
07:12:26.24 +01:50:34.4 -- not a known variable star
07:12:29.92 +00:35:37.6 -- not a known variable star
07:12:49.76 -03:03:25.8 -- a known variable star
07:13:11.69 +01:02:13.4 -- not a known variable star
07:13:43.93 -01:35:26.7 -- not a known variable star
07:13:48.27 -00:49:58.9 -- not a known variable star
07:13:59.84 -02:51:47.8 -- not a known variable star
07:14:38.83 -03:56:25.0 -- not a known variable star
07:15:10.56 -04:30:19.1 -- a known variable star
07:15:49.72 -00:37:02.7 -- a known variable star
07:16:03.79 -01:38:30.1 -- not a known variable star
07:16:04.59 +00:48:08.0 -- not a known variable star
07:16:12.87 -04:06:21.0 -- not a known variable star
07:16:13.30 -00:00:45.6 -- not a known variable star
07:17:30.99 +01:05:37.9 -- a known variable star
07:17:51.22 -01:41:37.7 -- a known variable star
07:18:18.05 -00:24:27.9 -- not a known variable star
07:18:58.87 -05:26:28.5 -- not a known variable star
Found 83 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
115 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 115 (excluding asteroids and hot pixels, 83 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461159.61239023 -observatory V36
01:25:01.51 +06:39:08.4 Mercury (-0.6mag)
04:14:16.80 +22:02:33.4 Venus (-3.9mag)
00:54:59.91 +04:54:24.0 Mars (1.2mag)
07:19:27.19 +22:34:23.6 Jupiter (-2.0mag)
00:34:52.79 +01:24:07.1 Saturn (0.9mag)
03:50:35.48 +19:56:37.9 Uranus (5.8mag)
00:12:28.85 -00:05:06.8 Neptune (7.8mag)
20:34:09.55 -22:53:49.7 Pluto (14.5mag)
12:30:05.47 -06:33:01.4 Moon (-12.0mag)
-rw-r--r-- 1 apache apache 363 Apr 28 21:44 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461159.61239023:
07:19:33.27 +22:34:08.3 Io (5.8mag)
07:19:15.93 +22:34:49.1 Europa (6.0mag)
07:19:43.23 +22:33:51.3 Ganymede (5.4mag)
07:19:32.71 +22:34:20.2 Callisto (6.7mag)
07:22:08.37 +22:16:38.4 Himalia (15.4mag)
07:19:24.47 +22:34:31.4 Thebe (16.3mag)
07:22:33.00 +22:46:20.8 Elara (17.4mag)
07:19:13.11 +23:07:32.0 Pasiphae (17.5mag)
07:27:27.41 +22:33:31.0 Carme (18.6mag)
00:35:03.61 +01:24:15.9 Titan (8.8mag)
00:34:49.28 +01:24:17.0 Rhea (10.1mag)
00:34:23.39 +01:22:25.3 Iapetus (11.5mag)
00:34:59.62 +01:23:47.7 Hyperion (14.8mag)
00:36:18.43 +01:31:25.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 28 21:45 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461159.61239023:
16:26:36.50 -24:01:14.0 JWST
01:37:55.09 -53:43:42.9 Chandra
17:11:27.05 -49:01:19.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 28 21:44 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461159.61239023 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
06:14:36.53 +30:12:36.5 17.9mag P/2009 WX51 (Catalina)
18:55:31.91 -29:36:48.9 13.8mag P/2010 H2 (Vales)
05:16:49.63 -69:05:29.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:35:42.05 +31:32:15.0 17.3mag C/2017 K2 (PANSTARRS)
17:28:18.79 +12:02:34.3 17.7mag C/2021 G2 (ATLAS)
23:13:05.71 +29:47:23.9 17.1mag C/2022 E2 (ATLAS)
04:44:48.66 +26:22:13.7 16.1mag C/2022 N2 (PANSTARRS)
09:07:17.70 +31:59:59.5 16.3mag C/2022 QE78 (ATLAS)
08:33:53.64 +01:08:29.8 17.4mag C/2022 R6 (PANSTARRS)
18:49:41.73 +19:34:48.0 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:35:53.07 -11:19:46.9 17.5mag P/2023 B1 (PANSTARRS)
09:02:50.40 -09:54:27.7 17.8mag C/2023 F3 (ATLAS)
22:05:29.36 +63:44:20.1 17.6mag C/2023 H5 (Lemmon)
19:05:02.39 -04:02:59.3 14.0mag C/2023 R1 (PANSTARRS)
20:19:34.03 +87:42:22.2 17.8mag C/2023 X2 (Lemmon)
06:26:07.05 +63:31:06.4 17.3mag C/2024 A1 (ATLAS)
05:39:39.76 +21:56:20.0 11.8mag C/2024 E1 (Wierzchos)
16:10:00.87 +08:29:34.0 17.3mag C/2024 G6 (ATLAS)
20:23:18.10 +18:58:13.2 14.4mag C/2024 J3 (ATLAS)
03:38:29.56 -20:29:17.5 16.3mag C/2024 T5 (ATLAS)
05:28:17.99 +42:13:52.5 17.8mag C/2025 J1 (Borisov)
