This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.32 06:51:13.30 -01:21:59.2
214.12344 -0.67114 galactic Mon Second-epoch detections are separated by 1.7" and 6.4 pix
The object was found in VSX 3" Gaia DR3 3106340083295507200
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.360 G 14.380 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 06:51:13.30 -01:21:59.2: 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 06:51:13.30 -01:21:59.2: 13.99 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.99 +/- 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 3106340083295507200,2461155.6093,13.32,0.05,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 3106340083295507200 20260425.1093 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.63 06:50:58.14 -02:14:41.0
214.87652 -1.12762 galactic Mon Second-epoch detections are separated by 0.2" and 6.2 pix
The object was found in VSX18" Gaia DR3 3106220580127465344
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.270 G 15.300 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 06:50:58.14 -02:14:41.0: 14.08 +/- 0.16 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:50:58.14 -02:14:41.0: 15.40 +/- 0.32 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106220580127465344,2461155.6093,13.63,0.05,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
Gaia DR3 3106220580127465344 20260425.1093 13.63CV 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 25.1093 2461155.6093 13.41 06:52:23.48 -02:34:55.9
215.33889 -0.96517 galactic Mon Second-epoch detections are separated by 2.9" and 5.8 pix
The object was found in VSX20" Gaia DR3 3106008305662642304
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.300 G 14.330 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 06:52:23.48 -02:34:55.9: 14.48 +/- 0.25 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:23.48 -02:34:55.9: 14.35 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106008305662642304,2461155.6093,13.41,0.05,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
Gaia DR3 3106008305662642304 20260425.1093 13.41CV 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 25.1093 2461155.6093 13.26 06:53:25.72 -04:34:19.7
217.22875 -1.64131 galactic Mon Second-epoch detections are separated by 2.2" 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 | target | 06:53:25.72 -04:34:19.7 (user input) | T | P | (position from user input) SpType: G7III 2012A&A...543A.125G CoRoT 110858597
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:25.72 -04:34:19.7: 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 06:53:25.72 -04:34:19.7: 15.53 +/- 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,2461155.6093,13.26,0.05,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
target 20260425.1093 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.38 06:53:30.53 -03:06:06.5
215.92865 -0.95364 galactic Mon Second-epoch detections are separated by 1.5" and 6.4 pix
The object was found in VSX19" Gaia DR3 3102837412905531904
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.910 G 13.930 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 06:53:30.53 -03:06:06.5: 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 06:53:30.53 -03:06:06.5: 15.01 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102837412905531904,2461155.6093,13.38,0.05,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 3102837412905531904 20260425.1093 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.24 06:50:18.43 -04:39:46.6
216.95559 -2.37532 galactic Mon Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.5784-04.6648 | 06:50:18.43 -04:39:46.6 (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 06:50:18.43 -04:39:46.6: 14.90 +/- 0.35 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:50:18.43 -04:39:46.6: 15.67 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.90 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.5784-04.6648,2461155.6093,13.24,0.05,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 J102.5784-04.6648 20260425.1093 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.20 06:49:36.09 -00:19:57.1
213.01853 -0.56022 galactic Mon Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113241198088231808 | 06:49:35.23 -00:19:44.7 (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 06:49:36.09 -00:19:57.1: 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 06:49:36.09 -00:19:57.1: 13.99 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.99 +/- 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 3113241198088231808,2461155.6093,13.20,0.05,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 3113241198088231808 20260425.1093 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.25 06:50:57.40 -01:59:58.4
214.65684 -1.01865 galactic Mon Second-epoch detections are separated by 1.8" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.7395-02.0003 | 06:50:57.40 -01:59:58.4 (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 06:50:57.40 -01:59:58.4: 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 06:50:57.40 -01:59:58.4: 14.61 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.61 +/- 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 J102.7395-02.0003,2461155.6093,13.25,0.05,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
ATO J102.7395-02.0003 20260425.1093 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.24 07:00:40.18 -02:26:31.6
216.15799 0.93843 galactic Mon Second-epoch detections are separated by 0.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.1671-02.4433 | 07:00:39.81 -02:26:12.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.667+/-0.067 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:00:40.18 -02:26:31.6: 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 07:00:40.18 -02:26:31.6: 15.05 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1671-02.4433,2461155.6093,13.24,0.05,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 J105.1671-02.4433 20260425.1093 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.10 06:54:46.06 -00:27:03.5
213.71288 0.53518 galactic Mon Second-epoch detections are separated by 2.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:54:46.06 -00:27:03.5 (user input) | T | P | (position from user input) J-Ks=0.297+/-0.044 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:46.06 -00:27:03.5: 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 06:54:46.06 -00:27:03.5: 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,2461155.6093,13.10,0.05,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 20260425.1093 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.15 06:59:01.82 -03:10:13.1
216.61861 0.24152 galactic Mon Second-epoch detections are separated by 0.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:59:01.82 -03:10:13.1 (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 06:59:01.82 -03:10:13.1: 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 06:59:01.82 -03:10:13.1: 13.96 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461155.6093,13.15,0.05,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
target 20260425.1093 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.25 06:52:03.56 -00:56:53.2
213.84657 -0.29406 galactic Mon Second-epoch detections are separated by 1.5" and 6.1 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 3112373928231097472 | 06:52:01.88 -00:56:23.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:52:03.56 -00:56:53.2: 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 06:52:03.56 -00:56:53.2: 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 3112373928231097472,2461155.6093,13.25,0.05,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
Gaia DR3 3112373928231097472 20260425.1093 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.12 07:07:54.99 -05:37:21.2
219.81351 1.08604 galactic Mon Second-epoch detections are separated by 2.3" and 6.1 pix
The object was found in VSX19" Gaia DR3 3053315104258422528
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.960 G 12.980 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 07:07:54.99 -05:37:21.2: 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 07:07:54.99 -05:37:21.2: 14.47 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.47 +/- 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 3053315104258422528,2461155.6093,13.12,0.05,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 3053315104258422528 20260425.1093 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.26 06:53:29.91 -01:56:22.6
214.89302 -0.42606 galactic Mon Second-epoch detections are separated by 1.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.3827-01.9302 | 06:53:29.91 -01:56:22.6 (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 06:53:29.91 -01:56:22.6: 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 06:53:29.91 -01:56:22.6: 14.34 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.34 +/- 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
ATO J103.3827-01.9302,2461155.6093,13.26,0.05,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
ATO J103.3827-01.9302 20260425.1093 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.17 07:06:01.56 -02:28:21.7
216.79778 2.11391 galactic Mon Second-epoch detections are separated by 2.2" 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 | target | 07:06:01.56 -02:28:21.7 (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 07:06:01.56 -02:28:21.7: 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 07:06:01.56 -02:28:21.7: 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
target,2461155.6093,13.17,0.05,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 20260425.1093 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.01 06:59:56.95 +01:13:10.5
212.81628 2.44968 galactic Mon Second-epoch detections are separated by 1.3" and 6.2 pix
The object was found in VSX16" Gaia DR3 3113873520353715712
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.530 G 15.560 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 06:59:56.95 +01:13:10.5: 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 06:59:56.95 +01:13:10.5: 15.04 +/- 0.26 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.26
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113873520353715712,2461155.6093,13.01,0.05,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 3113873520353715712 20260425.1093 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.04 07:19:13.98 -05:31:01.9
221.02376 3.63116 galactic Mon Second-epoch detections are separated by 2.9" and 6.6 pix
The object was found in VSX17" Gaia DR3 3058395913128645888
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.180 G 14.210 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 07:19:13.98 -05:31:01.9: 14.41 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:19:13.98 -05:31:01.9: 15.16 +/- 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 3058395913128645888,2461155.6093,13.04,0.05,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
Gaia DR3 3058395913128645888 20260425.1093 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.02 06:57:16.36 -02:12:54.6
215.56843 0.28728 galactic Mon Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.3224-02.2166 | 06:57:16.36 -02:12:54.6 (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 06:57:16.36 -02:12:54.6: 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 06:57:16.36 -02:12:54.6: 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
ATO J104.3224-02.2166,2461155.6093,13.02,0.05,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 J104.3224-02.2166 20260425.1093 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.07 07:00:14.73 -00:57:25.5
214.78829 1.52269 galactic Mon Second-epoch detections are separated by 1.5" and 6.1 pix
The object was found in VSX 4" Gaia DR3 3112197834571834752
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.480 G 14.500 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 07:00:14.73 -00:57:25.5: 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 07:00:14.73 -00:57:25.5: 15.58 +/- 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 3112197834571834752,2461155.6093,13.07,0.05,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
Gaia DR3 3112197834571834752 20260425.1093 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.98 07:02:32.32 -00:13:10.6
214.39371 2.36943 galactic Mon Second-epoch detections are separated by 0.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112672888012933248 | 07:02:32.73 -00:12:50.0 (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 07:02:32.32 -00:13:10.6: 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 07:02:32.32 -00:13:10.6: 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
Gaia DR3 3112672888012933248,2461155.6093,12.98,0.05,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 3112672888012933248 20260425.1093 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.89 07:06:24.61 -00:09:13.5
214.77762 3.26055 galactic Mon Second-epoch detections are separated by 2.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:06:24.61 -00:09:13.5 (user input) | T | P | (position from user input) J-Ks=0.204+/-0.041 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:06:24.61 -00:09:13.5: 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 07:06:24.61 -00:09:13.5: 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
target,2461155.6093,12.89,0.05,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 20260425.1093 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.07 06:50:56.01 -02:40:07.2
215.24996 -1.32866 galactic Mon Second-epoch detections are separated by 1.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.7265-02.6639 | 06:50:56.01 -02:40:07.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.305+/-0.043 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:50:56.01 -02:40:07.2: 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 06:50:56.01 -02:40:07.2: 13.78 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.78 +/- 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 J102.7265-02.6639,2461155.6093,13.07,0.05,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 J102.7265-02.6639 20260425.1093 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.13 06:53:34.00 -00:32:05.2
213.65054 0.22977 galactic Mon Second-epoch detections are separated by 1.3" 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 3113254808845036928 | 06:53:31.24 -00:31:46.7 (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 06:53:34.00 -00:32:05.2: 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 06:53:34.00 -00:32:05.2: 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 3113254808845036928,2461155.6093,13.13,0.05,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
Gaia DR3 3113254808845036928 20260425.1093 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.04 07:01:52.57 -01:40:51.6
215.61874 1.55447 galactic Mon Second-epoch detections are separated by 2.8" 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 J105.4717-01.6880 | 07:01:52.57 -01:40:51.6 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.349+/-0.034 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:52.57 -01:40:51.6: 14.48 +/- 0.26 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:52.57 -01:40:51.6: 14.87 +/- 0.20 detection
Forced photometry reference-image weighted average: 14.72 +/- 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 J105.4717-01.6880,2461155.6093,13.04,0.05,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 J105.4717-01.6880 20260425.1093 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.15 06:53:52.20 -02:12:22.9
215.17275 -0.46510 galactic Mon Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3106045203719510272 | 06:53:52.99 -02:12:05.9 (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 06:53:52.20 -02:12:22.9: 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 06:53:52.20 -02:12:22.9: 15.47 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.47 +/- 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 3106045203719510272,2461155.6093,13.15,0.05,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
Gaia DR3 3106045203719510272 20260425.1093 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.00 07:17:56.41 -02:49:58.3
218.48935 4.59004 galactic Mon Second-epoch detections are separated by 1.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J109.4891-02.8399 | 07:17:56.41 -02:49:58.3 (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 07:17:56.41 -02:49:58.3: 14.43 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:17:56.41 -02:49:58.3: 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 J109.4891-02.8399,2461155.6093,13.00,0.05,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 J109.4891-02.8399 20260425.1093 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.07 06:46:36.45 -03:38:14.6
215.62152 -2.73102 galactic Mon Second-epoch detections are separated by 2.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:46:36.45 -03:38:14.6 (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 06:46:36.45 -03:38:14.6: 13.92 +/- 0.16 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:46:36.45 -03:38:14.6: 14.60 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461155.6093,13.07,0.05,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
target 20260425.1093 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.91 06:59:32.97 -01:48:18.9
215.46353 0.98055 galactic Mon Second-epoch detections are separated by 5.1" and 6.4 pix
The object was found in VSX 9" GDS_J0659327-014810
Type: VAR
# Max. Min./Amp. JD0 Period
13.520 r Y 0.340 r
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 06:59:32.97 -01:48:18.9: 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 06:59:32.97 -01:48:18.9: 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
GDS_J0659327-014810,2461155.6093,12.91,0.05,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
GDS_J0659327-014810 20260425.1093 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.07 06:43:45.56 +00:35:14.9
211.53338 -1.44033 galactic Mon Second-epoch detections are separated by 5.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3125582872512184960 | 06:43:43.59 +00:34:43.5 (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 06:43:45.56 +00:35:14.9: 14.36 +/- 0.27 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:45.56 +00:35:14.9: 13.78 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.81 +/- 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 3125582872512184960,2461155.6093,13.07,0.05,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
Gaia DR3 3125582872512184960 20260425.1093 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.95 06:44:01.87 -04:32:27.5
216.13595 -3.71356 galactic Mon Second-epoch detections are separated by 1.8" and 6.2 pix
The object was found in VSX 1" Gaia DR3 3105251017027824384
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.060 G 14.090 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 06:44:01.87 -04:32:27.5: 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 06:44:01.87 -04:32:27.5: 15.33 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105251017027824384,2461155.6093,12.95,0.05,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 3105251017027824384 20260425.1093 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.81 07:16:07.40 +01:27:14.8
214.45456 6.15486 galactic CMi Second-epoch detections are separated by 7.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:16:07.40 +01:27:14.8 (user input) | T | P | (position from user input) J-Ks=0.075+/-0.060 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:16:07.40 +01:27:14.8: 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 07:16:07.40 +01:27:14.8: 14.69 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.69 +/- 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
target,2461155.6093,12.81,0.05,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
target 20260425.1093 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 25.1093 2461155.6093 12.93 06:57:49.50 -00:05:50.6
213.74686 1.37664 galactic Mon Second-epoch detections are separated by 1.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.4637-00.0973 | 06:57:49.06 -00:06:14.0 (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 06:57:49.50 -00:05:50.6: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:49.50 -00:05:50.6: 15.65 +/- 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 J104.4637-00.0973,2461155.6093,12.93,0.05,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 J104.4637-00.0973 20260425.1093 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.01 07:02:32.22 +00:30:19.8
213.74767 2.69995 galactic Mon Second-epoch detections are separated by 1.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:02:32.22 +00:30:19.8 (user input) | T | P | (position from user input) J-Ks=0.766+/-0.040 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:32.22 +00:30:19.8: 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 07:02:32.22 +00:30:19.8: 15.59 +/- 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,2461155.6093,13.01,0.05,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
target 20260425.1093 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.96 07:03:25.24 -00:05:26.4
214.37964 2.62448 galactic Mon Second-epoch detections are separated by 1.3" and 6.5 pix
The object was found in VSX 3" Gaia DR3 3112768614245470720
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.930 G 13.950 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 07:03:25.24 -00:05:26.4: 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 07:03:25.24 -00:05:26.4: 14.30 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112768614245470720,2461155.6093,12.96,0.05,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
Gaia DR3 3112768614245470720 20260425.1093 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.78 07:05:55.55 -03:57:45.4
218.11091 1.40836 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 | target | 07:05:55.55 -03:57:45.4 (user input) | T | P | (position from user input) J-Ks=0.218+/-0.040 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:55.55 -03:57:45.4: 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 07:05:55.55 -03:57:45.4: 15.37 +/- 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,2461155.6093,12.78,0.05,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 20260425.1093 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.62 07:12:16.06 -03:44:42.7
218.64573 2.91302 galactic Mon Second-epoch detections are separated by 0.2" 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 | ATO J108.0570-03.7413 | 07:12:16.06 -03:44:42.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.275+/-0.041 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:16.06 -03:44:42.7: 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 07:12:16.06 -03:44:42.7: 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
ATO J108.0570-03.7413,2461155.6093,12.62,0.05,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
ATO J108.0570-03.7413 20260425.1093 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 25.1093 2461155.6093 12.79 06:55:03.17 -01:02:50.6
214.27617 0.32657 galactic Mon Second-epoch detections are separated by 2.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:55:03.17 -01:02:50.6 (user input) | T | P | (position from user input) J-Ks=0.604+/-0.095 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:55:03.17 -01:02:50.6: 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 06:55:03.17 -01:02:50.6: 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,2461155.6093,12.79,0.05,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 20260425.1093 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.79 07:04:57.17 -01:40:50.3
215.97028 2.23833 galactic Mon Second-epoch detections are separated by 1.6" and 6.4 pix
The object was found in VSX 4" Gaia DR3 3109456545925792640
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.910 G 13.940 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 07:04:57.17 -01:40:50.3: 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 07:04:57.17 -01:40:50.3: 15.59 +/- 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 3109456545925792640,2461155.6093,12.79,0.05,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 3109456545925792640 20260425.1093 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.61 07:07:02.21 -01:54:20.2
216.40914 2.59824 galactic Mon Second-epoch detections are separated by 1.1" and 6.1 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 J106.7592-01.9064 | 07:07:02.21 -01:54:20.2 (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 07:07:02.21 -01:54:20.2: 14.54 +/- 0.28 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:02.21 -01:54:20.2: 15.44 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.54 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.7592-01.9064,2461155.6093,12.61,0.05,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
ATO J106.7592-01.9064 20260425.1093 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.67 07:13:23.19 +01:43:05.5
213.90488 5.66642 galactic CMi Second-epoch detections are separated by 5.5" and 6.9 pix
The object was found in VSX 6" Gaia DR3 3114835867904255872
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.730 G 13.760 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 07:13:23.19 +01:43:05.5: 13.60 +/- 0.13 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:13:23.19 +01:43:05.5: 15.22 +/- 0.31 detection
Forced photometry reference-image weighted average: 13.84 +/- 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 3114835867904255872,2461155.6093,12.67,0.05,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
Gaia DR3 3114835867904255872 20260425.1093 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.72 06:57:33.41 -03:31:48.4
216.77072 -0.24996 galactic Mon Second-epoch detections are separated by 1.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.3903-03.5266 | 06:57:33.41 -03:31:48.4 (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 06:57:33.41 -03:31:48.4: 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 06:57:33.41 -03:31:48.4: 15.08 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.3903-03.5266,2461155.6093,12.72,0.05,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 20260425.1093 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.66 07:14:02.03 -01:05:48.1
216.49248 4.52311 galactic Mon Second-epoch detections are separated by 2.4" 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 | target | 07:14:02.03 -01:05:48.1 (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 07:14:02.03 -01:05:48.1: 13.71 +/- 0.16 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:14:02.03 -01:05:48.1: 15.42 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.71 +/- 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
target,2461155.6093,12.66,0.05,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 20260425.1093 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.66 07:01:50.71 +01:44:17.8
212.57000 3.10775 galactic Mon Second-epoch detections are separated by 4.8" and 7.1 pix
The object was found in VSX24" Gaia DR3 3115399745572045696
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.490 G 13.520 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 07:01:50.71 +01:44:17.8: 14.16 +/- 0.21 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:50.71 +01:44:17.8: 15.48 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.16 +/- 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
Gaia DR3 3115399745572045696,2461155.6093,12.66,0.05,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 3115399745572045696 20260425.1093 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.72 06:55:47.99 +01:18:47.2
212.26018 1.56910 galactic Mon Second-epoch detections are separated by 1.5" and 6.2 pix
The object was found in VSX 4" Gaia DR3 3114103185143024128
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.820 G 13.840 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 06:55:47.99 +01:18:47.2: 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 06:55:47.99 +01:18:47.2: 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
Gaia DR3 3114103185143024128,2461155.6093,12.72,0.05,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 3114103185143024128 20260425.1093 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.72 06:51:34.68 -01:53:51.6
214.63690 -0.83403 galactic Mon Second-epoch detections are separated by 3.2" and 6.1 pix
The object was found in VSX 5" 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 06:51:34.68 -01:53:51.6: 13.35 +/- 0.09 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:34.68 -01:53:51.6: 14.25 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 3106258719436766848,2461155.6093,12.72,0.05,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 20260425.1093 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.73 06:51:17.40 -02:53:49.8
215.49399 -1.35349 galactic Mon Second-epoch detections are separated by 0.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 06:51:17.40 -02:53:49.8: 13.57 +/- 0.11 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:17.40 -02:53:49.8: 14.28 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.93 +/- 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 3105855610985039744,2461155.6093,12.73,0.05,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 3105855610985039744 20260425.1093 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 25.1093 2461155.6093 12.55 06:57:55.19 -04:37:48.5
217.79076 -0.67168 galactic Mon Second-epoch detections are separated by 1.5" and 6.5 pix
The object was found in VSX 3" Gaia DR3 3101673034391323264
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.730 G 13.750 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:55.19 -04:37:48.5: 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 06:57:55.19 -04:37:48.5: 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
Gaia DR3 3101673034391323264,2461155.6093,12.55,0.05,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
Gaia DR3 3101673034391323264 20260425.1093 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 25.1093 2461155.6093 12.54 07:19:03.35 -04:45:19.8
220.32730 3.94612 galactic Mon Second-epoch detections are separated by 7.6" and 5.9 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 3058882653180926848 | 07:19:03.35 -04:45:19.8 (user input) | DSCT/GDOR (local) | (local) | (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 07:19:03.35 -04:45:19.8: 12.95 +/- 0.09 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:19:03.35 -04:45:19.8: 14.24 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.27 +/- 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 3058882653180926848,2461155.6093,12.54,0.05,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 3058882653180926848 20260425.1093 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.68 06:53:42.56 -01:01:10.3
214.09820 0.04043 galactic Mon Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.4228-01.0262 | 06:53:42.56 -01:01:10.3 (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 06:53:42.56 -01:01:10.3: 13.69 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:42.56 -01:01:10.3: 13.98 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.86 +/- 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 J103.4228-01.0262,2461155.6093,12.68,0.05,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
ATO J103.4228-01.0262 20260425.1093 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 25.1093 2461155.6093 12.52 06:59:38.56 -06:13:04.0
219.39916 -1.01529 galactic Mon Second-epoch detections are separated by 2.0" 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 | target | 06:59:38.56 -06:13:04.0 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.035 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:38.56 -06:13:04.0: 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 06:59:38.56 -06:13:04.0: 15.33 +/- 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,2461155.6093,12.52,0.05,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
target 20260425.1093 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 25.1093 2461155.6093 12.63 07:04:17.38 +01:02:40.1
213.46735 3.33562 galactic Mon Second-epoch detections are separated by 2.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | NSV 17321 | 07:04:18.79 +01:02:36.8 (Gaia DR3) | VAR: (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 07:04:17.38 +01:02:40.1: 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 07:04:17.38 +01:02:40.1: 14.32 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.20 +/- 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
NSV 17321,2461155.6093,12.63,0.05,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
NSV 17321 20260425.1093 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.56 07:18:49.57 -01:01:56.9
216.98782 5.61655 galactic Mon Second-epoch detections are separated by 3.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:18:49.57 -01:01:56.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.541+/-0.029 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:18:49.57 -01:01:56.9: 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 07:18:49.57 -01:01:56.9: 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
target,2461155.6093,12.56,0.05,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 20260425.1093 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.55 07:09:59.74 +01:25:46.8
213.77517 4.78063 galactic CMi Second-epoch detections are separated by 2.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:09:59.74 +01:25:46.8 (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 07:09:59.74 +01:25:46.8: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:09:59.74 +01:25:46.8: 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
target,2461155.6093,12.55,0.05,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
target 20260425.1093 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 25.1093 2461155.6093 12.52 07:17:43.83 -04:05:30.0
219.58421 3.96132 galactic Mon Second-epoch detections are separated by 1.6" and 6.3 pix
The object was found in VSX 8" Gaia DR3 3059731991553637248
Type: E
# Max. Min./Amp. JD0 Period
17.340 G 17.510 G 27.793000000000
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 07:17:43.83 -04:05:30.0: 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 07:17:43.83 -04:05:30.0: 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 3059731991553637248,2461155.6093,12.52,0.05,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 3059731991553637248 20260425.1093 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 25.1093 2461155.6093 12.63 07:10:30.43 -02:58:56.4
217.76513 2.87414 galactic Mon Second-epoch detections are separated by 0.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.6363-02.9783 | 07:10:30.43 -02:58:56.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.265+/-0.035 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:10:30.43 -02:58:56.4: 14.51 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:10:30.43 -02:58:56.4: 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
ATO J107.6363-02.9783,2461155.6093,12.63,0.05,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 J107.6363-02.9783 20260425.1093 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.59 07:09:05.32 -01:22:05.7
216.16616 3.30022 galactic Mon Second-epoch detections are separated by 2.9" and 6.6 pix
The object was found in VSX 7" Gaia DR3 3109387001816320640
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.770 G 14.790 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 07:09:05.32 -01:22:05.7: 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 07:09:05.32 -01:22:05.7: 15.36 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.36 +/- 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 3109387001816320640,2461155.6093,12.59,0.05,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 3109387001816320640 20260425.1093 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.53 07:04:36.92 +00:42:05.6
213.81024 3.25173 galactic Mon Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.1537+00.6972 | 07:04:36.92 +00:42:05.6 (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 07:04:36.92 +00:42:05.6: 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 07:04:36.92 +00:42:05.6: 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 J106.1537+00.6972,2461155.6093,12.53,0.05,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 J106.1537+00.6972 20260425.1093 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 25.1093 2461155.6093 12.47 06:51:46.19 -05:25:56.1
217.80714 -2.40049 galactic Mon Second-epoch detections are separated by 1.6" and 6.1 pix
The object was found in VSX 1" 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 06:51:46.19 -05:25:56.1: 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 06:51:46.19 -05:25:56.1: 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 3101909360675940992,2461155.6093,12.47,0.05,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
Gaia DR3 3101909360675940992 20260425.1093 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 25.1093 2461155.6093 12.49 07:08:02.81 -03:23:35.8
217.84796 2.13985 galactic Mon Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.0115-03.3931 | 07:08:02.81 -03:23:35.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.670+/-0.033 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:02.81 -03:23:35.8: 13.45 +/- 0.13 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:02.81 -03:23:35.8: 15.42 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.45 +/- 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
ATO J107.0115-03.3931,2461155.6093,12.49,0.05,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 J107.0115-03.3931 20260425.1093 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 25.1093 2461155.6093 12.56 07:05:38.79 -00:02:18.3
214.58751 3.14340 galactic Mon Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.4031-00.0467 | 07:05:36.76 -00:02:48.4 (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 07:05:38.79 -00:02:18.3: 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 07:05:38.79 -00:02:18.3: 15.53 +/- 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 J106.4031-00.0467,2461155.6093,12.56,0.05,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 J106.4031-00.0467 20260425.1093 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.38 07:10:55.70 -00:46:12.4
215.84452 3.98300 galactic Mon Second-epoch detections are separated by 1.3" and 6.3 pix
The object was found in VSX 1" Gaia DR3 3109436308041776640
Type: E
# Max. Min./Amp. JD0 Period
13.700 G 13.780 G 1.446160000000 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 07:10:55.70 -00:46:12.4: 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 07:10:55.70 -00:46:12.4: 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
Gaia DR3 3109436308041776640,2461155.6093,12.38,0.05,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 3109436308041776640 20260425.1093 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 25.1093 2461155.6093 12.43 07:01:07.30 +00:37:52.7
213.47409 2.44243 galactic Mon Second-epoch detections are separated by 1.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113058374218275456 | 07:01:08.57 +00:37:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.143+/-0.032 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:07.30 +00:37:52.7: 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 07:01:07.30 +00:37:52.7: 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 3113058374218275456,2461155.6093,12.43,0.05,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 3113058374218275456 20260425.1093 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 25.1093 2461155.6093 12.56 07:02:34.25 -04:55:48.5
218.58741 0.22161 galactic Mon Second-epoch detections are separated by 2.7" and 5.9 pix
The object was found in VSX 3" Gaia DR3 3101426159675447424
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.750 G 13.770 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 07:02:34.25 -04:55:48.5: 14.59 +/- 0.31 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:34.25 -04:55:48.5: 15.48 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.59 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101426159675447424,2461155.6093,12.56,0.05,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 3101426159675447424 20260425.1093 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.47 07:02:01.73 +00:22:42.0
213.80296 2.52889 galactic Mon Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.5098+00.3896 | 07:02:01.73 +00:22:42.0 (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 07:02:01.73 +00:22:42.0: 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 07:02:01.73 +00:22:42.0: 15.49 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.49 +/- 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
ATO J105.5098+00.3896,2461155.6093,12.47,0.05,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
ATO J105.5098+00.3896 20260425.1093 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 25.1093 2461155.6093 12.49 07:14:41.20 -00:43:06.9
216.23053 4.84161 galactic Mon Second-epoch detections are separated by 3.8" 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 | ATO J108.6734-00.7153 | 07:14:41.28 -00:42:36.6 (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 07:14:41.20 -00:43:06.9: 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 07:14:41.20 -00:43:06.9: 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
ATO J108.6734-00.7153,2461155.6093,12.49,0.05,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 J108.6734-00.7153 20260425.1093 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 25.1093 2461155.6093 12.33 07:08:29.18 -00:58:27.7
215.74635 3.34681 galactic Mon Second-epoch detections are separated by 2.5" and 6.1 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 -00:58:27.7: 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 -00:58:27.7: 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 3109604288498805632,2461155.6093,12.33,0.05,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 20260425.1093 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.34 07:15:26.79 -03:19:53.3
218.64453 3.80762 galactic Mon Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3060038613557611904 | 07:15:27.18 -03:20:18.1 (Gaia DR3) | RS (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A 1949AnHar.112....1C HD 296685 J-Ks=0.237+/-0.037 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:15:26.79 -03:19:53.3: 13.85 +/- 0.19 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:15:26.79 -03:19:53.3: 15.29 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.85 +/- 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 3060038613557611904,2461155.6093,12.34,0.05,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 3060038613557611904 20260425.1093 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 25.1093 2461155.6093 12.42 06:52:53.59 +01:22:23.6
211.87552 0.94984 galactic Mon Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 06:52:53.59 +01:22:23.6: 14.29 +/- 0.23 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:53.59 +01:22:23.6: 13.51 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.56 +/- 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+01.3729,2461155.6093,12.42,0.05,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 20260425.1093 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.26 07:07:20.90 -03:23:28.5
217.76605 1.98593 galactic Mon Second-epoch detections are separated by 0.8" and 6.2 pix
The object was found in VSX 2" Gaia DR3 3107912900321471104
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.240 G 13.280 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 07:07:20.90 -03:23:28.5: 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 07:07:20.90 -03:23:28.5: 15.37 +/- 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 3107912900321471104,2461155.6093,12.26,0.05,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 3107912900321471104 20260425.1093 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.38 07:16:33.73 -05:05:45.9
220.34085 3.23788 galactic Mon Second-epoch detections are separated by 0.5" and 6.3 pix
The object was found in VSX 1" Gaia DR3 3059224670018297728
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.440 G 13.470 G 0.026660200000 F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:16:33.73 -05:05:45.9: 14.51 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:16:33.73 -05:05:45.9: 15.20 +/- 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 3059224670018297728,2461155.6093,12.38,0.05,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 3059224670018297728 20260425.1093 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 25.1093 2461155.6093 12.45 07:03:06.80 -04:06:44.4
217.92235 0.71641 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 | ATO J105.7704-04.1090 | 07:03:06.07 -04:06:33.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.282+/-0.040 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:06.80 -04:06:44.4: 14.47 +/- 0.27 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:06.80 -04:06:44.4: 15.47 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.47 +/- 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
ATO J105.7704-04.1090,2461155.6093,12.45,0.05,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
ATO J105.7704-04.1090 20260425.1093 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 25.1093 2461155.6093 12.35 07:03:22.27 -04:53:37.4
218.64637 0.41549 galactic Mon Second-epoch detections are separated by 1.7" and 6.1 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 3101509138446206464 | 07:03:22.42 -04:53:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.286+/-0.032 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:22.27 -04:53:37.4: 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 07:03:22.27 -04:53:37.4: 15.40 +/- 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 3101509138446206464,2461155.6093,12.35,0.05,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 3101509138446206464 20260425.1093 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 25.1093 2461155.6093 12.32 07:18:22.34 +00:01:08.7
215.99652 5.99869 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 3111050081870866944 | 07:18:22.49 +00:01:21.5 (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 07:18:22.34 +00:01:08.7: 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 07:18:22.34 +00:01:08.7: 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
Gaia DR3 3111050081870866944,2461155.6093,12.32,0.05,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 3111050081870866944 20260425.1093 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 25.1093 2461155.6093 12.23 06:57:47.57 +00:12:34.3
213.46997 1.50947 galactic Mon Second-epoch detections are separated by 2.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112935744312153600 | 06:57:49.11 +00:12:18.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1956ApJS....2..271M LF 9 +00 372 J-Ks=0.865+/-0.038 (M)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:47.57 +00:12:34.3: 13.13 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:47.57 +00:12:34.3: 15.57 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.13 +/- 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 3112935744312153600,2461155.6093,12.23,0.05,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
Gaia DR3 3112935744312153600 20260425.1093 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 25.1093 2461155.6093 12.30 07:10:16.97 -04:37:52.6
219.20462 2.06550 galactic Mon Second-epoch detections are separated by 3.6" and 5.9 pix
The object was found in VSX 4" Gaia DR3 3059462198893051776
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.350 G 13.380 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 07:10:16.97 -04:37:52.6: 14.51 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:10:16.97 -04:37:52.6: 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 3059462198893051776,2461155.6093,12.30,0.05,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 3059462198893051776 20260425.1093 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.31 07:03:26.98 -05:01:12.3
218.76764 0.37496 galactic Mon Second-epoch detections are separated by 0.6" and 6.2 pix
The object was found in VSX 3" Gaia DR3 3101503056772630528
Type: VAR
# Max. Min./Amp. JD0 Period
13.310 G 13.350 G 0.024475800000 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 07:03:26.98 -05:01:12.3: 14.42 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:26.98 -05:01:12.3: 15.12 +/- 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 3101503056772630528,2461155.6093,12.31,0.05,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 3101503056772630528 20260425.1093 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 25.1093 2461155.6093 12.19 06:59:30.36 +00:22:07.0
213.52374 1.96318 galactic Mon Second-epoch detections are separated by 1.4" and 6.2 pix
The object was found in VSX24" Gaia DR3 3112954088113989888
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.730 G 13.760 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 06:59:30.36 +00:22:07.0: 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 06:59:30.36 +00:22:07.0: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 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 3112954088113989888,2461155.6093,12.19,0.05,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 3112954088113989888 20260425.1093 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 25.1093 2461155.6093 12.23 06:50:59.53 -02:47:53.0
215.37185 -1.37455 galactic Mon Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3105904607971898368 | 06:50:58.10 -02:47:57.2 (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 06:50:59.53 -02:47:53.0: 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 06:50:59.53 -02:47:53.0: 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 3105904607971898368,2461155.6093,12.23,0.05,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
Gaia DR3 3105904607971898368 20260425.1093 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 25.1093 2461155.6093 12.13 06:57:31.08 +00:41:49.0
213.00466 1.67056 galactic Mon Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.3772+00.7028 | 06:57:31.08 +00:41:49.0 (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 06:57:31.08 +00:41:49.0: 13.97 +/- 0.15 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:31.08 +00:41:49.0: 13.94 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.95 +/- 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 J104.3772+00.7028,2461155.6093,12.13,0.05,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 J104.3772+00.7028 20260425.1093 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 25.1093 2461155.6093 12.14 07:13:10.29 -05:21:11.2
220.17772 2.37065 galactic Mon Second-epoch detections are separated by 6.8" and 7.2 pix
The object was found in VSX17" GDS_J0713093-052101
Type: VAR
# Max. Min./Amp. JD0 Period
12.650 r Y 0.070 r
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 07:13:10.29 -05:21:11.2: 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 07:13:10.29 -05:21:11.2: 13.65 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.09
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0713093-052101,2461155.6093,12.14,0.05,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
GDS_J0713093-052101 20260425.1093 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.07 07:00:35.32 -02:31:06.9
216.21676 0.88548 galactic Mon Second-epoch detections are separated by 1.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3108930086014619392 | 07:00:35.95 -02:31:28.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956ApJS....2..271M LF 9 -03 498 J-Ks=0.116+/-0.035 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:00:35.32 -02:31:06.9: 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 07:00:35.32 -02:31:06.9: 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 3108930086014619392,2461155.6093,12.07,0.05,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
Gaia DR3 3108930086014619392 20260425.1093 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 25.1093 2461155.6093 12.15 07:13:11.72 +01:02:12.9
214.49215 5.31330 galactic Mon Second-epoch detections are separated by 1.7" and 6.1 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 J108.2988+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 07:13:11.72 +01:02:12.9: 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 07:13:11.72 +01:02:12.9: 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+01.0363,2461155.6093,12.15,0.05,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 J108.2988+01.0363 20260425.1093 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 25.1093 2461155.6093 12.04 07:17:13.03 -00:34:59.2
216.40114 5.46582 galactic Mon Second-epoch detections are separated by 1.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3110248911552350208 | 07:17:13.89 -00:34:41.2 (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 07:17:13.03 -00:34:59.2: 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 07:17:13.03 -00:34:59.2: 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
Gaia DR3 3110248911552350208,2461155.6093,12.04,0.05,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
Gaia DR3 3110248911552350208 20260425.1093 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.15 06:58:50.25 -01:53:11.2
215.45450 0.78520 galactic Mon Second-epoch detections are separated by 4.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:58:50.25 -01:53:11.2 (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 06:58:50.25 -01:53:11.2: 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 06:58:50.25 -01:53:11.2: 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,2461155.6093,12.15,0.05,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
target 20260425.1093 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 25.1093 2461155.6093 12.01 07:05:00.04 +01:38:42.5
213.01270 3.76743 galactic Mon Second-epoch detections are separated by 1.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.2479+01.6428 | 07:05:00.04 +01:38:42.5 (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 07:05:00.04 +01:38:42.5: 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 07:05:00.04 +01:38:42.5: 14.67 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.67 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.2479+01.6428,2461155.6093,12.01,0.05,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
ATO J106.2479+01.6428 20260425.1093 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 25.1093 2461155.6093 12.01 07:08:41.86 +01:18:47.7
213.73083 4.43881 galactic CMi Second-epoch detections are separated by 1.6" and 6.2 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 07:08:41.86 +01:18:47.7: 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 07:08:41.86 +01:18:47.7: 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 3114481588940149120,2461155.6093,12.01,0.05,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 20260425.1093 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 25.1093 2461155.6093 12.06 06:55:20.59 +00:53:19.7
212.58594 1.27413 galactic Mon Second-epoch detections are separated by 1.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:55:20.59 +00:53:19.7 (user input) | T | P | (position from user input) SpType: A1IV (LAMOST DR5) J-Ks=0.129+/-0.037 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:55:20.59 +00:53:19.7: 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 06:55:20.59 +00:53:19.7: 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
target,2461155.6093,12.06,0.05,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
target 20260425.1093 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 25.1093 2461155.6093 11.98 06:59:09.54 +00:41:52.9
213.19080 2.03617 galactic Mon Second-epoch detections are separated by 1.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.7937+00.6981 | 06:59:10.49 +00:41:53.4 (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 06:59:09.54 +00:41:52.9: 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 06:59:09.54 +00:41:52.9: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.7937+00.6981,2461155.6093,11.98,0.05,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 J104.7937+00.6981 20260425.1093 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.05 07:12:26.22 +01:50:34.1
213.68485 5.51193 galactic CMi Second-epoch detections are separated by 0.9" 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 | target | 07:12:26.22 +01:50:34.1 (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 07:12:26.22 +01:50:34.1: 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 07:12:26.22 +01:50:34.1: 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,2461155.6093,12.05,0.05,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
target 20260425.1093 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 25.1093 2461155.6093 12.14 07:03:14.42 +01:07:06.3
213.28171 3.13585 galactic Mon Second-epoch detections are separated by 1.6" and 6.1 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 J105.8095+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 07:03:14.42 +01:07:06.3: 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 07:03:14.42 +01:07:06.3: 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+01.1236,2461155.6093,12.14,0.05,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 20260425.1093 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.17 07:15:49.73 -00:37:01.5
216.27148 5.14188 galactic Mon Second-epoch detections are separated by 2.0" and 6.1 pix
The object was found in VSX17" 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 07:15:49.73 -00:37:01.5: 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 07:15:49.73 -00:37:01.5: 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 3110157583366513664,2461155.6093,12.17,0.05,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 20260425.1093 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.05 07:18:17.99 -00:24:26.0
216.36897 5.78702 galactic Mon Second-epoch detections are separated by 1.9" 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 | ATO J109.5734-00.4114 | 07:18:17.99 -00:24:26.0 (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 07:18:17.99 -00:24:26.0: 13.99 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:18:17.99 -00:24:26.0: 15.34 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.99 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.5734-00.4114,2461155.6093,12.05,0.05,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 J109.5734-00.4114 20260425.1093 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 25.1093 2461155.6093 12.04 06:58:09.65 +00:53:07.1
212.91021 1.89945 galactic Mon Second-epoch detections are separated by 1.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.5385+00.8812 | 06:58:08.79 +00:53:19.8 (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 06:58:09.65 +00:53:07.1: 14.78 +/- 0.33 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:09.65 +00:53:07.1: 15.44 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.78 +/- 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 J104.5385+00.8812,2461155.6093,12.04,0.05,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 J104.5385+00.8812 20260425.1093 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.97 07:18:04.95 -01:25:37.0
217.25369 5.26999 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 | ATO J109.5177-01.4272 | 07:18:04.95 -01:25:37.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A6IV (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:18:04.95 -01:25:37.0: 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 07:18:04.95 -01:25:37.0: 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
ATO J109.5177-01.4272,2461155.6093,11.97,0.05,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
ATO J109.5177-01.4272 20260425.1093 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 25.1093 2461155.6093 12.02 07:10:41.27 -05:05:04.7
219.65373 1.94608 galactic Mon Second-epoch detections are separated by 1.9" and 6.6 pix
The object was found in VSX15" Gaia DR3 3059365613665871360
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.930 G 12.960 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 07:10:41.27 -05:05:04.7: 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 07:10:41.27 -05:05:04.7: 15.10 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.10 +/- 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 3059365613665871360,2461155.6093,12.02,0.05,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
Gaia DR3 3059365613665871360 20260425.1093 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 25.1093 2461155.6093 12.04 07:00:12.55 +00:10:02.4
213.78320 2.02782 galactic Mon Second-epoch detections are separated by 1.3" 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 3112899426068950528 | 07:00:11.28 +00:10:01.8 (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 07:00:12.55 +00:10:02.4: 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 07:00:12.55 +00:10:02.4: 15.58 +/- 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 3112899426068950528,2461155.6093,12.04,0.05,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
Gaia DR3 3112899426068950528 20260425.1093 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.97 07:01:00.95 -00:25:44.2
214.40617 1.93515 galactic Mon Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 07:01:00.95 -00:25:44.2: 14.19 +/- 0.19 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:00.95 -00:25:44.2: 15.15 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.19 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.2433-00.4249,2461155.6093,11.97,0.05,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
ATO J105.2433-00.4249 20260425.1093 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 25.1093 2461155.6093 11.89 06:59:40.22 -00:40:25.3
214.47041 1.52416 galactic Mon Second-epoch detections are separated by 0.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:59:40.22 -00:40:25.3 (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 06:59:40.22 -00:40:25.3: 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 06:59:40.22 -00:40:25.3: 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
target,2461155.6093,11.89,0.05,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 20260425.1093 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.92 07:05:50.93 -02:05:13.9
216.43458 2.25121 galactic Mon Second-epoch detections are separated by 1.2" 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 | ATO J106.4621-02.0972 | 07:05:50.77 -02:05:30.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.072+/-0.037 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:50.93 -02:05:13.9: 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 07:05:50.93 -02:05:13.9: 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
ATO J106.4621-02.0972,2461155.6093,11.92,0.05,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
ATO J106.4621-02.0972 20260425.1093 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 25.1093 2461155.6093 11.85 07:12:11.75 -01:59:49.6
217.08289 3.70157 galactic Mon Second-epoch detections are separated by 0.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 07:12:11.75 -01:59:49.6: 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 07:12:11.75 -01:59:49.6: 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 J108.0562-02.0008,2461155.6093,11.85,0.05,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 J108.0562-02.0008 20260425.1093 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 25.1093 2461155.6093 11.78 07:05:08.36 -04:26:25.2
218.44547 1.01492 galactic Mon Second-epoch detections are separated by 2.4" and 5.9 pix
The object was found in VSX 2" 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 07:05:08.36 -04:26:25.2: 14.32 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:08.36 -04:26:25.2: 15.47 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.32 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101552603515643008,2461155.6093,11.78,0.05,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 20260425.1093 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.86 06:59:25.58 -01:04:49.6
214.80455 1.28419 galactic Mon Second-epoch detections are separated by 0.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:25.58 -01:04:49.6: 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 06:59:25.58 -01:04:49.6: 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 J104.8632-01.0847,2461155.6093,11.86,0.05,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 20260425.1093 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.76 07:02:21.41 -04:03:30.8
217.78814 0.57334 galactic Mon Second-epoch detections are separated by 1.0" and 6.2 pix
The object was found in VSX 1" Gaia DR3 3101821880779349888
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.760 G 12.780 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 07:02:21.41 -04:03:30.8: 13.83 +/- 0.16 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:21.41 -04:03:30.8: 15.42 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.83 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101821880779349888,2461155.6093,11.76,0.05,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 3101821880779349888 20260425.1093 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 25.1093 2461155.6093 11.76 07:07:15.17 -04:18:17.6
218.56706 1.54513 galactic Mon Second-epoch detections are separated by 0.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.8127-04.3106 | 07:07:15.05 -04:18:38.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A 1949AnHar.112....1C HD 296496 J-Ks=0.233+/-0.050 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:15.17 -04:18:17.6: 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 07:07:15.17 -04:18:17.6: 15.53 +/- 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 J106.8127-04.3106,2461155.6093,11.76,0.05,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
ATO J106.8127-04.3106 20260425.1093 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 25.1093 2461155.6093 11.69 07:10:02.16 -03:03:52.9
217.78422 2.73181 galactic Mon Second-epoch detections are separated by 0.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.5103-03.0625 | 07:10:01.65 -03:04:17.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1949AnHar.112....1C HD 296399 J-Ks=0.238+/-0.035 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:10:02.16 -03:03:52.9: 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 07:10:02.16 -03:03:52.9: 14.80 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.80 +/- 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 J107.5103-03.0625,2461155.6093,11.69,0.05,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
ATO J107.5103-03.0625 20260425.1093 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.62 07:17:01.01 -00:19:59.4
216.15495 5.53602 galactic Mon Second-epoch detections are separated by 1.2" and 6.1 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 3111013381370932096 | 07:17:01.71 -00:19:47.3 (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 07:17:01.01 -00:19:59.4: 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 07:17:01.01 -00:19:59.4: 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 3111013381370932096,2461155.6093,11.62,0.05,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
Gaia DR3 3111013381370932096 20260425.1093 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 25.1093 2461155.6093 11.62 07:03:52.74 +00:49:48.2
213.61163 3.14651 galactic Mon Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.9684+00.8315 | 07:03:52.59 +00:49:31.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.172+/-0.031 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:52.74 +00:49:48.2: 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 07:03:52.74 +00:49:48.2: 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 J105.9684+00.8315,2461155.6093,11.62,0.05,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 J105.9684+00.8315 20260425.1093 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 25.1093 2461155.6093 11.62 07:02:00.71 +01:40:09.6
212.65047 3.11344 galactic Mon Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3115398203683281280 | 07:01:59.61 +01:40:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.374+/-0.030 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:00.71 +01:40:09.6: 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 07:02:00.71 +01:40:09.6: 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 3115398203683281280,2461155.6093,11.62,0.05,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
Gaia DR3 3115398203683281280 20260425.1093 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 25.1093 2461155.6093 11.51 07:04:20.84 -04:41:01.3
218.57119 0.72791 galactic Mon Second-epoch detections are separated by 0.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 07:04:20.84 -04:41:01.3: 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 07:04:20.84 -04:41:01.3: 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 3101541986356735360,2461155.6093,11.51,0.05,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 3101541986356735360 20260425.1093 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 25.1093 2461155.6093 11.21 07:09:39.86 -05:35:35.0
219.98762 1.48563 galactic Mon Second-epoch detections are separated by 1.1" and 6.5 pix
The object was found in VSX25" ASAS J070940-0536.0
Type: SR
# Max. Min./Amp. JD0 Period
8.244 Ic Y 0.070 Ic 2452490.60000 37.290000000000 M5
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 07:09:39.86 -05:35:35.0: 14.48 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:09:39.86 -05:35:35.0: 15.16 +/- 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 J070940-0536.0,2461155.6093,11.21,0.05,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 J070940-0536.0 20260425.1093 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.28 07:11:00.52 -02:53:38.9
217.74436 3.02588 galactic Mon Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 07:11:00.52 -02:53:38.9: 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 07:11:00.52 -02:53:38.9: 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 J107.7472-02.9052,2461155.6093,11.28,0.05,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 J107.7472-02.9052 20260425.1093 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.17 06:58:03.49 -05:54:02.5
218.93712 -1.22098 galactic Mon Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3100956290252215808 | 06:58:02.85 -05:54:24.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.253+/-0.032 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:58:03.49 -05:54:02.5: 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 06:58:03.49 -05:54:02.5: 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 3100956290252215808,2461155.6093,11.17,0.05,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 3100956290252215808 20260425.1093 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.09 07:08:43.92 -03:56:10.9
218.40923 2.04209 galactic Mon Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 07:08:43.92 -03:56:10.9: 12.71 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:43.92 -03:56:10.9: 15.35 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.71 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1828-03.9366,2461155.6093,11.09,0.05,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 J107.1828-03.9366 20260425.1093 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.10 07:02:47.42 -03:11:46.8
217.07104 1.06426 galactic Mon Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.6969-03.1929 | 07:02:48.14 -03:12:00.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A3 1949AnHar.112....1C HD 296072 J-Ks=0.604+/-0.032 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:47.42 -03:11:46.8: 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 07:02:47.42 -03:11:46.8: 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 J105.6969-03.1929,2461155.6093,11.10,0.05,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 J105.6969-03.1929 20260425.1093 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.07 07:12:39.25 -02:45:30.3
217.81300 3.45313 galactic Mon Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3108170594059819392 | 07:12:39.61 -02:45:45.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.496+/-0.033 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:39.25 -02:45:30.3: 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 07:12:39.25 -02:45:30.3: 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
Gaia DR3 3108170594059819392,2461155.6093,11.07,0.05,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
Gaia DR3 3108170594059819392 20260425.1093 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 10.82 06:54:05.71 -03:49:50.5
216.64423 -1.15562 galactic Mon Second-epoch detections are separated by 0.4" and 6.3 pix
The object was found in VSX23" Gaia DR3 3102714443704002688
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.430 G 13.460 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 06:54:05.71 -03:49:50.5: 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 06:54:05.71 -03:49:50.5: 15.32 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.32 +/- 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 3102714443704002688,2461155.6093,10.82,0.05,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 3102714443704002688 20260425.1093 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 10.70 07:14:38.80 -03:56:24.7
219.09319 3.34953 galactic Mon Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 07:14:38.80 -03:56:24.7: 14.42 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:14:38.80 -03:56:24.7: 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 J108.6673-03.9395,2461155.6093,10.70,0.05,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 20260425.1093 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 10.60 07:03:55.55 -04:49:26.2
218.64769 0.57028 galactic Mon Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3101513158535482624 | 07:03:56.84 -04:49:22.0 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 296333 J-Ks=0.106+/-0.031 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:55.55 -04:49:26.2: 13.17 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:55.55 -04:49:26.2: 15.49 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.17 +/- 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 3101513158535482624,2461155.6093,10.60,0.05,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 3101513158535482624 20260425.1093 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 10.00 07:17:51.17 -01:41:37.6
217.46499 5.09617 galactic Mon Second-epoch detections are separated by 1.2" and 6.5 pix
The object was found in VSX19" 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 07:17:51.17 -01:41:37.6: 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 07:17:51.17 -01:41:37.6: 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 3109822923819222400,2461155.6093,10.00,0.05,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 20260425.1093 10.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 10.22 07:03:02.18 +01:23:58.0
213.00789 3.21849 galactic Mon Second-epoch detections are separated by 0.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 07:03:02.18 +01:23:58.0: 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 07:03:02.18 +01:23:58.0: 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+01.3967,2461155.6093,10.22,0.05,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