12:47:56.50 +51:14:00.8 15.8mag C/2025 L1 (ATLAS)
03:47:14.17 -28:25:29.5 17.9mag C/2025 Q3 (ATLAS)
03:20:24.49 +03:17:32.4 8.1mag C/2025 R3 (PANSTARRS)
12:48:42.43 +03:44:06.5 17.3mag C/2025 Y1 (ATLAS)
04:44:18.67 +01:47:45.2 16.1mag C/2026 A1 (MAPS)
00:34:49.60 +39:20:21.3 15.0mag C/2026 B2 (Sun-Gao)
19:08:19.00 -09:00:22.8 11.1mag 10P/Tempel
14:42:44.65 +01:36:34.3 15.2mag 24P/Schaumasse
11:00:06.01 -01:09:47.6 15.8mag 29P/Schwassmann-Wachmann
10:38:52.44 -03:13:56.3 17.2mag 43P/Wolf-Harrington
02:09:04.30 +19:40:21.5 17.3mag 47P/Ashbrook-Jackson
07:36:03.67 +34:05:46.7 17.0mag 63P/Wild
23:45:13.98 -09:56:31.1 15.7mag 65P/Gunn
04:39:35.66 +25:25:23.0 16.0mag 76P/West-Kohoutek-Ikemura
01:34:58.15 +10:44:54.2 14.2mag 78P/Gehrels
23:41:09.86 -05:31:57.9 14.8mag 88P/Howell
02:48:35.03 +23:55:17.5 15.0mag 93P/Lovas
05:20:41.77 +32:53:16.8 16.1mag 123P/West-Hartley
08:45:34.94 +32:20:54.6 16.3mag 124P/Mrkos
02:53:46.90 +15:46:49.9 16.4mag 128P/Shoemaker-Holt
03:13:26.87 +15:59:17.2 17.6mag 131P/Mueller
02:36:42.27 +17:03:08.7 10.6mag 141P/Machholz
02:43:18.81 +09:36:12.2 10.6mag 141P-A/Machholz
01:24:02.61 +05:20:53.1 11.4mag 141P-D/Machholz
01:39:21.82 +05:06:00.7 14.9mag 162P/SidingSpring
22:13:44.67 -08:22:31.4 17.9mag 218P/LINEAR
17:16:49.38 -12:19:17.5 16.1mag 235P/LINEAR
06:03:24.51 +35:28:58.7 17.0mag 240P/NEAT
07:45:55.98 -03:52:45.4 17.8mag 242P/Spahr
22:49:46.48 -17:12:57.1 17.5mag 260P/McNaught
02:25:56.29 +23:42:38.9 17.9mag 295P/LINEAR
15:36:39.53 +07:44:43.9 17.4mag 391P/Kowalski
07:40:10.25 +21:21:22.1 17.7mag 450P/LONEOS
05:55:36.95 +44:15:55.8 17.6mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 28 21:44 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
16:34:34.94 -54:34:58.20 2026-04-25.14 15.99
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
16:34:34.94 -54:34:58.20 2026-04-25.14 15.99
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 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -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
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -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
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
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
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
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
-rw-r--r-- 1 apache apache 5.8K Apr 28 21:44 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
-rw-r--r-- 1 apache apache 188K Apr 28 21:44 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:56:52.527 +38:43:02.06 AT 2026khl 2026-04-20.25 19.73
16:16:44.333 +52:18:26.69 AT 2026khk 2026-04-19.51 20.2
14:44:33.224 +13:28:05.23 AT 2026khj 2026-04-21.41 19.73
16:09:12.398 +04:55:54.03 AT 2026khi 2026-04-20.52 20.97
19:02:47.110 +47:03:07.12 AT 2026khh 2026-04-14.23 19.64
20:50:35.204 +13:38:49.37 AT 2026khg 2026-04-14.22 19.81
20:26:18.237 -36:23:03.88 AT 2026khf 2026-04-14.80 19.84
11:31:56.240 +09:46:11.18 AT 2026khe 2026-04-11.98 19.99
17:14:06.281 -09:07:50.24 AT 2026khd 2026-03-24.78 20.41
11:51:39.769 -32:37:47.81 AT 2026khc 2026-04-12.44 20.23
11:31:53.568 -43:58:12.63 AT 2026khb 2026-04-12.44 20.17
12:49:47.564 +53:21:17.16 AT 2026kha 2026-04-13.100 19.83
15:43:26.957 +41:52:55.68 AT 2026kgz 2026-04-12.12 19.96
14:26:51.866 +60:24:31.86 AT 2026kgy 2026-04-21.11 19.1
04:18:17.932 -46:11:54.70 AT 2026kgx 2026-01-04.13 23.26
17:39:40.560 +14:49:02.18 AT 2026kgw 2026-04-21.45 19.4006
13:34:06.597 +11:18:46.85 AT 2026kgv 2026-04-17.31 20.5502
04:07:49.305 -49:16:52.86 AT 2026kgu 2026-01-11.08 23.7
04:06:28.945 -47:25:15.01 AT 2026kgt 2026-02-17.10 22.87
09:51:04.284 +41:30:11.28 AT 2026kgs 2026-04-14.88 19.38
-rw-r--r-- 1 apache apache 29K Apr 28 21:44 tns_transients_list.txt