ATO J105.7726+01.3967 20260425.1093 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 10.70 06:53:07.39 -01:35:07.7
214.53506 -0.34804 galactic Mon Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 06:53:07.39 -01:35:07.7: 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 06:53:07.39 -01:35:07.7: 12.14 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112275315783496832,2461155.6093,10.70,0.05,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 20260425.1093 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.49 06:58:08.39 -01:38:52.7
215.16271 0.73900 galactic Mon Second-epoch detections are separated by 3.0" 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 3112051973180962048 | 06:58:08.30 -01:38:32.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1956ApJS....2..271M LF 9 -02 476
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:58:08.39 -01:38:52.7: 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 06:58:08.39 -01:38:52.7: 14.66 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.66 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112051973180962048,2461155.6093,11.49,0.05,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
Gaia DR3 3112051973180962048 20260425.1093 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.43 07:05:24.98 -00:59:48.6
215.41474 2.65419 galactic Mon Second-epoch detections are separated by 1.1" and 6.3 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 07:05:24.98 -00:59:48.6: 14.57 +/- 0.31 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:24.98 -00:59:48.6: 15.36 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.57 +/- 0.31
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109568627391618304,2461155.6093,11.43,0.05,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 3109568627391618304 20260425.1093 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 25.1093 2461155.6093 11.48 07:05:30.61 +01:36:36.6
213.10200 3.86487 galactic Mon Second-epoch detections are separated by 0.8" 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 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 07:05:30.61 +01:36:36.6: 14.05 +/- 0.20 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:30.61 +01:36:36.6: 15.39 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.05 +/- 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 3114643388949636736,2461155.6093,11.48,0.05,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 3114643388949636736 20260425.1093 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.53 07:08:30.45 -01:56:44.1
216.61334 2.90649 galactic Mon Second-epoch detections are separated by 0.6" and 6.3 pix
The object was found in VSX 8" Gaia DR3 3109213450777879808
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
15.350 G 15.390 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 07:08:30.45 -01:56:44.1: 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 07:08:30.45 -01:56:44.1: 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 3109213450777879808,2461155.6093,11.53,0.05,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 3109213450777879808 20260425.1093 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.73 07:01:24.07 +01:06:07.7
213.08646 2.71923 galactic Mon Second-epoch detections are separated by 0.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 07:01:24.07 +01:06:07.7: 13.67 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:24.07 +01:06:07.7: 14.92 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.94 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113861670543456896,2461155.6093,11.73,0.05,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 3113861670543456896 20260425.1093 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.71 07:06:24.10 +00:20:28.4
214.33554 3.48470 galactic Mon Second-epoch detections are separated by 1.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3114263159786050944 | 07:06:23.17 +00:20:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A 1949AnHar.112....1C HD 293175 J-Ks=0.194+/-0.035 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:06:24.10 +00:20:28.4: 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 07:06:24.10 +00:20:28.4: 13.91 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.91 +/- 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 3114263159786050944,2461155.6093,11.71,0.05,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 3114263159786050944 20260425.1093 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.86 07:13:48.27 -00:49:58.0
216.23085 4.59327 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 | 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 -00:49:58.0: 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 07:13:48.27 -00:49:58.0: 15.20 +/- 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 3110877252388089856,2461155.6093,11.86,0.05,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 20260425.1093 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 11.87 06:56:12.23 +00:18:26.3
213.20173 1.20052 galactic Mon Second-epoch detections are separated by 1.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113702584955259648 | 06:56:13.80 +00:18:21.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8V 1956ApJS....2..271M LF 9 +00 328
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:56:12.23 +00:18:26.3: 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 06:56:12.23 +00:18:26.3: 14.23 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113702584955259648,2461155.6093,11.87,0.05,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 3113702584955259648 20260425.1093 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.20 07:14:57.39 -05:11:43.0
220.24341 2.83762 galactic Mon Second-epoch detections are separated by 1.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J108.7462-05.1977 | 07:14:57.33 -05:12:11.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.133+/-0.037 (A)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:14:57.39 -05:11:43.0: 14.15 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:14:57.39 -05:11:43.0: 15.25 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.15 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.7462-05.1977,2461155.6093,12.20,0.05,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 J108.7462-05.1977 20260425.1093 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.19 06:54:57.30 -01:11:47.8
214.39781 0.23674 galactic Mon Second-epoch detections are separated by 1.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 06:54:57.30 -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 06:54:57.30 -01:11:47.8: 15.55 +/- 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 J103.7386-01.1974,2461155.6093,12.19,0.05,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
ATO J103.7386-01.1974 20260425.1093 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 25.1093 2461155.6093 12.11 07:05:49.13 +01:38:16.9
213.11234 3.94624 galactic Mon Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 07:05:49.13 +01:38:16.9: 13.32 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:49.13 +01:38:16.9: 14.43 +/- 0.14 detection
Forced photometry reference-image weighted average: 13.70 +/- 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+01.6243,2461155.6093,12.11,0.05,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 20260425.1093 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.21 06:59:50.16 +00:16:20.9
213.64699 1.99275 galactic Mon Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:59:50.16 +00:16:20.9 (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 06:59:50.16 +00:16:20.9: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:50.16 +00:16:20.9: 15.55 +/- 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,2461155.6093,12.21,0.05,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 20260425.1093 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.21 06:52:46.10 -01:34:15.7
214.48177 -0.42038 galactic Mon Second-epoch detections are separated by 1.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 06:52:46.10 -01:34:15.7: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:46.10 -01:34:15.7: 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 3112286925076234752,2461155.6093,12.21,0.05,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 20260425.1093 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.19 06:51:14.95 -04:32:31.6
216.95469 -2.11130 galactic Mon Second-epoch detections are separated by 1.2" 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 3102286596240635008 | 06:51:13.50 -04:32:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B9 1949AnHar.112....1C HD 295687 J-Ks=0.314+/-0.061 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:51:14.95 -04:32:31.6: 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 06:51:14.95 -04:32:31.6: 15.38 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.38 +/- 0.29
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102286596240635008,2461155.6093,12.19,0.05,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 3102286596240635008 20260425.1093 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 25.1093 2461155.6093 12.18 06:52:07.76 +00:28:19.8
212.59051 0.36913 galactic Mon Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113577274989419904 | 06:52:06.22 +00:27:58.8 (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 06:52:07.76 +00:28:19.8: 13.08 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:07.76 +00:28:19.8: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113577274989419904,2461155.6093,12.18,0.05,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 3113577274989419904 20260425.1093 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 25.1093 2461155.6093 12.22 07:07:11.39 -02:58:18.8
217.37506 2.14326 galactic Mon Second-epoch detections are separated by 3.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 07:07:11.39 -02:58:18.8: 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 07:07:11.39 -02:58:18.8: 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 3107988968482458496,2461155.6093,12.22,0.05,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 3107988968482458496 20260425.1093 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 25.1093 2461155.6093 12.27 07:04:44.65 -03:46:31.1
217.80920 1.23238 galactic Mon Second-epoch detections are separated by 1.2" 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 | ATO J106.1874-03.7754 | 07:04:44.87 -03:47:04.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 1949AnHar.112....1C HD 296276
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:04:44.65 -03:46:31.1: 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 07:04:44.65 -03:46:31.1: 15.55 +/- 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 J106.1874-03.7754,2461155.6093,12.27,0.05,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
ATO J106.1874-03.7754 20260425.1093 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 25.1093 2461155.6093 12.29 06:57:00.74 +00:17:38.0
213.30586 1.37429 galactic Mon Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 06:57:00.74 +00:17:38.0: 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 06:57:00.74 +00:17:38.0: 15.65 +/- 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 3113688634901420928,2461155.6093,12.29,0.05,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 3113688634901420928 20260425.1093 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 25.1093 2461155.6093 12.21 06:58:26.68 -00:54:20.5
214.53699 1.14565 galactic Mon Second-epoch detections are separated by 1.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 06:58:26.68 -00:54:20.5: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:26.68 -00:54:20.5: 14.41 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.41 +/- 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
Gaia DR3 3112254596859130368,2461155.6093,12.21,0.05,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 20260425.1093 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.28 07:10:29.63 -04:23:43.2
219.01930 2.22086 galactic Mon Second-epoch detections are separated by 3.4" and 6.2 pix
The object was found in VSX 7" Gaia DR3 3059484429643337728
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 07:10:29.63 -04:23:43.2: 12.98 +/- 0.09 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:10:29.63 -04:23:43.2: 13.24 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059484429643337728,2461155.6093,12.28,0.05,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
Gaia DR3 3059484429643337728 20260425.1093 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 25.1093 2461155.6093 12.23 06:53:05.71 +00:29:07.9
212.68871 0.59012 galactic Mon Second-epoch detections are separated by 0.9" and 6.1 pix
The object was found in VSX23" Gaia DR3 3113392179077237376
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.330 G 14.360 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 06:53:05.71 +00:29:07.9: 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 06:53:05.71 +00:29:07.9: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.72 +/- 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 3113392179077237376,2461155.6093,12.23,0.05,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
Gaia DR3 3113392179077237376 20260425.1093 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 25.1093 2461155.6093 12.53 06:51:43.68 -00:26:00.9
213.35087 -0.13317 galactic Mon Second-epoch detections are separated by 0.7" and 6.1 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 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 06:51:43.68 -00:26:00.9: 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 06:51:43.68 -00:26:00.9: 14.67 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.67 +/- 0.16
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113180901047215360,2461155.6093,12.53,0.05,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 3113180901047215360 20260425.1093 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 25.1093 2461155.6093 12.35 07:16:22.46 -02:57:52.8
218.42553 4.18240 galactic Mon Second-epoch detections are separated by 1.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J109.0965-02.9684 | 07:16:22.46 -02:57:52.8 (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 07:16:22.46 -02:57:52.8: 13.98 +/- 0.23 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:16:22.46 -02:57:52.8: 14.96 +/- 0.28 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.18
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.0965-02.9684,2461155.6093,12.35,0.05,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
ATO J109.0965-02.9684 20260425.1093 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 25.1093 2461155.6093 12.34 06:52:57.37 -03:04:55.0
215.84808 -1.06739 galactic Mon Second-epoch detections are separated by 2.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:52:57.37 -03:04:55.0 (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 06:52:57.37 -03:04:55.0: 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 06:52:57.37 -03:04:55.0: 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
target,2461155.6093,12.34,0.05,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
target 20260425.1093 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 25.1093 2461155.6093 12.45 07:04:20.49 -00:08:22.7
214.52849 2.80693 galactic Mon Second-epoch detections are separated by 1.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112723499907565952 | 07:04:20.67 -00:07:56.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3 1949AnHar.112....1C HD 293065
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:04:20.49 -00:08:22.7: 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 07:04:20.49 -00:08:22.7: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 3112723499907565952,2461155.6093,12.45,0.05,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 3112723499907565952 20260425.1093 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 25.1093 2461155.6093 12.29 07:01:46.09 +01:19:50.1
212.92470 2.90496 galactic Mon Second-epoch detections are separated by 1.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3115367176839807872 | 07:01:47.56 +01:19:29.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.170+/-0.037 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:46.09 +01:19:50.1: 13.80 +/- 0.14 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:46.09 +01:19:50.1: 15.48 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.80 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115367176839807872,2461155.6093,12.29,0.05,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 3115367176839807872 20260425.1093 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 25.1093 2461155.6093 12.54 06:39:36.65 -04:34:34.5
215.66733 -4.71173 galactic Mon Second-epoch detections are separated by 1.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:39:36.65 -04:34:34.5 (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 06:39:36.65 -04:34:34.5: 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 06:39:36.65 -04:34:34.5: 14.00 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.00 +/- 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
target,2461155.6093,12.54,0.05,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 20260425.1093 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.43 06:57:11.88 -03:58:11.5
217.12111 -0.53036 galactic Mon Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.2896-03.9733 | 06:57:10.73 -03:58:39.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: B9 1949AnHar.112....1C HD 295858 J-Ks=0.342+/-0.033 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:11.88 -03:58:11.5: 14.50 +/- 0.27 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:11.88 -03:58:11.5: 14.64 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.61 +/- 0.14
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2896-03.9733,2461155.6093,12.43,0.05,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
ATO J104.2896-03.9733 20260425.1093 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 25.1093 2461155.6093 12.38 07:08:12.41 -03:12:25.9
217.70090 2.26079 galactic Mon Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:08:12.41 -03:12:25.9 (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 07:08:12.41 -03:12:25.9: 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 07:08:12.41 -03:12:25.9: 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,2461155.6093,12.38,0.05,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
target 20260425.1093 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 25.1093 2461155.6093 12.51 07:02:02.02 +00:07:46.9
214.02497 2.41653 galactic Mon Second-epoch detections are separated by 2.8" 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 | 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 07:02:02.02 +00:07:46.9: 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 07:02:02.02 +00:07:46.9: 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
ATO J105.5011+00.1277,2461155.6093,12.51,0.05,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 J105.5011+00.1277 20260425.1093 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 25.1093 2461155.6093 12.56 06:54:48.32 +00:23:19.3
212.96984 0.92647 galactic Mon Second-epoch detections are separated by 2.7" and 6.1 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 06:54:48.32 +00:23:19.3: 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 06:54:48.32 +00:23:19.3: 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+002321.1,2461155.6093,12.56,0.05,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 20260425.1093 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.55 06:59:40.39 -00:39:47.1
214.46129 1.52963 galactic Mon Second-epoch detections are separated by 2.2" 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 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 06:59:40.39 -00:39:47.1: 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 06:59:40.39 -00:39:47.1: 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 3112640181842895232,2461155.6093,12.55,0.05,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
Gaia DR3 3112640181842895232 20260425.1093 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 25.1093 2461155.6093 12.48 07:13:15.22 -00:27:59.6
215.84099 4.63878 galactic Mon Second-epoch detections are separated by 1.1" and 6.4 pix
The object was found in VSX22" Gaia DR3 3110970362981607424
Type: E
# Max. Min./Amp. JD0 Period
15.370 G 15.470 G 0.872020000000 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 07:13:15.22 -00:27:59.6: 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 07:13:15.22 -00:27:59.6: 15.40 +/- 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 3110970362981607424,2461155.6093,12.48,0.05,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 3110970362981607424 20260425.1093 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 25.1093 2461155.6093 12.50 07:06:31.76 -04:48:14.7
218.92772 1.15564 galactic Mon Second-epoch detections are separated by 1.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.6359-04.8059 | 07:06:30.76 -04:47:57.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.260+/-0.031 (Very red! L if it's a dwarf)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:06:31.76 -04:48:14.7: 14.05 +/- 0.20 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:06:31.76 -04:48:14.7: 15.37 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.05 +/- 0.20
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.6359-04.8059,2461155.6093,12.50,0.05,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
ATO J106.6359-04.8059 20260425.1093 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.50 07:08:43.17 -05:05:29.3
219.43390 1.50790 galactic Mon Second-epoch detections are separated by 3.4" and 6.4 pix
The object was found in VSX19" Gaia DR3 3053416980884797824
Type: RS
# Max. Min./Amp. JD0 Period
15.430 G 15.530 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 07:08:43.17 -05:05:29.3: 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 07:08:43.17 -05:05:29.3: 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
Gaia DR3 3053416980884797824,2461155.6093,12.50,0.05,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 3053416980884797824 20260425.1093 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.59 06:49:46.85 -03:36:01.0
215.94873 -2.00897 galactic Mon Second-epoch detections are separated by 2.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:49:46.85 -03:36:01.0 (user input) | T | P | (position from user input) SpType: F5IV 2012A&A...543A.125G CoRoT 110831125 J-Ks=0.253+/-0.035 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:49:46.85 -03:36:01.0: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:49:46.85 -03:36:01.0: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461155.6093,12.59,0.05,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 20260425.1093 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.54 06:50:50.97 -02:36:25.9
215.18566 -1.31933 galactic Mon Second-epoch detections are separated by 0.8" and 6.1 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 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 J-Ks=0.286+/-0.035 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:50:50.97 -02:36:25.9: 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 06:50:50.97 -02:36:25.9: 13.87 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 3105927800794434176,2461155.6093,12.54,0.05,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 20260425.1093 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.59 07:10:18.85 -06:07:57.8
220.54118 1.38020 galactic Mon Second-epoch detections are separated by 2.8" and 5.9 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 3053046892140239232 | 07:10:17.09 -06:08:17.4 (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 07:10:18.85 -06:07:57.8: 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 07:10:18.85 -06:07:57.8: 15.08 +/- 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 3053046892140239232,2461155.6093,12.59,0.05,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 3053046892140239232 20260425.1093 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.54 07:03:11.83 +01:45:15.4
212.70977 3.41584 galactic Mon Second-epoch detections are separated by 0.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3115408855201939072 | 07:03:10.55 +01:45:39.5 (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 07:03:11.83 +01:45:15.4: 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 07:03:11.83 +01:45:15.4: 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
Gaia DR3 3115408855201939072,2461155.6093,12.54,0.05,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 3115408855201939072 20260425.1093 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.59 07:01:59.85 -02:00:41.8
215.92674 1.43027 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 3109059209911958144 | 07:02:01.26 -02:00:24.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2V 1956ApJS....2..271M LF 9 -02 643
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:59.85 -02:00:41.8: 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 07:01:59.85 -02:00:41.8: 15.59 +/- 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 3109059209911958144,2461155.6093,12.59,0.05,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 3109059209911958144 20260425.1093 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.60 07:17:27.88 +00:52:46.6
215.12263 6.19086 galactic Mon Second-epoch detections are separated by 4.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3111553310299877760 | 07:17:27.78 +00:53:12.1 (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 07:17:27.88 +00:52:46.6: 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 07:17:27.88 +00:52:46.6: 14.87 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.87 +/- 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 3111553310299877760,2461155.6093,12.60,0.05,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 3111553310299877760 20260425.1093 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.69 06:54:07.36 -03:06:07.8
215.99883 -0.81742 galactic Mon Second-epoch detections are separated by 1.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:54:07.36 -03:06:07.8 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.039 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:07.36 -03:06:07.8: 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 06:54:07.36 -03:06:07.8: 15.37 +/- 0.35 detection
Forced photometry reference-image weighted average: 15.37 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461155.6093,12.69,0.05,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
target 20260425.1093 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 25.1093 2461155.6093 12.63 07:00:27.47 -00:07:02.7
214.06512 1.95322 galactic Mon Second-epoch detections are separated by 2.6" and 5.9 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 J105.1134-00.1178 | 07:00:27.47 -00:07:02.7 (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 07:00:27.47 -00:07:02.7: 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 07:00:27.47 -00:07:02.7: 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
ATO J105.1134-00.1178,2461155.6093,12.63,0.05,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 J105.1134-00.1178 20260425.1093 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.68 07:04:33.60 -04:28:40.3
218.41257 0.86940 galactic Mon Second-epoch detections are separated by 2.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:04:33.60 -04:28:40.3 (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 07:04:33.60 -04:28:40.3: 14.21 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:04:33.60 -04:28:40.3: 15.31 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.21 +/- 0.24
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461155.6093,12.68,0.05,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
target 20260425.1093 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 25.1093 2461155.6093 12.62 07:06:45.54 -01:30:49.7
216.02865 2.71599 galactic Mon Second-epoch detections are separated by 0.8" and 6.4 pix
The object was found in VSX 1" Gaia DR3 3109297872654329344
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.150 G 14.190 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 07:06:45.54 -01:30:49.7: 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 07:06:45.54 -01:30:49.7: 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
Gaia DR3 3109297872654329344,2461155.6093,12.62,0.05,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 3109297872654329344 20260425.1093 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 25.1093 2461155.6093 12.70 06:54:15.22 -02:04:22.9
215.09780 -0.31899 galactic Mon Second-epoch detections are separated by 1.2" and 6.2 pix
The object was found in VSX 3" Gaia DR3 3106053763595735040
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.740 G 13.760 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 06:54:15.22 -02:04:22.9: 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 06:54:15.22 -02:04:22.9: 14.27 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.27 +/- 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 3106053763595735040,2461155.6093,12.70,0.05,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 3106053763595735040 20260425.1093 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.62 06:59:35.88 -05:28:09.7
218.72827 -0.68323 galactic Mon Second-epoch detections are separated by 2.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3101380392503930240 | 06:59:37.79 -05:28:22.2 (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 06:59:35.88 -05:28:09.7: 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 06:59:35.88 -05:28:09.7: 15.37 +/- 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 3101380392503930240,2461155.6093,12.62,0.05,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 3101380392503930240 20260425.1093 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 25.1093 2461155.6093 12.59 07:12:56.91 +00:52:07.2
214.61420 5.18161 galactic Mon Second-epoch detections are separated by 0.8" and 6.2 pix
The object was found in VSX 1" Gaia DR3 3111409553452325120
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.630 G 13.660 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:56.91 +00:52:07.2: 14.49 +/- 0.35 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:56.91 +00:52:07.2: 15.28 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.49 +/- 0.35
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111409553452325120,2461155.6093,12.59,0.05,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 3111409553452325120 20260425.1093 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.65 07:01:00.36 -00:27:54.0
214.43714 1.91651 galactic Mon Second-epoch detections are separated by 1.2" and 6.3 pix
The object was found in VSX23" Gaia DR3 3112649905648673536
Type: E
# Max. Min./Amp. JD0 Period
15.800 G 15.920 G 11.931300000000
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 07:01:00.36 -00:27:54.0: 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 07:01:00.36 -00:27:54.0: 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 3112649905648673536,2461155.6093,12.65,0.05,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 3112649905648673536 20260425.1093 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.72 06:44:39.52 +00:10:06.0
212.00908 -1.43153 galactic Mon Second-epoch detections are separated by 1.4" and 6.1 pix
The object was found in VSX 6" Gaia DR3 3125504223071142784
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.400 G 14.420 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 06:44:39.52 +00:10:06.0: 13.49 +/- 0.11 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:39.52 +00:10:06.0: 13.54 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.52 +/- 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 3125504223071142784,2461155.6093,12.72,0.05,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 3125504223071142784 20260425.1093 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.58 07:01:49.00 -03:26:19.2
217.17528 0.73728 galactic Mon Second-epoch detections are separated by 1.8" and 6.1 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 3108614766697923456 | 07:01:50.08 -03:26:04.4 (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 07:01:49.00 -03:26:19.2: 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 07:01:49.00 -03:26:19.2: 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
Gaia DR3 3108614766697923456,2461155.6093,12.58,0.05,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 3108614766697923456 20260425.1093 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.62 06:50:00.14 -03:51:11.7
216.19931 -2.07484 galactic Mon Second-epoch detections are separated by 2.9" and 6.0 pix
The object was found in VSX 4" Gaia DR3 3102406339927761536
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.700 G 13.730 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 06:50:00.14 -03:51:11.7: 14.72 +/- 0.32 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:50:00.14 -03:51:11.7: 13.67 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 3102406339927761536,2461155.6093,12.62,0.05,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 3102406339927761536 20260425.1093 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 25.1093 2461155.6093 12.63 06:55:10.24 -02:56:00.4
215.96799 -0.50763 galactic Mon Second-epoch detections are separated by 1.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3102925000179656192 | 06:55:08.85 -02:56:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1956ApJS....2..271M LF 9 -03 305 J-Ks=12.825+/- (unrealisitic color!)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:55:10.24 -02:56:00.4: 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 06:55:10.24 -02:56:00.4: 14.79 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.79 +/- 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 3102925000179656192,2461155.6093,12.63,0.05,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
Gaia DR3 3102925000179656192 20260425.1093 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.63 06:56:49.12 +00:46:33.2
212.85465 1.55095 galactic Mon Second-epoch detections are separated by 1.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.2021+00.7657 | 06:56:49.12 +00:46:33.2 (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 06:56:49.12 +00:46:33.2: 13.90 +/- 0.15 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:56:49.12 +00:46:33.2: 15.37 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.90 +/- 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 J104.2021+00.7657,2461155.6093,12.63,0.05,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 J104.2021+00.7657 20260425.1093 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.74 06:46:16.99 -05:17:46.5
217.06528 -3.55577 galactic Mon Second-epoch detections are separated by 1.8" 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 | ATO J101.5668-05.2956 | 06:46:14.58 -05:17:55.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.416+/-0.033 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:46:16.99 -05:17:46.5: 13.79 +/- 0.19 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:46:16.99 -05:17:46.5: 15.23 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.79 +/- 0.19
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.5668-05.2956,2461155.6093,12.74,0.05,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
ATO J101.5668-05.2956 20260425.1093 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 25.1093 2461155.6093 12.72 06:58:24.59 -03:02:34.6
216.43455 0.16192 galactic Mon Second-epoch detections are separated by 0.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 06:58:24.59 -03:02:34.6: 14.37 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:24.59 -03:02:34.6: 15.26 +/- 0.34 detection
Forced photometry reference-image weighted average: 14.67 +/- 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 3102885172944943488,2461155.6093,12.72,0.05,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 20260425.1093 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.78 06:59:34.21 -02:33:57.8
216.14271 0.63753 galactic Mon Second-epoch detections are separated by 0.3" and 6.2 pix
The object was found in VSX 3" Gaia DR3 3108920254829056000
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.010 G 14.040 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 06:59:34.21 -02:33:57.8: 14.31 +/- 0.22 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:34.21 -02:33:57.8: 15.46 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.31 +/- 0.22
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108920254829056000,2461155.6093,12.78,0.05,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 3108920254829056000 20260425.1093 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.84 06:52:51.61 -02:22:45.2
215.21158 -0.76843 galactic Mon Second-epoch detections are separated by 1.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J103.2108-02.3799 | 06:52:51.61 -02:22:45.2 (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 06:52:51.61 -02:22:45.2: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:51.61 -02:22:45.2: 14.93 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.93 +/- 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 J103.2108-02.3799,2461155.6093,12.84,0.05,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
ATO J103.2108-02.3799 20260425.1093 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 25.1093 2461155.6093 12.68 07:05:41.67 -01:29:58.7
215.89412 2.48596 galactic Mon Second-epoch detections are separated by 1.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.4248-01.4982 | 07:05:41.67 -01:29:58.7 (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 07:05:41.67 -01:29:58.7: 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 07:05:41.67 -01:29:58.7: 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
ATO J106.4248-01.4982,2461155.6093,12.68,0.05,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
ATO J106.4248-01.4982 20260425.1093 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 25.1093 2461155.6093 12.77 06:51:08.17 -02:08:43.6
214.80716 -1.04521 galactic Mon Second-epoch detections are separated by 0.6" and 6.2 pix
The object was found in VSX22" ZTF J065108.49-020905.3
Type: BY
# Max. Min./Amp. JD0 Period
16.342 r Y 0.107 r 2458375.90760 9.551564200000
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 06:51:08.17 -02:08:43.6: 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 06:51:08.17 -02:08:43.6: 14.30 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J065108.49-020905.3,2461155.6093,12.77,0.05,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
ZTF J065108.49-020905.3 20260425.1093 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.69 07:04:26.89 +00:59:22.0
213.53450 3.34580 galactic Mon Second-epoch detections are separated by 3.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3114548590432067072 | 07:04:28.27 +00:58:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B8 1949AnHar.112....1C HD 289581 J-Ks=0.701+/-0.030 (K)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:04:26.89 +00:59:22.0: 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 07:04:26.89 +00:59:22.0: 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
Gaia DR3 3114548590432067072,2461155.6093,12.69,0.05,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 3114548590432067072 20260425.1093 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 25.1093 2461155.6093 12.80 06:54:00.04 -05:06:47.0
217.77546 -1.76073 galactic Mon Second-epoch detections are separated by 2.8" and 5.8 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 J103.4970-05.1141 | 06:53:58.83 -05:07:05.9 (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 06:54:00.04 -05:06:47.0: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:00.04 -05:06:47.0: 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
ATO J103.4970-05.1141,2461155.6093,12.80,0.05,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
ATO J103.4970-05.1141 20260425.1093 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.74 06:55:24.68 -00:53:53.6
214.18431 0.47437 galactic Mon Second-epoch detections are separated by 3.8" and 5.9 pix
The object was found in VSX 4" Gaia DR3 3112432305426346496
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.300 G 14.330 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 06:55:24.68 -00:53:53.6: 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 06:55:24.68 -00:53:53.6: 13.70 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.70 +/- 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 3112432305426346496,2461155.6093,12.74,0.05,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 3112432305426346496 20260425.1093 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 25.1093 2461155.6093 12.82 06:57:24.07 -02:57:03.4
216.23770 -0.02009 galactic Mon Second-epoch detections are separated by 0.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.3550-02.9498 | 06:57:24.07 -02:57:03.4 (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 06:57:24.07 -02:57:03.4: 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 06:57:24.07 -02:57:03.4: 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
ATO J104.3550-02.9498,2461155.6093,12.82,0.05,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
ATO J104.3550-02.9498 20260425.1093 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.95 06:48:45.19 +01:09:19.8
211.59750 -0.07036 galactic Mon Second-epoch detections are separated by 1.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.1800+01.1786 | 06:48:44.22 +01:10:02.1 (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 06:48:45.19 +01:09:19.8: 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 06:48:45.19 +01:09:19.8: 13.74 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 J102.1800+01.1786,2461155.6093,12.95,0.05,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 J102.1800+01.1786 20260425.1093 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.79 07:00:54.96 -03:04:10.3
216.74416 0.70625 galactic Mon Second-epoch detections are separated by 2.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 07:00:54.96 -03:04:10.3: 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 07:00:54.96 -03:04:10.3: 15.24 +/- 0.30 detection
Forced photometry reference-image weighted average: 15.24 +/- 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 3108690216381698304,2461155.6093,12.79,0.05,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 20260425.1093 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.79 06:56:39.00 -01:28:50.8
214.84398 0.48405 galactic Mon Second-epoch detections are separated by 2.5" and 6.0 pix
The object was found in VSX 4" Gaia DR3 3112107777697271296
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.850 G 13.880 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 06:56:39.00 -01:28:50.8: 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 06:56:39.00 -01:28:50.8: 15.67 +/- 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 3112107777697271296,2461155.6093,12.79,0.05,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 3112107777697271296 20260425.1093 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.80 07:05:06.30 -04:50:35.6
218.79956 0.82246 galactic Mon Second-epoch detections are separated by 3.0" and 6.2 pix
The object was found in VSX 1" Gaia DR3 3101486289219649920
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.770 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 07:05:06.30 -04:50:35.6: 14.64 +/- 0.34 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:06.30 -04:50:35.6: 15.29 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.64 +/- 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 3101486289219649920,2461155.6093,12.80,0.05,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 3101486289219649920 20260425.1093 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.00 06:54:55.00 -01:21:36.2
214.53889 0.15366 galactic Mon Second-epoch detections are separated by 1.2" 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 | ATO J103.7291-01.3664 | 06:54:55.00 -01:21:36.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.389+/-0.042 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:55.00 -01:21:36.2: 14.85 +/- 0.34 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:55.00 -01:21:36.2: 14.63 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.68 +/- 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 J103.7291-01.3664,2461155.6093,13.00,0.05,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 J103.7291-01.3664 20260425.1093 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.02 07:06:11.11 -02:50:59.9
217.15152 1.97628 galactic Mon Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.5462-02.8483 | 07:06:09.60 -02:50:36.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 1949AnHar.112....1C HD 296222
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:06:11.11 -02:50:59.9: 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 07:06:11.11 -02:50:59.9: 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
ATO J106.5462-02.8483,2461155.6093,13.02,0.05,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 J106.5462-02.8483 20260425.1093 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.02 06:40:24.07 -03:51:05.6
215.10875 -4.20786 galactic Mon Second-epoch detections are separated by 1.0" 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 3104083816714430592 | 06:40:23.65 -03:50:21.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 47819
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:40:24.07 -03:51:05.6: 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 06:40:24.07 -03:51:05.6: 13.75 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.75 +/- 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 3104083816714430592,2461155.6093,13.02,0.05,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
Gaia DR3 3104083816714430592 20260425.1093 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.08 07:09:21.54 +01:07:27.5
213.97509 4.49981 galactic Mon Second-epoch detections are separated by 1.0" and 6.2 pix
The object was found in VSX 3" Gaia DR3 3114460526421262848
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
14.120 G 14.150 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:09:21.54 +01:07:27.5: 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 07:09:21.54 +01:07:27.5: 15.40 +/- 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 3114460526421262848,2461155.6093,13.08,0.05,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 3114460526421262848 20260425.1093 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.95 06:59:49.61 -06:00:34.9
219.23495 -0.87950 galactic Mon Second-epoch detections are separated by 2.3" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:59:49.61 -06:00:34.9 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.036 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:49.61 -06:00:34.9: 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 06:59:49.61 -06:00:34.9: 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,2461155.6093,12.95,0.05,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 20260425.1093 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.02 06:51:34.23 -01:39:22.5
214.42115 -0.72565 galactic Mon Second-epoch detections are separated by 2.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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 06:51:34.23 -01:39:22.5: 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 06:51:34.23 -01:39:22.5: 15.33 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.33 +/- 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
ATO J102.9043-01.6544,2461155.6093,13.02,0.05,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 J102.9043-01.6544 20260425.1093 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.97 07:11:26.80 -03:39:48.3
218.47858 2.76890 galactic Mon Second-epoch detections are separated by 1.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.8637-03.6635 | 07:11:24.68 -03:39:42.1 (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 07:11:26.80 -03:39:48.3: 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 07:11:26.80 -03:39:48.3: 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 J107.8637-03.6635,2461155.6093,12.97,0.05,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 J107.8637-03.6635 20260425.1093 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 25.1093 2461155.6093 13.04 06:51:37.36 +01:29:00.1
211.63273 0.71742 galactic Mon Second-epoch detections are separated by 0.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3126072571803216256 | 06:51:37.91 +01:28:26.5 (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 06:51:37.36 +01:29:00.1: 14.49 +/- 0.25 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:37.36 +01:29:00.1: 13.82 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.87 +/- 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 3126072571803216256,2461155.6093,13.04,0.05,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
Gaia DR3 3126072571803216256 20260425.1093 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 12.96 07:07:34.13 -03:14:12.8
217.65412 2.10569 galactic Mon Second-epoch detections are separated by 2.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.8958-03.2412 | 07:07:34.13 -03:14:12.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.321+/-0.043 (F)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:34.13 -03:14:12.8: 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 07:07:34.13 -03:14:12.8: 14.49 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.49 +/- 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 J106.8958-03.2412,2461155.6093,12.96,0.05,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 J106.8958-03.2412 20260425.1093 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.01 06:44:56.87 +00:56:56.5
211.34724 -1.01097 galactic Mon Second-epoch detections are separated by 0.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3125630499409158144 | 06:44:59.42 +00:56:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A3 1949AnHar.112....1C HD 289052
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:44:56.87 +00:56:56.5: 14.22 +/- 0.21 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:56.87 +00:56:56.5: 13.81 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.85 +/- 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 3125630499409158144,2461155.6093,13.01,0.05,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 3125630499409158144 20260425.1093 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.30 06:47:59.48 -01:20:54.9
213.73952 -1.38162 galactic Mon Second-epoch detections are separated by 0.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J101.9913-01.3476 | 06:47:58.93 -01:20:20.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 1956ApJS....2..271M LF 9 -02 84 J-Ks=0.423+/-0.094 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:47:59.48 -01:20:54.9: 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 06:47:59.48 -01:20:54.9: 14.06 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.06 +/- 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 J101.9913-01.3476,2461155.6093,13.30,0.05,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 J101.9913-01.3476 20260425.1093 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.12 06:57:44.45 -03:47:48.0
217.02883 -0.33083 galactic Mon Second-epoch detections are separated by 2.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.4331-03.7891 | 06:57:42.32 -03:47:34.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 1949AnHar.112....1C HD 295853
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:44.45 -03:47:48.0: 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 06:57:44.45 -03:47:48.0: 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 J104.4331-03.7891,2461155.6093,13.12,0.05,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
ATO J104.4331-03.7891 20260425.1093 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.23 06:54:22.77 -02:36:36.8
215.59022 -0.53602 galactic Mon Second-epoch detections are separated by 0.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3105951818253305728 | 06:54:25.04 -02:36:29.9 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE SpType: F2III 1956ApJS....2..271M LF 9 -03 274
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:22.77 -02:36:36.8: 13.57 +/- 0.11 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:22.77 -02:36:36.8: 14.29 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.93 +/- 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 3105951818253305728,2461155.6093,13.23,0.05,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
Gaia DR3 3105951818253305728 20260425.1093 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.54 06:51:16.10 -00:44:17.2
213.56951 -0.37429 galactic Mon Second-epoch detections are separated by 4.0" and 6.6 pix
The object was found in VSX 3" Gaia DR3 3113142624299169920
Type: RS
# Max. Min./Amp. JD0 Period
14.530 G 14.580 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 06:51:16.10 -00:44:17.2: 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 06:51:16.10 -00:44:17.2: 14.94 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.94 +/- 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 3113142624299169920,2461155.6093,13.54,0.05,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 3113142624299169920 20260425.1093 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.35 06:52:15.35 -01:03:58.8
213.97418 -0.30425 galactic Mon Second-epoch detections are separated by 4.1" 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 3112368911709379328 | 06:52:16.75 -01:03:52.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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 06:52:15.35 -01:03:58.8: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:15.35 -01:03:58.8: 14.77 +/- 0.17 detection
Forced photometry reference-image weighted average: 14.77 +/- 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 3112368911709379328,2461155.6093,13.35,0.05,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 3112368911709379328 20260425.1093 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.60 06:57:50.56 -00:57:55.8
214.52152 0.98447 galactic Mon Second-epoch detections are separated by 0.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:57:50.56 -00:57:55.8 (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 06:57:50.56 -00:57:55.8: 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 06:57:50.56 -00:57:55.8: 15.46 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.46 +/- 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
target,2461155.6093,13.60,0.05,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 20260425.1093 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.54 06:46:21.66 -00:23:11.6
212.69720 -1.30586 galactic Mon Second-epoch detections are separated by 1.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:46:21.66 -00:23:11.6 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.399+/-0.061 (G)
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:46:21.66 -00:23:11.6: 14.00 +/- 0.16 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:46:21.66 -00:23:11.6: 14.67 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461155.6093,13.54,0.05,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 20260425.1093 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 25.1093 2461155.6093 13.47 06:47:48.31 -01:09:01.5
213.54186 -1.33274 galactic Mon Second-epoch detections are separated by 1.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:47:48.31 -01:09:01.5 (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 06:47:48.31 -01:09:01.5: 14.91 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:47:48.31 -01:09:01.5: 14.42 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461155.6093,13.47,0.05,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
target 20260425.1093 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461155.6093,11.92,0.05,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
AK Mon 20260425.1093 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
## 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: 2461155.60955620 25.04.2026 02:37:35.656 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.94
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: 9 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): 29386
Objects passed selection criteria: 29296
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 23467
Average stars matched: 23007 (98.0398 %)
Memory usage VmPeak: 133824 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 Fri Apr 24 21:40:44 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: 2461155.60955620 25.04.2026 02:37:35.656 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 719
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: 256 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): 183556
Objects passed selection criteria: 183247
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 163812
Average stars matched: 158937 (97.0239 %)
Memory usage VmPeak: 2009164 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 Fri Apr 24 21:47:42 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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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: 2461155.60897248
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_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
Image size: 937.3'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: 06:51:27.274 -01:59:11.12 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 06:51:27.274 -01:59:11.12
Angular distance between the image centers 0.0439 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
Image size: 937.3'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: 06:51:24.968 -01:59:24.69 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 06:51:24.968 -01:59:24.69
Angular distance between the image centers 0.0361 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 06:51:27.274 -01:59:11.12
Second-epoch second image center 06:51:24.968 -01:59:24.69
Angular distance between the image centers 0.01032 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.JiiYOguusX
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.RSBqNkbMhr
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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits &> /tmp/tmp.EWZQtAY0o3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits &> /tmp/tmp.UEZ0Mj46b3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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 6 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_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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
14.2 mag. fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
14.2 mag. fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.4 (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.JiiYOguusX (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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/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.RSBqNkbMhr (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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/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.EWZQtAY0o3 (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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1751, passed=19088
Got 19088 stars (including 17319 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat
util/solve_plate_with_UCAC5 got 19088 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 18683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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 3.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 18680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 18679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.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.UEZ0Mj46b3 (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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1756, passed=19096
Got 19096 stars (including 17318 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 19096 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 18650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 18648 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 18647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51797.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 51588_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 51588_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:03:13.47 -02:58:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 3.435 3108665344231750784 105.80536966336 -02.98366744401 11.5158 10.8539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51590_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 51590_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:10:16.96 +01:29:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.78, MAG_FAINT_SEARCH_LIMIT=11.76)GAIADR2_OUTPUT=# 0.787 3114511825510240128 107.57076222618 +01.49863681537 10.7072 9.9163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51591_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 51591_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:07:17.10 +01:47:30.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51631_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 51631_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:37:38.14 +01:48:59.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51703_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 51703_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:03:02.16 +01:23:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 1.012 3114625143928364160 105.75911570779 +01.39910487476 11.2408 11.0074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51797_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 51797_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:45:28.30 -05:20:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 1.900 3100646605929886080 101.36801318123 -05.33771345461 11.4252 10.6825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Mon-02-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 ####
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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
Image size: 937.3'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: 06:51:27.274 -01:59:11.12 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 06:51:27.274 -01:59:11.12
Angular distance between the image centers 0.0439 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 937.3'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: 06:51:24.968 -01:59:24.69 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 06:51:24.968 -01:59:24.69
Angular distance between the image centers 0.0361 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 06:51:27.274 -01:59:11.12
Second-epoch second image center 06:51:24.968 -01:59:24.69
Angular distance between the image centers 0.01032 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.U8MdFd81BJ
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.hz0rqaS5qa
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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits &> /tmp/tmp.GPW39FO9dL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits &> /tmp/tmp.UtCCAFnbcR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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 583 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
2.2 pix fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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
13.5 mag. fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
13.5 mag. fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 12.9 (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.U8MdFd81BJ (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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/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.hz0rqaS5qa (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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/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.GPW39FO9dL (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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=17121, passed=148020
Got 148020 stars (including 130729 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat
util/solve_plate_with_UCAC5 got 148020 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 144729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 144729 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 144727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.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.UtCCAFnbcR (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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=17170, passed=148031
Got 148031 stars (including 130691 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 148031 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 143660 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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 143659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 143656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 926 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-36-45_20.00sec_-5.00C_LIGHT_0024.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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_2026-04-24_CI_Mon-02-Q2b1x1_213825_TTUQ2b1x1_2997574_CnzwtDKw/wcs_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025.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__out246477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246711.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246721.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246752.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246857.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246881.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out246990.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out247051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247065.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out248758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248778.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out248839.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out248877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248948.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out248999.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out249115.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out249194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out246590.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out246690.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out129332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246467.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246545.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__out246572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out247993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249217.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 395s
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: 148s
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Considering the candidate 246463_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246463_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:45:19.87 +00:59:32.5: 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 06:45:19.87 +00:59:32.5: 13.88 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.07
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Considering the candidate 246464_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246464_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246467_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246467_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246471_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246471_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246477_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246477_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:48:35.60 +00:16:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 4.262 3113510960692565248 102.14835692583 +00.26773302302 14.0882 13.5365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246478_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246478_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:42.54 -03:38:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.546 3102732443905284352 103.42748600938 -03.64716473221 14.0124 13.1027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246484_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246484_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:05.75 -02:59:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.654 3102932490602739456 103.52376521153 -02.98907259691 14.3500 13.8088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246487_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246487_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:01.27 +00:29:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.047 3113577549866799616 103.00495354139 +00.48327835342 14.0740 13.5981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246490_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246490_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246492_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246492_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:46:52.93 -02:18:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 3.862 3106163542958726016 101.72072078075 -02.30614112029 14.2635 13.7596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246497_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246497_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:03:25.62 +01:04:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 4.474 3114597754916518272 105.85659462129 +01.07854474038 14.1847 13.3025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246501_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246501_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:45:05.20 +01:54:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246502_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246502_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246504_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246504_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:51:40.84 -00:36:46.8: 14.55 +/- 0.28 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:40.84 -00:36:46.8: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.05
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Considering the candidate 246506_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246506_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246508_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246508_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:12.43 -00:22:24.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 246511_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246511_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246524_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246524_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246525_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246525_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246533_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246533_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:49:48.71 -02:24:16.0: 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 06:49:48.71 -02:24:16.0: 13.68 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.06
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Considering the candidate 246537_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246537_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246541_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246541_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:03:25.57 +00:30:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.817 3113014909149644800 105.85631451922 +00.50937572696 14.1968 13.5938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246542_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246542_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:49.05 -00:01:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.042 3113344693919326464 102.95463126522 -00.02844406435 14.0254 13.1735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246544_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246544_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246545_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246545_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246546_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246546_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:15:24.20 -03:45:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.554 3059946430681908096 108.85113662115 -03.75080832305 13.9526 13.5200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246547_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246547_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:48:52.45 +00:01:17.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 246555_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246555_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:06:09.65 +01:40:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.598 3114738462345623936 106.54001995350 +01.67373695407 13.8368 13.3807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246556_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246556_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:09:18.97 -01:02:04.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)
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Considering the candidate 246560_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246560_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246562_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246562_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246563_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246563_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:12.25 -01:38:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.290 3106282393294895616 103.05084692845 -01.63594856993 13.8388 13.2832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246572_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246572_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246576_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246576_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:26.56 -02:18:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.367 3105995729997787136 103.61075390990 -02.30575843373 13.8993 12.8680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246581_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246581_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246586_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246586_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246588_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246588_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246589_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246589_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246590_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246590_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:00:08.47 -00:53:10.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)
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Considering the candidate 246593_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246593_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246595_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246595_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:05:05.37 -01:20:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.793 3109483552679630848 106.27182408873 -01.34757338600 14.0116 13.3794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246599_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246599_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:08:05.73 -01:20:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.612 3109307489078739840 107.02347784580 -01.34677406656 13.7410 13.2441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246603_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246603_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:45:41.61 +01:54:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246605_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246605_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:52:54.11 -01:19:23.1: 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 06:52:54.11 -01:19:23.1: 15.56 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.51 +/- 0.10
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Considering the candidate 246606_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246606_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246611_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246611_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:15:05.38 -03:41:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.899 3059993984559810304 108.77212298728 -03.69080561438 13.8025 13.0620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246613_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246613_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246616_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246616_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:58:25.69 +00:09:36.4: 13.24 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:25.69 +00:09:36.4: 15.58 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.24 +/- 0.08
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Considering the candidate 246621_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246621_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:07:42.05 +02:06:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246626_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246626_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:46.96 +01:14:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 4.450 3114016907839549696 103.44545394980 +01.24053236295 13.8689 13.0160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246627_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246627_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246629_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246629_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246630_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246630_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246638_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246638_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:02:40.64 +02:19:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246642_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246642_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246643_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246643_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246648_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246648_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:42:20.32 -04:14:07.7: 14.10 +/- 0.18 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:42:20.32 -04:14:07.7: 13.61 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.06
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Considering the candidate 246657_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246657_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246659_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246659_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246660_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246660_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246662_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246662_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:48:54.76 -01:11:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 2.580 3107117403657526528 102.22825343963 -01.19129461822 13.7508 13.1636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246666_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246666_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:57:31.53 -00:23:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.974 3112478862871393408 104.38125970601 -00.39559567903 13.9610 13.3817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246667_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246667_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:49:53.81 +01:06:20.2: 12.55 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:49:53.81 +01:06:20.2: 13.53 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.04
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Considering the candidate 246677_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246677_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:05:25.41 -03:36:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 2.836 3107820060307074816 106.35605107274 -03.60946233271 13.9552 13.1959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246679_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246679_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:43:04.67 +01:03:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.555 3125820714918979840 100.76924916467 +01.05284958449 13.7488 12.9598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246681_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246681_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:10:06.74 +01:31:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.375 3114506293592372864 107.52847174994 +01.52114664367 13.8687 13.2191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246682_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246682_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:09:23.61 +01:30:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.953 3114508458255479936 107.34810748940 +01.51382395742 13.4403 12.6268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246685_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246685_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:58:59.45 -01:25:29.2: 12.77 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:59.45 -01:25:29.2: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.04
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Considering the candidate 246688_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246688_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 246690_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246690_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:10:14.40 -00:48:25.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)
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Considering the candidate 246695_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246695_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:58:27.11 -03:14:42.3: 12.79 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:27.11 -03:14:42.3: 15.42 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.79 +/- 0.06
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Considering the candidate 246699_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246699_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:50:06.88 +01:00:26.4: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:50:06.88 +01:00:26.4: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.05
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Considering the candidate 246700_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246700_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:43:14.22 +00:53:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 4.632 3125791126885006976 100.80966884910 +00.88622772154 13.8705 13.4089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246704_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246704_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:46:00.55 +01:38:15.6: 13.17 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:46:00.55 +01:38:15.6: 13.64 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.05
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Considering the candidate 246707_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246707_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246711_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246711_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:09:47.06 -02:45:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 0.249 3108346726378018688 107.44601518342 -02.75837405372 13.6228 12.8091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246712_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246712_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246719_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246719_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:10:19.17 +00:56:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.072 3114406684711231488 107.57909466657 +00.93929319959 13.4578 12.4673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246721_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246721_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:02:53.25 +01:00:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.834 3114595697632768640 105.72191786647 +01.00240844232 13.9258 13.5892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246724_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246724_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:06:09.35 +01:04:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.794 3114562437406316800 106.53856654254 +01.06758091161 13.6554 13.1770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246727_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246727_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246731_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246731_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246733_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246733_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:43.08 -04:53:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 3.626 3102071607357522688 102.92917658583 -04.88487085681 13.7782 13.2112 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 246734_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246734_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:51:54.91 -01:10:35.1: 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 06:51:54.91 -01:10:35.1: 13.52 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.05
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Considering the candidate 246735_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246735_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:42:30.45 +00:58:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.625 3125806726206403200 100.62650063837 +00.96875962341 13.6495 13.0741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246737_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246737_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:03:13.61 +00:35:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 3.253 3113028202068372608 105.80657819021 +00.59368913725 13.4034 12.5609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246738_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246738_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:43:06.91 -04:32:46.1: 12.82 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:06.91 -04:32:46.1: 14.76 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.06
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Considering the candidate 246740_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246740_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:57.99 +00:08:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 4.039 3113355826474361088 102.99123640799 +00.14000315365 13.4062 12.5154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246741_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246741_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246742_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246742_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:42:59.39 -00:24:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.869 3119455401588618496 100.74732956184 -00.41078656802 13.8492 13.2626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246743_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246743_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:00:09.61 -00:53:35.2: 12.11 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:00:09.61 -00:53:35.2: 15.60 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.11 +/- 0.03
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Considering the candidate 246746_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246746_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246749_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246749_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:09:13.80 +01:24:59.0: 13.10 +/- 0.09 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:09:13.80 +01:24:59.0: 15.46 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.10 +/- 0.09
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Considering the candidate 246751_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246751_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:53:41.55 -01:02:04.9: 14.27 +/- 0.20 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:41.55 -01:02:04.9: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.04
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Considering the candidate 246752_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246752_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:55:51.86 -00:57:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.159 3112427873020082304 103.96604863601 -00.96298805966 13.6983 12.9359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246753_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246753_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246754_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246754_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:00:47.34 -03:03:14.2: 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 07:00:47.34 -03:03:14.2: 13.47 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.06
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Considering the candidate 246756_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246756_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:09:10.32 -05:50:43.5: 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 07:09:10.32 -05:50:43.5: 13.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.06
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Considering the candidate 246763_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246763_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:15:54.50 -00:50:17.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
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Considering the candidate 246764_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246764_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:48:27.85 -01:25:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.366 3107077408922384256 102.11572553129 -01.43270975303 13.7130 13.1484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246765_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246765_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:05:15.28 +00:02:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 2.684 3112750747182534016 106.31349513794 +00.04560779328 13.7548 12.9125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246784_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246784_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:44:16.05 +00:37:26.7: 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 06:44:16.05 +00:37:26.7: 13.59 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.07
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Considering the candidate 246787_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246787_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:55:36.18 -01:20:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.200 3112125125067207296 103.90070937037 -01.34677655805 13.6992 13.2146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246788_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246788_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246791_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246791_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:57:33.23 +00:12:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.750 3112935503794000512 104.38837249421 +00.20049091823 13.5211 12.6837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246792_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246792_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:51:10.42 +01:05:59.9: 14.41 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:10.42 +01:05:59.9: 13.48 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.06
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Considering the candidate 246793_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246793_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:41:44.17 +00:27:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.820 3119584108871539072 100.43410634763 +00.45760760434 13.7271 13.1248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246794_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246794_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:43:42.09 +00:45:00.5: 14.96 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:42.09 +00:45:00.5: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.04
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Considering the candidate 246796_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246796_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:07:40.85 +01:39:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 3.226 3114691458223357952 106.91997434472 +01.65494042696 13.5480 12.9820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246799_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246799_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:05:19.21 -01:29:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.797 3109468056438096000 106.33034015352 -01.48790042039 13.5034 12.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246800_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246800_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:06:40.12 +01:37:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.465 3114734510975681664 106.66678328984 +01.61683924863 13.6497 13.4376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246802_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246802_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:09:19.77 +00:54:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.145 3114403553674802304 107.33240204310 +00.91393234250 13.5820 13.1737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246808_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246808_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:09:22.47 +01:06:33.9: 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 07:09:22.47 +01:06:33.9: 12.91 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.91 +/- 0.04
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Considering the candidate 246809_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246809_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:04:35.51 -05:56:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246810_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246810_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:16:57.11 +00:37:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 2.599 3111516274799177600 109.23810483921 +00.62290405066 13.4683 12.7778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246815_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246815_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:59:14.41 -03:28:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 2.965 3102664553364102016 104.80958162134 -03.48026694023 13.6652 13.1213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.965#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246818_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246818_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:53:17.16 -00:29:49.0: 11.86 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:17.16 -00:29:49.0: 12.35 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
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Considering the candidate 246819_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246819_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:40:34.01 -00:46:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.121 3119345828381931392 100.14173885979 -00.77486633461 13.2605 12.4490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246820_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246820_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:55:07.23 -01:18:59.1: 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 06:55:07.23 -01:18:59.1: 15.50 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.67 +/- 0.02
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Considering the candidate 246823_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246823_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:49:52.71 +01:08:13.3: 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 06:49:52.71 +01:08:13.3: 13.21 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.05
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Considering the candidate 246826_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246826_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246829_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246829_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246830_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246830_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:14:34.16 -00:57:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 2.713 3110122021036942208 108.64177513267 -00.95995102604 13.6522 12.9041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246833_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246833_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246834_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246834_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246838_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246838_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:45:44.01 +00:37:59.4: 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 06:45:44.01 +00:37:59.4: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.05
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Considering the candidate 246841_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246841_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246842_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246842_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:55:04.31 +01:01:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.436 3113996188918170624 103.76812450097 +01.03036562985 13.3729 12.4930 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246844_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246844_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246845_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246845_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246847_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246847_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:15.06 -02:29:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.824 3105969719676192768 103.31269253401 -02.49761441291 13.6303 13.1757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246848_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246848_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246850_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246850_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:02:54.58 +01:24:51.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)
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Considering the candidate 246852_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246852_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:43:56.89 +01:29:50.8: 14.73 +/- 0.33 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:56.89 +01:29:50.8: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.04
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Considering the candidate 246854_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246854_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246857_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246857_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:42:01.62 +02:09:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.323 3126792369663064576 100.50656244946 +02.15807692781 13.5734 13.1059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246860_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246860_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246862_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246862_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:16:32.52 -01:58:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 2.307 3108310305058886144 109.13572149055 -01.98190685908 13.5243 12.9767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246866_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246866_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:47:02.05 -01:27:12.5: 12.74 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:47:02.05 -01:27:12.5: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.03
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Considering the candidate 246867_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246867_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:08:55.72 +01:02:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.593 3114453894991876608 107.23218533478 +01.04294655856 13.3769 12.8666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246869_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246869_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:13:55.83 -03:09:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246875_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246875_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246876_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246876_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:05:49.60 +01:33:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.826 3114733102226564608 106.45677691624 +01.55902096947 13.5132 13.0159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246878_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246878_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246881_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246881_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:09:20.82 +01:37:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 4.248 3114699567122221824 107.33691596801 +01.62877624939 13.3990 12.9341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246884_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246884_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:09:57.95 +00:39:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.531 3114287490778891904 107.49132137484 +00.66128257443 13.4911 13.1180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246887_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246887_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:08:43.56 +01:59:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.303 3114730628324738432 107.18117361815 +01.98960102822 13.4946 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246889_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246889_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:35:07.40 -03:03:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.138 3105134640594000512 098.78093694492 -03.05146524854 13.5639 12.6234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246890_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246890_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:11:23.88 -00:34:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.384 3110953359207885056 107.84935637987 -00.57097982644 13.4770 13.3188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246892_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246892_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:46:00.26 -00:22:08.3: 13.71 +/- 0.14 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:46:00.26 -00:22:08.3: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.04
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Considering the candidate 246893_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246893_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246894_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246894_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246901_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246901_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:46:53.59 -02:03:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.744 3106205736717357056 101.72309014252 -02.05865175173 13.5639 13.1354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246902_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246902_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246903_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246903_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:19.64 -00:56:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.186 3112396674377837312 103.08194226820 -00.93746166653 13.4631 13.0185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246904_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246904_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:22.10 -01:03:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 4.006 3112368254573440640 103.09128864892 -01.06161225827 13.5055 12.7404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.006#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246905_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246905_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:44:23.00 -00:41:22.3: 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 06:44:23.00 -00:41:22.3: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.04
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Considering the candidate 246911_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246911_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:12:31.14 -04:22:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246912_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246912_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:49:54.58 +02:12:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246913_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246913_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246918_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246918_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:40.85 -03:42:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.736 3102775191720876800 102.92016284722 -03.70592443961 13.4568 13.2110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246920_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246920_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246921_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246921_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:48:59.63 -00:19:58.5: 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 06:48:59.63 -00:19:58.5: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.03
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Considering the candidate 246923_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246923_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246926_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246926_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:14:41.93 -02:06:15.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)
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Considering the candidate 246928_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246928_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:18:24.18 +01:34:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.271 3111877395649942656 109.60074644029 +01.57417466618 13.3622 12.6617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246931_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246931_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:03:42.74 +02:18:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246932_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246932_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:08:39.12 -00:21:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.705 3109664456700761600 107.16306297148 -00.36135835888 13.1910 12.3130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246934_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246934_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246935_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246935_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:08:32.74 -00:30:37.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)
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Considering the candidate 246936_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246936_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246937_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246937_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246940_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246940_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:43:43.74 -01:42:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 3.000 3107018585049274240 100.93236374119 -01.70415877100 13.4004 12.9923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246944_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246944_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246947_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246947_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246949_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246949_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246955_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246955_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:06:30.85 -05:36:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.359 3053325446539501184 106.62885354037 -05.60713260437 13.2577 12.4661 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246956_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246956_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:06:36.89 -01:52:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 3.416 3109252930116765568 106.65344933049 -01.88299616986 13.3675 13.0803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246957_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246957_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246960_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246960_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:02:50.74 -03:46:45.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)
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Considering the candidate 246962_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246962_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:48:02.77 +01:53:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246964_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246964_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246966_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246966_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:15:10.70 -00:43:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.086 3110905697949824640 108.79509097315 -00.71880200457 13.2715 12.8363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246969_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246969_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246972_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246972_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:13:43.82 -01:35:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 1.080 3108583636772982912 108.43260527323 -01.59113247863 13.3460 13.0949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246974_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246974_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246978_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246978_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:11:01.13 -03:05:21.0: 12.93 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:11:01.13 -03:05:21.0: 15.41 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.93 +/- 0.07
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Considering the candidate 246979_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246979_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:52:51.58 -00:05:55.1: 11.81 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:51.58 -00:05:55.1: 13.07 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.02
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Considering the candidate 246983_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246983_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246986_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246986_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:02:34.61 -02:48:22.6: 12.65 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:34.61 -02:48:22.6: 15.49 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.65 +/- 0.05
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Considering the candidate 246988_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246988_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:13:32.80 +00:13:14.7: 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 07:13:32.80 +00:13:14.7: 12.82 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.03
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Considering the candidate 246989_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246989_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246990_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246990_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:58:53.91 +00:32:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 3.519 3112971822037304448 104.72483387692 +00.53662840684 13.2525 12.4300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 246991_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246991_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:37:29.62 +01:45:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246996_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246996_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246997_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246997_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246998_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 246998_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 246999_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 246999_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:59:54.47 -02:15:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.344 3108958260999173760 104.97700976779 -02.25426093610 13.3224 12.7954 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247000_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247000_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:16:07.91 -03:01:52.2: 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 07:16:07.91 -03:01:52.2: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.41 +/- 0.01
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Considering the candidate 247001_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247001_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247002_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247002_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:12:09.84 +01:52:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 2.504 3114889335955565440 108.04095643351 +01.87027812878 13.1614 12.7350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247004_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247004_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247006_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247006_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:12:01.91 -01:11:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.952 3109362980057899520 108.00777394664 -01.18852132347 13.1550 12.6082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247008_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247008_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:54:15.77 -00:38:32.0: 11.12 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:15.77 -00:38:32.0: 15.54 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.12 +/- 0.01
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Considering the candidate 247010_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247010_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:07:22.75 +00:47:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.516 3114352426386304384 106.84475170251 +00.79641349732 13.2005 12.4883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247011_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247011_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:05:01.45 +01:48:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.728 3114755436055724928 106.25598204354 +01.81022333530 13.0723 12.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247014_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247014_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247016_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247016_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:16:22.37 -05:57:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247017_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247017_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247020_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247020_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:06.23 -02:04:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.645 3106231162926784256 102.77580301690 -02.08169042820 13.3129 12.8657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247021_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247021_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:04:22.02 -05:00:14.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)
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Considering the candidate 247024_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247024_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:00:49.63 +00:12:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 3.710 3112897600704146688 105.20638841578 +00.19971839969 13.1438 12.7506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247025_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247025_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:08:01.54 -02:46:25.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)
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Considering the candidate 247026_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247026_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247027_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247027_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:58:21.74 -00:45:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.538 3112259991337990912 104.59069682268 -00.76308458794 13.0407 12.6471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247034_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247034_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:16:04.49 +00:48:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.619 3111713083082158848 109.01857918206 +00.80161741102 13.1287 12.7305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247037_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247037_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:13:09.15 +00:52:29.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)
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Considering the candidate 247039_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247039_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:17:17.42 -01:16:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.409 3110060074730787840 109.32259039609 -01.26844658731 13.1751 12.5654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247040_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247040_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247041_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247041_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:48:54.42 -05:18:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.649 3101952447785931648 102.22673217314 -05.31126321634 12.9501 12.3869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247042_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247042_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247044_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247044_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:01.21 -01:37:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 2.281 3106285382592168960 103.00494216818 -01.61926474040 13.1404 12.6260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247046_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247046_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247051_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247051_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:03:40.18 -01:07:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 3.240 3109539726551184896 105.91785337662 -01.13150935500 13.1102 12.6753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247055_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247055_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:49:38.80 +02:08:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247057_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247057_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:17:42.82 -05:39:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247058_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247058_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247059_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247059_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:48:07.15 +02:07:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247060_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247060_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247061_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247061_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247062_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247062_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247065_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247065_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:10:18.96 -01:49:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.464 3108468462929071232 107.57886303127 -01.82932746549 13.1484 12.6857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247066_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247066_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247067_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247067_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247068_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247068_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:47:37.69 -05:05:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.906 3102156162372521216 101.90732041157 -05.09306200924 12.7114 12.2280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247069_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247069_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:59:04.73 -02:54:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.901 3108892771339006976 104.76908012237 -02.90136663294 13.0312 12.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247070_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247070_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247071_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247071_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247072_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247072_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247073_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247073_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:08.21 -05:53:00.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247074_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247074_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247075_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247075_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247077_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247077_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:07:58.71 -02:58:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.149 3107963993251302912 106.99440881430 -02.97752881737 12.9544 12.4417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247078_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247078_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:02.39 +01:07:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247079_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247079_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247081_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247081_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247083_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247083_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:10:32.31 +02:01:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.830 3115091160759117056 107.63445348678 +02.02860480844 12.8638 12.0750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247084_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247084_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247086_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247086_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:06.91 -01:27:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 2.283 3112284318034616192 103.52878928410 -01.46702302221 12.8078 12.2175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247089_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247089_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:16:12.80 -04:06:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.343 3059915193379489024 109.05299124807 -04.10595624574 12.9249 12.4416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247091_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247091_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247092_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247092_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247093_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247093_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:41:51.00 -01:29:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.236 3107222578817255040 100.46257646404 -01.49991807461 13.0180 12.6381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247095_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247095_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247098_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247098_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247099_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247099_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:13.35 -00:19:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247101_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247101_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:17:38.35 +01:13:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 1.668 3111755968334593536 109.41025479268 +01.21751632338 12.8697 12.1561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247102_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247102_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:09:17.07 -00:03:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 3.507 3111226514826337920 107.32061170805 -00.05252245179 12.7735 12.4631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247103_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247103_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:09:18.43 -01:42:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 2.176 3109224617692615680 107.32664531728 -01.70983647051 12.2567 11.3087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247104_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247104_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247106_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247106_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:56:24.04 +01:22:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.899 3114102218772312704 104.10002976772 +01.37115075284 12.7076 11.9544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247107_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247107_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247108_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247108_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247109_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247109_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:57:16.21 -02:14:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 2.327 3108993548450195200 104.31719717852 -02.24007477606 12.6315 11.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247111_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247111_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:20.08 +02:12:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247113_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247113_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:34.38 -00:35:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 2.716 3112500646945331200 103.64333226518 -00.58988869865 12.8288 12.5671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247114_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247114_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:40:59.58 +00:10:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.860 3119546935930633600 100.24843993955 +00.16765835915 12.7899 12.3203 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247115_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247115_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247116_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247116_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247120_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247120_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:59:44.07 +02:12:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247121_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247121_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247122_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247122_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247125_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247125_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:05:36.71 -00:02:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 2.409 3112746280414092416 106.40317434936 -00.04677212351 11.7990 10.5944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247126_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247126_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:01:37.18 -04:14:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 3.129 3101747972982311552 105.40574746029 -04.24506783820 12.7532 12.0169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247127_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247127_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:03:49.67 +01:05:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 2.270 3114600881653061376 105.95718131582 +01.09466021958 12.6217 12.1501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247129_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247129_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:50.83 +01:53:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247131_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247131_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247132_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247132_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:17:28.42 -00:24:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247134_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247134_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:07:31.65 +00:12:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 2.256 3114246259093425152 106.88170355241 +00.21575829068 12.6479 12.2206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247135_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247135_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:06:04.90 -02:19:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 0.989 3108812472631846016 106.52019261220 -02.32731304734 12.7137 11.9922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247137_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247137_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:16:13.22 -00:00:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 2.279 3111060591651425408 109.05523221248 -00.01311527828 12.5451 12.4000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247139_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247139_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:46:32.73 -00:16:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 2.276 3113418292478710400 101.63655821592 -00.27449398241 12.6208 12.1052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247140_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247140_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:12:11.62 +00:30:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 2.464 3111363988141876864 108.04845873087 +00.50334469064 12.3696 11.7618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247141_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247141_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:59:03.20 -02:17:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 1.351 3108998320154606464 104.76311203704 -02.29796996872 12.4004 11.6148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247143_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247143_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247144_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247144_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247145_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247145_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:05:10.26 -00:00:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 3.021 3112749063552893568 106.29355861945 -00.00675260357 12.5454 11.6367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247148_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247148_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:09:21.24 +02:14:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 1.973 3115156963958576256 107.33847751877 +02.23567456553 12.4681 12.0482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247150_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247150_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 247152_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247152_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:45:25.91 -04:51:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 1.522 3102225057948914176 101.35791455966 -04.86586500739 12.0278 11.0816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247154_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247154_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:47:56.85 +01:22:25.6: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:47:56.85 +01:22:25.6: 11.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.02
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Considering the candidate 247156_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247156_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:59:16.74 +02:09:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247159_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247159_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247160_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247160_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:08:35.58 +01:46:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247168_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247168_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:57:05.67 +01:24:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 2.562 3114108059926391040 104.27346090126 +01.41316855347 12.1037 11.3783 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 247170_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247170_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247171_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247171_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247177_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247177_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:44.37 +00:30:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247179_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247179_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247180_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247180_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:03:10.60 +01:53:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247181_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247181_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247182_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247182_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247183_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247183_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247185_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247185_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:14:24.34 +01:15:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247186_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247186_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:45.41 -02:45:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 1.288 3105864510156957184 102.93913002799 -02.75923800483 11.8631 11.1761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247187_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247187_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:40:43.66 -02:23:03.0: 11.59 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:40:43.66 -02:23:03.0: 11.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.01
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Considering the candidate 247188_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247188_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247189_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247189_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:52:52.43 -02:58:21.6: 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 06:52:52.43 -02:58:21.6: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.27 +/- 0.01
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Considering the candidate 247190_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247190_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247191_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247191_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247193_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247193_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:59:07.08 -02:19:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 0.905 3108997117563765376 104.77927634851 -02.32808757244 10.6917 9.5111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247195_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247195_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:52:55.96 -03:45:08.4: 13.75 +/- 0.14 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:55.96 -03:45:08.4: 10.94 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.94 +/- 0.01
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Considering the candidate 247196_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247196_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247197_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247197_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:10:16.99 +01:29:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.96, MAG_FAINT_SEARCH_LIMIT=10.94)GAIADR2_OUTPUT=# 0.617 3114511825510240128 107.57076222618 +01.49863681537 10.7072 9.9163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247198_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247198_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:07:17.11 +01:47:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247312_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247312_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247390_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247390_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247427_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247427_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:37.23 +00:27:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247428_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247428_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:12:18.81 -05:03:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247468_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247468_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:48:15.62 +01:46:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247484_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247484_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:54:11.36 -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 06:54:11.36 -00:35:54.1: 11.13 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.13 +/- 0.01
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Considering the candidate 247555_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247555_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:35.34 -02:12:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.985 3106059119416461056 103.14724547473 -02.20513469630 12.3893 11.6338 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 247564_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247564_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:03:05.49 +01:48:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247571_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247571_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247572_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247572_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:58:46.81 -00:25:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.259 3112837956497867520 104.69451278972 -00.41944890287 12.5216 11.6631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247574_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247574_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247587_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247587_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:00:37.43 -01:51:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 3.784 3109109680066395904 105.15642782143 -01.86277396635 12.3871 11.5938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247595_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247595_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247598_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247598_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:25.48 -05:17:26.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247617_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247617_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:47:30.68 -03:11:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 1.491 3105509054361904256 101.87804397042 -03.18963463726 12.3748 12.0173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247624_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247624_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247636_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247636_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:47:44.05 +00:29:30.2: 13.59 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:47:44.05 +00:29:30.2: 12.18 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.02
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Considering the candidate 247645_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247645_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:50:25.20 +01:51:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247654_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247654_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:37:20.25 -01:34:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.726 3118893104469502592 099.33473063189 -01.57021074993 12.3993 11.5750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247663_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247663_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:39:00.26 +01:56:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247665_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247665_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:57:39.87 -05:17:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 0.958 3101213777831416960 104.41613637585 -05.29032131842 12.4704 11.6797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247666_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247666_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:48:44.90 -03:54:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.331 3105384809550346752 102.18699027417 -03.90188566934 12.6478 12.1454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247698_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247698_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:08.12 -04:35:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247709_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247709_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247717_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247717_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:49:41.89 -01:43:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 1.462 3106304276146697728 102.42464614919 -01.72289255606 12.6059 11.8271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247719_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247719_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:36:41.04 -05:13:20.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247724_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247724_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:04:32.34 +01:08:10.6: 12.07 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:04:32.34 +01:08:10.6: 15.38 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.07 +/- 0.03
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Considering the candidate 247725_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247725_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:45:27.96 +00:57:47.3: 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 06:45:27.96 +00:57:47.3: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.02
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Considering the candidate 247737_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247737_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247743_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247743_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:53:50.86 -02:31:49.8: 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 06:53:50.86 -02:31:49.8: 11.22 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.22 +/- 0.01
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Considering the candidate 247768_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247768_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247788_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247788_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:01:52.68 -01:19:03.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247794_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247794_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247818_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247818_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:50:44.39 -00:31:37.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247837_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247837_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:44:33.72 -01:39:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247845_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247845_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:08:09.37 -00:32:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.299 3109654664175447040 107.03933749885 -00.53365091178 12.7814 12.0137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.299#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247859_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247859_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:01:13.48 +02:02:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247873_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247873_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:34:16.10 -00:47:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 2.015 3119181966788483328 098.56717370501 -00.79646892197 12.8155 12.3971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247901_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247901_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247902_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247902_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247903_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247903_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:02:39.53 -04:37:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247904_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247904_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247916_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247916_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:15:27.15 -00:49:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247929_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247929_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:43:35.21 -01:19:39.8: 12.76 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:35.21 -01:19:39.8: 12.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.03
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Considering the candidate 247932_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247932_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:45:10.86 -03:57:02.1: 11.76 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:45:10.86 -03:57:02.1: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
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Considering the candidate 247939_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247939_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:48:06.52 -01:40:40.3: 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 06:48:06.52 -01:40:40.3: 12.90 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
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Considering the candidate 247943_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247943_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247945_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247945_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:41:30.12 +00:57:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 2.306 3125804325323474944 100.37578011780 +00.96206277387 13.1485 12.7058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247949_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247949_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:06:42.24 -03:09:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 2.157 3107979111536590592 106.67588059035 -03.15417042601 13.0043 12.3122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247950_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247950_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247953_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247953_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247957_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247957_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:13:04.74 -05:12:23.6: 13.09 +/- 0.09 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:13:04.74 -05:12:23.6: 15.29 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.09 +/- 0.09
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Considering the candidate 247962_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247962_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:30.05 -04:07:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247965_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247965_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:16.45 +02:11:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247970_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247970_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:47:25.86 -01:17:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.504 3107094447052075136 101.85775483899 -01.29002878528 13.2204 12.7533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247972_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247972_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:09.46 -05:52:25.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247976_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247976_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247979_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247979_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:56:27.55 +00:06:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.331 3113677261828133888 104.11429280310 +00.10422085836 13.1732 12.4789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247980_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247980_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247982_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247982_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:56:36.47 +01:00:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 2.653 3113810440173047680 104.15183892639 +01.00207826748 13.1756 12.7501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 247987_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247987_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247989_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247989_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:44:43.23 -03:43:20.3: 12.28 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:43.23 -03:43:20.3: 13.79 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.03
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Considering the candidate 247990_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247990_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 247992_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 247992_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:35:16.37 -04:45:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247993_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 247993_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248001_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248001_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248007_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248007_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:05:07.36 -04:50:54.0: 12.96 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:07.36 -04:50:54.0: 15.29 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.96 +/- 0.07
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Considering the candidate 248008_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248008_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:50:25.76 -01:02:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.464 3113118503763351424 102.60699024335 -01.04634213930 13.2485 12.7977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248015_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248015_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 248017_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248017_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:17:05.28 -05:55:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248027_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248027_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:01:32.43 -05:17:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 4.717 3101401244562695680 105.38457775638 -05.28896930257 12.4362 11.2755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248029_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248029_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:28.89 -00:00:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248039_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248039_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248040_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248040_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:00:21.37 -05:50:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 2.763 3100935640049817728 105.08895116582 -05.84376213725 12.7701 11.8846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248041_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248041_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248042_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248042_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:11:28.37 -00:19:00.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248058_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248058_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:47:23.01 -01:59:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.354 3106212776163414144 101.84609672672 -01.99519846415 13.3080 12.7592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248059_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248059_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:01:22.73 -06:08:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.531 3052874406254774656 105.34484077065 -06.13892768243 13.2836 12.7701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248060_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248060_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248061_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248061_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:37:58.49 -01:25:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248064_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248064_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:35:10.49 +00:53:59.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248065_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248065_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248068_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248068_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:08:51.18 -01:46:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.491 3109234234118285952 107.21394667394 -01.77617496224 13.0380 12.3331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248090_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248090_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:16:55.90 -05:22:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248111_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248111_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:58:39.00 -04:20:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.993 3101710349067118720 104.66302468638 -04.33867408529 13.0563 12.0264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248116_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248116_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248117_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248117_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:04:20.98 +01:30:24.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248120_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248120_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:45:04.71 -01:02:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.752 3107346681891637888 101.26967865935 -01.04031808691 13.2059 12.6723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248123_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248123_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:25.60 -05:20:07.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248125_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248125_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:43:50.43 -01:04:07.2: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:50.43 -01:04:07.2: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
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Considering the candidate 248140_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248140_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:40:17.43 -04:25:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 2.427 3103981287255761536 100.07307980311 -04.43283226625 13.2340 12.7718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248148_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248148_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:02:47.24 -04:14:50.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248150_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248150_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:43:00.68 +00:23:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.451 3119568410766803968 100.75309723994 +00.39363410704 13.2345 12.5585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248155_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248155_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:45.31 -01:43:48.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248161_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248161_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:50:45.86 +01:52:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248163_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248163_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:50:05.62 +00:15:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 3.727 3113554112226157568 102.52351755616 +00.25513630730 13.0221 12.1110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248167_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248167_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:07.41 -01:52:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248170_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248170_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248175_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248175_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:15.12 -05:59:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248178_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248178_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:33.04 +02:06:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248179_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248179_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:47:03.97 -03:46:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248183_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248183_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:47:26.21 +02:03:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.885 3126362769851744256 101.85924991798 +02.06333923017 13.2439 12.7224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248184_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248184_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:35:07.08 -01:31:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 5.277 3118812874479474048 098.77860290306 -01.52424273167 13.1457 12.5678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248192_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248192_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248194_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248194_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:47:18.75 -05:59:32.0: 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 06:47:18.75 -05:59:32.0: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.04
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Considering the candidate 248200_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248200_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:26.87 -01:48:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.410 3106273253605006720 102.86178694703 -01.81278591851 13.3935 12.6677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248212_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248212_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:59:37.40 -00:31:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 5.131 3112646160437322112 104.90516011811 -00.52192288748 13.4503 12.5426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248219_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248219_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:54:19.87 -06:13:47.1: 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 06:54:19.87 -06:13:47.1: 13.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.05
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Considering the candidate 248234_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248234_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248235_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248235_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:50:40.96 -02:43:01.8: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:50:40.96 -02:43:01.8: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.04
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Considering the candidate 248237_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248237_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:58.21 -04:52:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 4.044 3102048861211058176 103.49329046444 -04.88125653681 13.3973 12.5488 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 248239_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248239_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248248_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248248_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248250_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248250_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:39:58.66 -01:44:21.5: 14.49 +/- 0.32 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:39:58.66 -01:44:21.5: 13.23 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.05
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Considering the candidate 248252_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248252_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248256_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248256_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:43:08.69 -00:01:09.4: 10.84 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:08.69 -00:01:09.4: 13.37 +/- 0.06 detection
Forced photometry reference-image weighted average: 10.92 +/- 0.01
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Considering the candidate 248257_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248257_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248260_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248260_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248261_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248261_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:44:36.07 +01:45:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248276_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248276_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:17:13.09 -01:33:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.788 3109840442983964928 109.30494289540 -01.55141250493 13.3889 12.9959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248281_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248281_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:44:26.19 -06:06:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.632 3100303317781995776 101.10954090124 -06.10697565398 13.0595 11.9466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248287_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248287_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248288_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248288_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:45:06.04 -00:02:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 2.669 3107483330569016576 101.27521621046 -00.04654528542 13.5111 12.9685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248295_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248295_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:49:52.42 -02:39:52.6: 10.77 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:49:52.42 -02:39:52.6: 13.26 +/- 0.04 detection
Forced photometry reference-image weighted average: 10.86 +/- 0.01
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Considering the candidate 248299_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248299_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:47:04.44 +01:41:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248300_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248300_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:39:38.94 -05:24:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.518 3103600645774811648 099.91216764943 -05.40094449932 13.0651 12.2041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248310_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248310_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:52.60 -02:32:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.371 3105965046751696128 103.46898690164 -02.54235597013 13.5725 13.0352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248312_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248312_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248314_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248314_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248323_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248323_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:49:57.70 -05:31:44.8: 7.99 +/- 0.00 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:49:57.70 -05:31:44.8: 12.81 +/- 0.03 detection
Forced photometry reference-image weighted average: 7.99 +/- 0.00
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Considering the candidate 248326_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248326_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:42:03.21 -06:07:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248329_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248329_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248333_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248333_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:46:11.91 +01:50:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248350_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248350_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248359_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248359_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:49:43.82 -06:16:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248362_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248362_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248364_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248364_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:06:28.76 -05:57:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248369_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248369_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248377_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248377_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:48:48.49 +00:23:28.6: 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 06:48:48.49 +00:23:28.6: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.04
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Considering the candidate 248378_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248378_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248384_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248384_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:40:19.79 -03:22:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 4.663 3105616604643085952 100.08227451735 -03.38133788963 13.4827 13.0462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248393_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248393_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248408_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248408_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:54:44.70 +00:23:48.8: 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 06:54:44.70 +00:23:48.8: 10.91 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.91 +/- 0.01
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Considering the candidate 248411_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248411_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:55.02 -02:23:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.627 3106018510504636160 103.22925868247 -02.38539636749 13.5296 12.9702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248418_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248418_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:43:17.32 -02:45:53.4: 11.12 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:17.32 -02:45:53.4: 13.13 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.30 +/- 0.01
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Considering the candidate 248419_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248419_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248420_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248420_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248421_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248421_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:01:33.35 +02:08:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248430_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248430_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248433_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248433_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248438_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248438_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:44:46.28 -01:13:49.1: 14.18 +/- 0.19 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:46.28 -01:13:49.1: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
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Considering the candidate 248441_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248441_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248451_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248451_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:23.97 +01:48:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248454_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248454_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:49:10.42 -02:16:27.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248461_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248461_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248463_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248463_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248465_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248465_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:43:55.18 +01:18:02.6: 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 06:43:55.18 +01:18:02.6: 13.33 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.05
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Considering the candidate 248466_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248466_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248469_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248469_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:25.77 -01:06:03.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248471_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248471_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248472_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248472_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248477_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248477_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:47:37.23 +00:28:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.824 3113532877908279936 101.90503476239 +00.48169308884 13.6277 13.1530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248485_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248485_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:59.66 -02:44:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 3.672 3105945972795426816 103.49787131933 -02.73864765651 13.4074 12.4613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248488_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248488_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:43:32.24 -01:20:34.0: 9.30 +/- 0.00 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:32.24 -01:20:34.0: 13.34 +/- 0.05 detection
Forced photometry reference-image weighted average: 9.30 +/- 0.00
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Considering the candidate 248498_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248498_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248500_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248500_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:50:43.21 +01:18:04.1: 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 06:50:43.21 +01:18:04.1: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.05
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Considering the candidate 248504_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248504_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:06:39.82 -02:47:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.895 3108029448552969984 106.66546376749 -02.79246343920 13.7321 12.9686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248514_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248514_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:04:16.36 -03:15:22.8: 12.14 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:04:16.36 -03:15:22.8: 15.52 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.14 +/- 0.03
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Considering the candidate 248518_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248518_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:26.25 -02:20:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.853 3106030429041323008 102.85927994532 -02.34428815611 13.6111 12.7372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248520_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248520_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248523_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248523_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248526_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248526_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:57:10.30 +01:44:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248529_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248529_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248532_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248532_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:55:38.80 +00:54:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.791 3113803014169734272 103.91154923036 +00.89978677975 13.7118 13.1253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248544_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248544_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:48.10 +01:20:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 2.810 3114065939186146688 103.45021127452 +01.33658020400 13.6390 13.0996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248550_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248550_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248552_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248552_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:45:03.55 +00:45:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.178 3125607336645920384 101.26475451617 +00.75120147011 13.7487 13.2464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248555_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248555_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:50:38.51 +01:52:23.2: 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 06:50:38.51 +01:52:23.2: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.05
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Considering the candidate 248557_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248557_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248564_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248564_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248568_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248568_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248569_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248569_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248577_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248577_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 07:02:55.16 -00:14:54.0: 10.98 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:55.16 -00:14:54.0: 15.63 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 10.98 +/- 0.01
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Considering the candidate 248580_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248580_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248582_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248582_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:39:24.85 +00:07:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.687 3119729764098083584 099.85426175068 +00.11897430785 13.7172 12.9279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248584_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248584_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:47:28.44 -01:17:33.0: 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 06:47:28.44 -01:17:33.0: 13.40 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.05
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Considering the candidate 248585_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248585_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248589_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248589_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:56:40.61 -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 06:56:40.61 -02:50:20.5: 9.99 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.99 +/- 0.00
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Considering the candidate 248610_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248610_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:14:25.68 -04:29:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248626_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248626_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:49:25.37 -02:53:37.5: 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 06:49:25.37 -02:53:37.5: 13.10 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.04
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Considering the candidate 248633_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248633_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:26.45 +00:47:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.662 3113601086287321216 103.11008331811 +00.78771273287 13.7467 13.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248637_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248637_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:57:09.46 -01:07:38.6: 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 06:57:09.46 -01:07:38.6: 11.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.01
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Considering the candidate 248639_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248639_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:49:56.13 -02:40:54.1: 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 06:49:56.13 -02:40:54.1: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.03
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Considering the candidate 248642_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248642_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248648_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248648_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:45:54.86 +00:45:35.3: 13.48 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:45:54.86 +00:45:35.3: 13.63 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.05
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Considering the candidate 248655_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248655_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:44:56.70 +01:18:46.8: 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 06:44:56.70 +01:18:46.8: 13.04 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.04
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Considering the candidate 248660_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248660_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:42:29.68 -04:08:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.836 3105326264854304256 100.62362023901 -04.13992208149 13.6824 12.7988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248670_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248670_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:49:53.45 +01:00:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.406 3113667160062874624 102.47290955156 +01.00760342702 13.7268 13.1981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248675_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248675_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248682_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248682_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:50:06.69 -00:14:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 3.064 3113243568910176640 102.52787935957 -00.24543432310 13.7853 13.1600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248692_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248692_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:48:00.02 +00:36:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.213 3113629364350926080 102.00032003377 +00.61505611669 13.5982 13.0037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248699_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248699_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:41:47.01 -00:16:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.490 3119468149051361920 100.44582555146 -00.27157940447 13.7130 13.3699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248700_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248700_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:35:18.05 -03:54:03.9: 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 06:35:18.05 -03:54:03.9: 13.64 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.06
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Considering the candidate 248701_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248701_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248703_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248703_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248712_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248712_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:55:16.95 -00:23:20.2: 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 06:55:16.95 -00:23:20.2: 13.44 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.05
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Considering the candidate 248715_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248715_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:45:27.34 -03:40:33.1: 12.78 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:45:27.34 -03:40:33.1: 14.30 +/- 0.12 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.05
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Considering the candidate 248741_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248741_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248744_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248744_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:34:24.41 +00:41:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.547 3120492687727587328 098.60232194656 +00.69514795680 13.8556 13.2614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248749_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248749_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:42.13 +00:25:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248750_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248750_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:41:49.56 +01:29:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.111 3125906614263961216 100.45621341687 +01.49890678620 13.7451 13.1793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248758_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248758_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:58:12.69 +00:18:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 3.420 3112960311525033472 104.55217649698 +00.31416181811 13.5417 12.4430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248765_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248765_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:39:27.67 +00:01:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.138 3119728041811538432 099.86531208765 +00.02823966872 13.6764 12.8084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248774_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248774_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:58:44.18 +01:49:39.1: 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 06:58:44.18 +01:49:39.1: 11.98 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.98 +/- 0.01
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Considering the candidate 248778_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248778_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:39:23.31 -02:11:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.852 3106786862973868672 099.84737561734 -02.19954032355 13.8568 13.1770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248785_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248785_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:05:23.37 -01:12:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.929 3109509013245659392 106.34752805624 -01.20582695463 13.7346 13.2486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248790_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248790_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:47:28.73 -01:01:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.771 3107173165213600896 101.86916799478 -01.02454829849 12.9061 10.7625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248792_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248792_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:37:13.46 -01:07:55.7: 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 06:37:13.46 -01:07:55.7: 13.50 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.05
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Considering the candidate 248815_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248815_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:42:11.42 -01:15:35.2: 10.99 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:42:11.42 -01:15:35.2: 13.91 +/- 0.08 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.01
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Considering the candidate 248831_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248831_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248839_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248839_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:28.93 +00:03:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.922 3113359979703523456 103.37015109381 +00.06206638468 14.0352 13.4798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248841_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248841_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248843_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248843_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:35:07.76 -01:47:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 2.008 3118798443389486592 098.78210684817 -01.78578744001 13.3480 12.4328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248855_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248855_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:56.48 -04:43:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.286 3102055458280756864 103.48505444976 -04.73232095785 14.0018 13.4206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248877_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248877_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:59.73 +00:10:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.797 3113319370792412800 103.74872486234 +00.18032112282 13.8383 13.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248881_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248881_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:10:24.65 +02:20:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.759 3115118343612453632 107.60230636112 +02.33784729094 13.8710 13.1518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248899_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248899_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:54:59.46 -01:03:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.570 3112333791758054272 103.74773607348 -01.05207476769 13.3921 12.4083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248902_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248902_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:53:04.98 +00:10:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.737 3113365687719085440 103.27079700425 +00.17690733783 13.8514 13.0052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248904_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248904_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248908_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248908_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248917_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248917_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248926_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248926_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248929_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248929_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248935_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248935_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248936_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248936_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248948_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248948_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:45:53.57 -00:10:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.542 3113470587999887744 101.47333523738 -00.17608354364 13.8713 12.8040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248961_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 248961_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 248963_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248963_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:46:37.79 -02:06:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 2.839 3106205049522620672 101.65723942165 -02.10495206113 14.0430 13.4886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248964_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248964_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:48:46.48 -02:23:34.2: 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 06:48:46.48 -02:23:34.2: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.06
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Considering the candidate 248974_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248974_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:50:36.14 -05:34:29.6: 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 06:50:36.14 -05:34:29.6: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.02
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Considering the candidate 248986_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248986_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:13:56.26 -02:08:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248999_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 248999_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:40:24.80 -03:51:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 5.576 3104083610556005760 100.10388378574 -03.85567044820 13.6866 12.6817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249014_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249014_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:12:32.25 -01:10:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.328 3109361094573771776 108.13450362302 -01.17491163022 13.8219 13.5006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249017_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 249017_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 249018_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249018_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 07:03:33.19 -02:48:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.411 3108675342915385344 105.88815276368 -02.81463402636 14.1979 13.8038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249020_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 249020_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 249042_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249042_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:51:01.64 -02:13:05.0: 11.37 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:01.64 -02:13:05.0: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.63 +/- 0.01
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Considering the candidate 249049_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249049_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:52:59.01 +00:32:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.604 3113580431783529216 103.24582706418 +00.53999990457 14.1457 13.7959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249058_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249058_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:44:24.84 -00:04:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.530 3119491273155424256 101.10363098451 -00.08086075308 14.0849 13.5434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249059_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249059_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:47:04.43 -03:10:25.4: 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 06:47:04.43 -03:10:25.4: 13.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.59 +/- 0.05
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Considering the candidate 249085_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249085_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:47.66 +00:30:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.132 3113578408860276992 102.94837614475 +00.50448231975 13.7897 12.9917 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249096_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249096_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:50:37.02 -01:46:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.036 3106322662908980736 102.65406281871 -01.78241089868 14.1429 13.7557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249114_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249114_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 249115_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249115_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:57:14.49 -02:23:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.440 3108982518975009536 104.31020165281 -02.39396072309 14.1972 13.2434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249117_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249117_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:56:56.05 -00:51:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 4.200 3112425261679814400 104.23338714528 -00.86054530195 14.3594 13.4729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249127_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249127_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:53:47.24 -02:38:42.7: 14.66 +/- 0.27 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:47.24 -02:38:42.7: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
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Considering the candidate 249129_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 249129_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 249145_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249145_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 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 06:51:48.38 -01:05:38.9: 13.66 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q2b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:48.38 -01:05:38.9: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.02
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Considering the candidate 249176_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 249176_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 249178_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 249178_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
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Considering the candidate 249180_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249180_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:38:12.85 -02:02:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.828 3106804077202849280 099.55361231780 -02.04769906103 14.3130 13.6943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249181_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249181_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:49:43.49 +00:02:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.147 3113446398744161664 102.43094111013 +00.04499060411 14.3513 13.5608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249194_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249194_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:51:34.99 -02:45:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.272 3105910036811446656 102.89546607578 -02.75540196241 14.3462 13.9020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249196_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
The candidate 249196_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025 did not pass the final checks
**** FOUND 06:47:18.91 +01:54:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249197_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 249197_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249203_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 249203_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 249217_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 249217_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129332_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
Preparing report for the candidate 129332_fd_Mon-02-Q2b1x1_2026-04-24_21-37-35_20.00sec_-4.90C_LIGHT_0025
make_report_in_HTML.sh Phase 2 (HTML assembly): 17s
make_report_in_HTML.sh TOTAL: 560s
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 ####
07:12:49.82 -03:03:25.7
06:51:13.30 -01:21:59.2
06:50:58.14 -02:14:41.0
06:52:23.48 -02:34:55.9
06:53:25.72 -04:34:19.7
06:53:30.53 -03:06:06.5
06:50:18.43 -04:39:46.6
06:49:36.09 -00:19:57.1
06:50:57.40 -01:59:58.4
07:00:40.18 -02:26:31.6
06:54:46.06 -00:27:03.5
06:59:01.82 -03:10:13.1
06:52:03.56 -00:56:53.2
07:07:54.99 -05:37:21.2
06:53:29.91 -01:56:22.6
07:06:01.56 -02:28:21.7
06:59:56.95 +01:13:10.5
07:19:13.98 -05:31:01.9
06:57:16.36 -02:12:54.6
07:00:14.73 -00:57:25.5
07:02:32.32 -00:13:10.6
07:06:24.61 -00:09:13.5
06:50:56.01 -02:40:07.2
06:53:34.00 -00:32:05.2
07:01:52.57 -01:40:51.6
06:53:52.20 -02:12:22.9
07:17:56.41 -02:49:58.3
06:46:36.45 -03:38:14.6
06:59:32.97 -01:48:18.9
06:43:45.56 +00:35:14.9
06:44:01.87 -04:32:27.5
07:16:07.40 +01:27:14.8
06:57:49.50 -00:05:50.6
07:02:32.22 +00:30:19.8
07:03:25.24 -00:05:26.4
07:05:55.55 -03:57:45.4
07:12:16.06 -03:44:42.7
06:55:03.17 -01:02:50.6
07:04:57.17 -01:40:50.3
07:07:02.21 -01:54:20.2
07:13:23.19 +01:43:05.5
06:57:33.41 -03:31:48.4
07:14:02.03 -01:05:48.1
07:01:50.71 +01:44:17.8
06:55:47.99 +01:18:47.2
06:51:34.68 -01:53:51.6
06:51:17.40 -02:53:49.8
06:57:55.19 -04:37:48.5
07:19:03.35 -04:45:19.8
06:53:42.56 -01:01:10.3
06:59:38.56 -06:13:04.0
07:04:17.38 +01:02:40.1
07:18:49.57 -01:01:56.9
07:09:59.74 +01:25:46.8
07:17:43.83 -04:05:30.0
07:10:30.43 -02:58:56.4
07:09:05.32 -01:22:05.7
07:04:36.92 +00:42:05.6
06:51:46.19 -05:25:56.1
07:08:02.81 -03:23:35.8
07:05:38.79 -00:02:18.3
07:10:55.70 -00:46:12.4
07:01:07.30 +00:37:52.7
07:02:34.25 -04:55:48.5
07:02:01.73 +00:22:42.0
07:14:41.20 -00:43:06.9
07:08:29.18 -00:58:27.7
07:15:26.79 -03:19:53.3
06:52:53.59 +01:22:23.6
07:07:20.90 -03:23:28.5
07:16:33.73 -05:05:45.9
07:03:06.80 -04:06:44.4
07:03:22.27 -04:53:37.4
07:18:22.34 +00:01:08.7
06:57:47.57 +00:12:34.3
07:10:16.97 -04:37:52.6
07:03:26.98 -05:01:12.3
06:59:30.36 +00:22:07.0
06:50:59.53 -02:47:53.0
06:57:31.08 +00:41:49.0
07:13:10.29 -05:21:11.2
07:00:35.32 -02:31:06.9
07:13:11.72 +01:02:12.9
07:17:13.03 -00:34:59.2
06:58:50.25 -01:53:11.2
07:05:00.04 +01:38:42.5
07:08:41.86 +01:18:47.7
06:55:20.59 +00:53:19.7
06:59:09.54 +00:41:52.9
07:12:26.22 +01:50:34.1
07:03:14.42 +01:07:06.3
07:15:49.73 -00:37:01.5
07:18:17.99 -00:24:26.0
06:58:09.65 +00:53:07.1
07:18:04.95 -01:25:37.0
07:10:41.27 -05:05:04.7
07:00:12.55 +00:10:02.4
07:01:00.95 -00:25:44.2
06:59:40.22 -00:40:25.3
07:05:50.93 -02:05:13.9
07:12:11.75 -01:59:49.6
07:05:08.36 -04:26:25.2
06:59:25.58 -01:04:49.6
07:02:21.41 -04:03:30.8
07:07:15.17 -04:18:17.6
07:10:02.16 -03:03:52.9
07:17:01.01 -00:19:59.4
07:03:52.74 +00:49:48.2
07:02:00.71 +01:40:09.6
07:04:20.84 -04:41:01.3
07:09:39.86 -05:35:35.0
07:11:00.52 -02:53:38.9
06:58:03.49 -05:54:02.5
07:08:43.92 -03:56:10.9
07:02:47.42 -03:11:46.8
07:12:39.25 -02:45:30.3
06:54:05.71 -03:49:50.5
07:14:38.80 -03:56:24.7
07:03:55.55 -04:49:26.2
07:17:51.17 -01:41:37.6
07:03:02.18 +01:23:58.0
06:53:07.39 -01:35:07.7
06:58:08.39 -01:38:52.7
07:05:24.98 -00:59:48.6
07:05:30.61 +01:36:36.6
07:08:30.45 -01:56:44.1
07:01:24.07 +01:06:07.7
07:06:24.10 +00:20:28.4
07:13:48.27 -00:49:58.0
06:56:12.23 +00:18:26.3
07:14:57.39 -05:11:43.0
06:54:57.30 -01:11:47.8
07:05:49.13 +01:38:16.9
06:59:50.16 +00:16:20.9
06:52:46.10 -01:34:15.7
06:51:14.95 -04:32:31.6
06:52:07.76 +00:28:19.8
07:07:11.39 -02:58:18.8
07:04:44.65 -03:46:31.1
06:57:00.74 +00:17:38.0
06:58:26.68 -00:54:20.5
07:10:29.63 -04:23:43.2
06:53:05.71 +00:29:07.9
06:51:43.68 -00:26:00.9
07:16:22.46 -02:57:52.8
06:52:57.37 -03:04:55.0
07:04:20.49 -00:08:22.7
07:01:46.09 +01:19:50.1
06:39:36.65 -04:34:34.5
06:57:11.88 -03:58:11.5
07:08:12.41 -03:12:25.9
07:02:02.02 +00:07:46.9
06:54:48.32 +00:23:19.3
06:59:40.39 -00:39:47.1
07:13:15.22 -00:27:59.6
07:06:31.76 -04:48:14.7
07:08:43.17 -05:05:29.3
06:49:46.85 -03:36:01.0
06:50:50.97 -02:36:25.9
07:10:18.85 -06:07:57.8
07:03:11.83 +01:45:15.4
07:01:59.85 -02:00:41.8
07:17:27.88 +00:52:46.6
06:54:07.36 -03:06:07.8
07:00:27.47 -00:07:02.7
07:04:33.60 -04:28:40.3
07:06:45.54 -01:30:49.7
06:54:15.22 -02:04:22.9
06:59:35.88 -05:28:09.7
07:12:56.91 +00:52:07.2
07:01:00.36 -00:27:54.0
06:44:39.52 +00:10:06.0
07:01:49.00 -03:26:19.2
06:50:00.14 -03:51:11.7
06:55:10.24 -02:56:00.4
06:56:49.12 +00:46:33.2
06:46:16.99 -05:17:46.5
06:58:24.59 -03:02:34.6
06:59:34.21 -02:33:57.8
06:52:51.61 -02:22:45.2
07:05:41.67 -01:29:58.7
06:51:08.17 -02:08:43.6
07:04:26.89 +00:59:22.0
06:54:00.04 -05:06:47.0
06:55:24.68 -00:53:53.6
06:57:24.07 -02:57:03.4
06:48:45.19 +01:09:19.8
07:00:54.96 -03:04:10.3
06:56:39.00 -01:28:50.8
07:05:06.30 -04:50:35.6
06:54:55.00 -01:21:36.2
07:06:11.11 -02:50:59.9
06:40:24.07 -03:51:05.6
07:09:21.54 +01:07:27.5
06:59:49.61 -06:00:34.9
06:51:34.23 -01:39:22.5
07:11:26.80 -03:39:48.3
06:51:37.36 +01:29:00.1
07:07:34.13 -03:14:12.8
06:44:56.87 +00:56:56.5
06:47:59.48 -01:20:54.9
06:57:44.45 -03:47:48.0
06:54:22.77 -02:36:36.8
06:51:16.10 -00:44:17.2
06:52:15.35 -01:03:58.8
06:57:50.56 -00:57:55.8
06:46:21.66 -00:23:11.6
06:47:48.31 -01:09:01.5
########### 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 ####
06:51:13.30 -01:21:59.2
06:50:58.14 -02:14:41.0
06:52:23.48 -02:34:55.9
06:53:25.72 -04:34:19.7
06:53:30.53 -03:06:06.5
06:50:18.43 -04:39:46.6
06:49:36.09 -00:19:57.1
06:50:57.40 -01:59:58.4
07:00:40.18 -02:26:31.6
06:54:46.06 -00:27:03.5
06:59:01.82 -03:10:13.1
06:52:03.56 -00:56:53.2
07:07:54.99 -05:37:21.2
06:53:29.91 -01:56:22.6
07:06:01.56 -02:28:21.7
06:59:56.95 +01:13:10.5
07:19:13.98 -05:31:01.9
06:57:16.36 -02:12:54.6
07:00:14.73 -00:57:25.5
07:02:32.32 -00:13:10.6
07:06:24.61 -00:09:13.5
06:50:56.01 -02:40:07.2
06:53:34.00 -00:32:05.2
07:01:52.57 -01:40:51.6
06:53:52.20 -02:12:22.9
07:17:56.41 -02:49:58.3
06:46:36.45 -03:38:14.6
06:59:32.97 -01:48:18.9
06:43:45.56 +00:35:14.9
06:44:01.87 -04:32:27.5
07:16:07.40 +01:27:14.8
06:57:49.50 -00:05:50.6
07:02:32.22 +00:30:19.8
07:03:25.24 -00:05:26.4
07:05:55.55 -03:57:45.4
07:12:16.06 -03:44:42.7
06:55:03.17 -01:02:50.6
07:04:57.17 -01:40:50.3
07:07:02.21 -01:54:20.2
07:13:23.19 +01:43:05.5
06:57:33.41 -03:31:48.4
07:14:02.03 -01:05:48.1
07:01:50.71 +01:44:17.8
06:55:47.99 +01:18:47.2
06:51:34.68 -01:53:51.6
06:51:17.40 -02:53:49.8
06:57:55.19 -04:37:48.5
07:19:03.35 -04:45:19.8
06:53:42.56 -01:01:10.3
06:59:38.56 -06:13:04.0
07:04:17.38 +01:02:40.1
07:18:49.57 -01:01:56.9
07:09:59.74 +01:25:46.8
07:17:43.83 -04:05:30.0
07:10:30.43 -02:58:56.4
07:09:05.32 -01:22:05.7
07:04:36.92 +00:42:05.6
06:51:46.19 -05:25:56.1
07:08:02.81 -03:23:35.8
07:05:38.79 -00:02:18.3
07:10:55.70 -00:46:12.4
07:01:07.30 +00:37:52.7
07:02:34.25 -04:55:48.5
07:02:01.73 +00:22:42.0
07:14:41.20 -00:43:06.9
07:08:29.18 -00:58:27.7
07:15:26.79 -03:19:53.3
06:52:53.59 +01:22:23.6
07:07:20.90 -03:23:28.5
07:16:33.73 -05:05:45.9
07:03:06.80 -04:06:44.4
07:03:22.27 -04:53:37.4
07:18:22.34 +00:01:08.7
06:57:47.57 +00:12:34.3
07:10:16.97 -04:37:52.6
07:03:26.98 -05:01:12.3
06:59:30.36 +00:22:07.0
06:50:59.53 -02:47:53.0
06:57:31.08 +00:41:49.0
07:13:10.29 -05:21:11.2
07:00:35.32 -02:31:06.9
07:13:11.72 +01:02:12.9
07:17:13.03 -00:34:59.2
06:58:50.25 -01:53:11.2
07:05:00.04 +01:38:42.5
07:08:41.86 +01:18:47.7
06:55:20.59 +00:53:19.7
06:59:09.54 +00:41:52.9
07:12:26.22 +01:50:34.1
07:03:14.42 +01:07:06.3
07:15:49.73 -00:37:01.5
07:18:17.99 -00:24:26.0
06:58:09.65 +00:53:07.1
07:18:04.95 -01:25:37.0
07:10:41.27 -05:05:04.7
07:00:12.55 +00:10:02.4
07:01:00.95 -00:25:44.2
06:59:40.22 -00:40:25.3
07:05:50.93 -02:05:13.9
07:12:11.75 -01:59:49.6
07:05:08.36 -04:26:25.2
06:59:25.58 -01:04:49.6
07:02:21.41 -04:03:30.8
07:07:15.17 -04:18:17.6
07:10:02.16 -03:03:52.9
07:17:01.01 -00:19:59.4
07:03:52.74 +00:49:48.2
07:02:00.71 +01:40:09.6
07:04:20.84 -04:41:01.3
07:09:39.86 -05:35:35.0
07:11:00.52 -02:53:38.9
06:58:03.49 -05:54:02.5
07:08:43.92 -03:56:10.9
07:02:47.42 -03:11:46.8
07:12:39.25 -02:45:30.3
06:54:05.71 -03:49:50.5
07:14:38.80 -03:56:24.7
07:03:55.55 -04:49:26.2
07:17:51.17 -01:41:37.6
07:03:02.18 +01:23:58.0
06:53:07.39 -01:35:07.7
06:58:08.39 -01:38:52.7
07:05:24.98 -00:59:48.6
07:05:30.61 +01:36:36.6
07:08:30.45 -01:56:44.1
07:01:24.07 +01:06:07.7
07:06:24.10 +00:20:28.4
07:13:48.27 -00:49:58.0
06:56:12.23 +00:18:26.3
07:14:57.39 -05:11:43.0
06:54:57.30 -01:11:47.8
07:05:49.13 +01:38:16.9
06:59:50.16 +00:16:20.9
06:52:46.10 -01:34:15.7
06:51:14.95 -04:32:31.6
06:52:07.76 +00:28:19.8
07:07:11.39 -02:58:18.8
07:04:44.65 -03:46:31.1
06:57:00.74 +00:17:38.0
06:58:26.68 -00:54:20.5
07:10:29.63 -04:23:43.2
06:53:05.71 +00:29:07.9
06:51:43.68 -00:26:00.9
07:16:22.46 -02:57:52.8
06:52:57.37 -03:04:55.0
07:04:20.49 -00:08:22.7
07:01:46.09 +01:19:50.1
06:39:36.65 -04:34:34.5
06:57:11.88 -03:58:11.5
07:08:12.41 -03:12:25.9
07:02:02.02 +00:07:46.9
06:54:48.32 +00:23:19.3
06:59:40.39 -00:39:47.1
07:13:15.22 -00:27:59.6
07:06:31.76 -04:48:14.7
07:08:43.17 -05:05:29.3
06:49:46.85 -03:36:01.0
06:50:50.97 -02:36:25.9
07:10:18.85 -06:07:57.8
07:03:11.83 +01:45:15.4
07:01:59.85 -02:00:41.8
07:17:27.88 +00:52:46.6
06:54:07.36 -03:06:07.8
07:00:27.47 -00:07:02.7
07:04:33.60 -04:28:40.3
07:06:45.54 -01:30:49.7
06:54:15.22 -02:04:22.9
06:59:35.88 -05:28:09.7
07:12:56.91 +00:52:07.2
07:01:00.36 -00:27:54.0
06:44:39.52 +00:10:06.0
07:01:49.00 -03:26:19.2
06:50:00.14 -03:51:11.7
06:55:10.24 -02:56:00.4
06:56:49.12 +00:46:33.2
06:46:16.99 -05:17:46.5
06:58:24.59 -03:02:34.6
06:59:34.21 -02:33:57.8
06:52:51.61 -02:22:45.2
07:05:41.67 -01:29:58.7
06:51:08.17 -02:08:43.6
07:04:26.89 +00:59:22.0
06:54:00.04 -05:06:47.0
06:55:24.68 -00:53:53.6
06:57:24.07 -02:57:03.4
06:48:45.19 +01:09:19.8
07:00:54.96 -03:04:10.3
06:56:39.00 -01:28:50.8
07:05:06.30 -04:50:35.6
06:54:55.00 -01:21:36.2
07:06:11.11 -02:50:59.9
06:40:24.07 -03:51:05.6
07:09:21.54 +01:07:27.5
06:59:49.61 -06:00:34.9
06:51:34.23 -01:39:22.5
07:11:26.80 -03:39:48.3
06:51:37.36 +01:29:00.1
07:07:34.13 -03:14:12.8
06:44:56.87 +00:56:56.5
06:47:59.48 -01:20:54.9
06:57:44.45 -03:47:48.0
06:54:22.77 -02:36:36.8
06:51:16.10 -00:44:17.2
06:52:15.35 -01:03:58.8
06:57:50.56 -00:57:55.8
06:46:21.66 -00:23:11.6
06:47:48.31 -01:09:01.5
07:12:49.82 -03:03:25.7
###################################################################################
06:51:13.30 -01:21:59.2 -- not an asteroid (will add it to exclusion list)
06:50:58.14 -02:14:41.0 -- not an asteroid (will add it to exclusion list)
06:52:23.48 -02:34:55.9 -- not an asteroid (will add it to exclusion list)
06:53:25.72 -04:34:19.7 -- not an asteroid (will add it to exclusion list)
06:53:30.53 -03:06:06.5 -- not an asteroid (will add it to exclusion list)
06:50:18.43 -04:39:46.6 -- not an asteroid (will add it to exclusion list)
06:49:36.09 -00:19:57.1 -- not an asteroid (will add it to exclusion list)
06:50:57.40 -01:59:58.4 -- not an asteroid (will add it to exclusion list)
07:00:40.18 -02:26:31.6 -- not an asteroid (will add it to exclusion list)
06:54:46.06 -00:27:03.5 -- not an asteroid (will add it to exclusion list)
06:59:01.82 -03:10:13.1 -- not an asteroid (will add it to exclusion list)
06:52:03.56 -00:56:53.2 -- not an asteroid (will add it to exclusion list)
07:07:54.99 -05:37:21.2 -- not an asteroid (will add it to exclusion list)
06:53:29.91 -01:56:22.6 -- not an asteroid (will add it to exclusion list)
07:06:01.56 -02:28:21.7 -- not an asteroid (will add it to exclusion list)
06:59:56.95 +01:13:10.5 -- not an asteroid (will add it to exclusion list)
07:19:13.98 -05:31:01.9 -- not an asteroid (will add it to exclusion list)
06:57:16.36 -02:12:54.6 -- not an asteroid (will add it to exclusion list)
07:00:14.73 -00:57:25.5 -- not an asteroid (will add it to exclusion list)
07:02:32.32 -00:13:10.6 -- not an asteroid (will add it to exclusion list)
07:06:24.61 -00:09:13.5 -- not an asteroid (will add it to exclusion list)
06:50:56.01 -02:40:07.2 -- not an asteroid (will add it to exclusion list)
06:53:34.00 -00:32:05.2 -- not an asteroid (will add it to exclusion list)
07:01:52.57 -01:40:51.6 -- not an asteroid (will add it to exclusion list)
06:53:52.20 -02:12:22.9 -- not an asteroid (will add it to exclusion list)
07:17:56.41 -02:49:58.3 -- not an asteroid (will add it to exclusion list)
06:46:36.45 -03:38:14.6 -- not an asteroid (will add it to exclusion list)
06:59:32.97 -01:48:18.9 -- not an asteroid (will add it to exclusion list)
06:43:45.56 +00:35:14.9 -- not an asteroid (will add it to exclusion list)
06:44:01.87 -04:32:27.5 -- not an asteroid (will add it to exclusion list)
07:16:07.40 +01:27:14.8 -- not an asteroid (will add it to exclusion list)
06:57:49.50 -00:05:50.6 -- not an asteroid (will add it to exclusion list)
07:02:32.22 +00:30:19.8 -- not an asteroid (will add it to exclusion list)
07:03:25.24 -00:05:26.4 -- not an asteroid (will add it to exclusion list)
07:05:55.55 -03:57:45.4 -- not an asteroid (will add it to exclusion list)
07:12:16.06 -03:44:42.7 -- not an asteroid (will add it to exclusion list)
06:55:03.17 -01:02:50.6 -- not an asteroid (will add it to exclusion list)
07:04:57.17 -01:40:50.3 -- not an asteroid (will add it to exclusion list)
07:07:02.21 -01:54:20.2 -- not an asteroid (will add it to exclusion list)
07:13:23.19 +01:43:05.5 -- not an asteroid (will add it to exclusion list)
06:57:33.41 -03:31:48.4 -- not an asteroid (will add it to exclusion list)
07:14:02.03 -01:05:48.1 -- not an asteroid (will add it to exclusion list)
07:01:50.71 +01:44:17.8 -- not an asteroid (will add it to exclusion list)
06:55:47.99 +01:18:47.2 -- not an asteroid (will add it to exclusion list)
06:51:34.68 -01:53:51.6 -- not an asteroid (will add it to exclusion list)
06:51:17.40 -02:53:49.8 -- not an asteroid (will add it to exclusion list)
06:57:55.19 -04:37:48.5 -- not an asteroid (will add it to exclusion list)
07:19:03.35 -04:45:19.8 -- not an asteroid (will add it to exclusion list)
06:53:42.56 -01:01:10.3 -- not an asteroid (will add it to exclusion list)
06:59:38.56 -06:13:04.0 -- not an asteroid (will add it to exclusion list)
07:04:17.38 +01:02:40.1 -- not an asteroid (will add it to exclusion list)
07:18:49.57 -01:01:56.9 -- not an asteroid (will add it to exclusion list)
07:09:59.74 +01:25:46.8 -- not an asteroid (will add it to exclusion list)
07:17:43.83 -04:05:30.0 -- not an asteroid (will add it to exclusion list)
07:10:30.43 -02:58:56.4 -- not an asteroid (will add it to exclusion list)
07:09:05.32 -01:22:05.7 -- not an asteroid (will add it to exclusion list)
07:04:36.92 +00:42:05.6 -- not an asteroid (will add it to exclusion list)
06:51:46.19 -05:25:56.1 -- not an asteroid (will add it to exclusion list)
07:08:02.81 -03:23:35.8 -- not an asteroid (will add it to exclusion list)
07:05:38.79 -00:02:18.3 -- not an asteroid (will add it to exclusion list)
07:10:55.70 -00:46:12.4 -- not an asteroid (will add it to exclusion list)
07:01:07.30 +00:37:52.7 -- not an asteroid (will add it to exclusion list)
07:02:34.25 -04:55:48.5 -- not an asteroid (will add it to exclusion list)
07:02:01.73 +00:22:42.0 -- not an asteroid (will add it to exclusion list)
07:14:41.20 -00:43:06.9 -- not an asteroid (will add it to exclusion list)
07:08:29.18 -00:58:27.7 -- not an asteroid (will add it to exclusion list)
07:15:26.79 -03:19:53.3 -- not an asteroid (will add it to exclusion list)
06:52:53.59 +01:22:23.6 -- not an asteroid (will add it to exclusion list)
07:07:20.90 -03:23:28.5 -- not an asteroid (will add it to exclusion list)
07:16:33.73 -05:05:45.9 -- not an asteroid (will add it to exclusion list)
07:03:06.80 -04:06:44.4 -- not an asteroid (will add it to exclusion list)
07:03:22.27 -04:53:37.4 -- not an asteroid (will add it to exclusion list)
07:18:22.34 +00:01:08.7 -- not an asteroid (will add it to exclusion list)
06:57:47.57 +00:12:34.3 -- not an asteroid (will add it to exclusion list)
07:10:16.97 -04:37:52.6 -- not an asteroid (will add it to exclusion list)
07:03:26.98 -05:01:12.3 -- not an asteroid (will add it to exclusion list)
06:59:30.36 +00:22:07.0 -- not an asteroid (will add it to exclusion list)
06:50:59.53 -02:47:53.0 -- not an asteroid (will add it to exclusion list)
06:57:31.08 +00:41:49.0 -- not an asteroid (will add it to exclusion list)
07:13:10.29 -05:21:11.2 -- not an asteroid (will add it to exclusion list)
07:00:35.32 -02:31:06.9 -- not an asteroid (will add it to exclusion list)
07:13:11.72 +01:02:12.9 -- not an asteroid (will add it to exclusion list)
07:17:13.03 -00:34:59.2 -- not an asteroid (will add it to exclusion list)
06:58:50.25 -01:53:11.2 -- not an asteroid (will add it to exclusion list)
07:05:00.04 +01:38:42.5 -- not an asteroid (will add it to exclusion list)
07:08:41.86 +01:18:47.7 -- not an asteroid (will add it to exclusion list)
06:55:20.59 +00:53:19.7 -- not an asteroid (will add it to exclusion list)
06:59:09.54 +00:41:52.9 -- not an asteroid (will add it to exclusion list)
07:12:26.22 +01:50:34.1 -- not an asteroid (will add it to exclusion list)
07:03:14.42 +01:07:06.3 -- not an asteroid (will add it to exclusion list)
07:15:49.73 -00:37:01.5 -- not an asteroid (will add it to exclusion list)
07:18:17.99 -00:24:26.0 -- not an asteroid (will add it to exclusion list)
06:58:09.65 +00:53:07.1 -- not an asteroid (will add it to exclusion list)
07:18:04.95 -01:25:37.0 -- not an asteroid (will add it to exclusion list)
07:10:41.27 -05:05:04.7 -- not an asteroid (will add it to exclusion list)
07:00:12.55 +00:10:02.4 -- not an asteroid (will add it to exclusion list)
07:01:00.95 -00:25:44.2 -- not an asteroid (will add it to exclusion list)
06:59:40.22 -00:40:25.3 -- not an asteroid (will add it to exclusion list)
07:05:50.93 -02:05:13.9 -- not an asteroid (will add it to exclusion list)
07:12:11.75 -01:59:49.6 -- not an asteroid (will add it to exclusion list)
07:05:08.36 -04:26:25.2 -- not an asteroid (will add it to exclusion list)
06:59:25.58 -01:04:49.6 -- not an asteroid (will add it to exclusion list)
07:02:21.41 -04:03:30.8 -- not an asteroid (will add it to exclusion list)
07:07:15.17 -04:18:17.6 -- not an asteroid (will add it to exclusion list)
07:10:02.16 -03:03:52.9 -- not an asteroid (will add it to exclusion list)
07:17:01.01 -00:19:59.4 -- not an asteroid (will add it to exclusion list)
07:03:52.74 +00:49:48.2 -- not an asteroid (will add it to exclusion list)
07:02:00.71 +01:40:09.6 -- not an asteroid (will add it to exclusion list)
07:04:20.84 -04:41:01.3 -- not an asteroid (will add it to exclusion list)
07:09:39.86 -05:35:35.0 -- not an asteroid (will add it to exclusion list)
07:11:00.52 -02:53:38.9 -- not an asteroid (will add it to exclusion list)
06:58:03.49 -05:54:02.5 -- not an asteroid (will add it to exclusion list)
07:08:43.92 -03:56:10.9 -- not an asteroid (will add it to exclusion list)
07:02:47.42 -03:11:46.8 -- not an asteroid (will add it to exclusion list)
07:12:39.25 -02:45:30.3 -- not an asteroid (will add it to exclusion list)
06:54:05.71 -03:49:50.5 -- not an asteroid (will add it to exclusion list)
07:14:38.80 -03:56:24.7 -- not an asteroid (will add it to exclusion list)
07:03:55.55 -04:49:26.2 -- not an asteroid (will add it to exclusion list)
07:17:51.17 -01:41:37.6 -- not an asteroid (will add it to exclusion list)
07:03:02.18 +01:23:58.0 -- not an asteroid (will add it to exclusion list)
06:53:07.39 -01:35:07.7 -- not an asteroid (will add it to exclusion list)
06:58:08.39 -01:38:52.7 -- not an asteroid (will add it to exclusion list)
07:05:24.98 -00:59:48.6 -- not an asteroid (will add it to exclusion list)
07:05:30.61 +01:36:36.6 -- not an asteroid (will add it to exclusion list)
07:08:30.45 -01:56:44.1 -- not an asteroid (will add it to exclusion list)
07:01:24.07 +01:06:07.7 -- not an asteroid (will add it to exclusion list)
07:06:24.10 +00:20:28.4 -- not an asteroid (will add it to exclusion list)
07:13:48.27 -00:49:58.0 -- not an asteroid (will add it to exclusion list)
06:56:12.23 +00:18:26.3 -- not an asteroid (will add it to exclusion list)
07:14:57.39 -05:11:43.0 -- not an asteroid (will add it to exclusion list)
06:54:57.30 -01:11:47.8 -- not an asteroid (will add it to exclusion list)
07:05:49.13 +01:38:16.9 -- not an asteroid (will add it to exclusion list)
06:59:50.16 +00:16:20.9 -- not an asteroid (will add it to exclusion list)
06:52:46.10 -01:34:15.7 -- not an asteroid (will add it to exclusion list)
06:51:14.95 -04:32:31.6 -- not an asteroid (will add it to exclusion list)
06:52:07.76 +00:28:19.8 -- not an asteroid (will add it to exclusion list)
07:07:11.39 -02:58:18.8 -- not an asteroid (will add it to exclusion list)
07:04:44.65 -03:46:31.1 -- not an asteroid (will add it to exclusion list)
06:57:00.74 +00:17:38.0 -- not an asteroid (will add it to exclusion list)
06:58:26.68 -00:54:20.5 -- not an asteroid (will add it to exclusion list)
07:10:29.63 -04:23:43.2 -- not an asteroid (will add it to exclusion list)
06:53:05.71 +00:29:07.9 -- not an asteroid (will add it to exclusion list)
06:51:43.68 -00:26:00.9 -- not an asteroid (will add it to exclusion list)
07:16:22.46 -02:57:52.8 -- not an asteroid (will add it to exclusion list)
06:52:57.37 -03:04:55.0 -- not an asteroid (will add it to exclusion list)
07:04:20.49 -00:08:22.7 -- not an asteroid (will add it to exclusion list)
07:01:46.09 +01:19:50.1 -- not an asteroid (will add it to exclusion list)
06:39:36.65 -04:34:34.5 -- not an asteroid (will add it to exclusion list)
06:57:11.88 -03:58:11.5 -- not an asteroid (will add it to exclusion list)
07:08:12.41 -03:12:25.9 -- not an asteroid (will add it to exclusion list)
07:02:02.02 +00:07:46.9 -- not an asteroid (will add it to exclusion list)
06:54:48.32 +00:23:19.3 -- not an asteroid (will add it to exclusion list)
06:59:40.39 -00:39:47.1 -- not an asteroid (will add it to exclusion list)
07:13:15.22 -00:27:59.6 -- not an asteroid (will add it to exclusion list)
07:06:31.76 -04:48:14.7 -- not an asteroid (will add it to exclusion list)
07:08:43.17 -05:05:29.3 -- not an asteroid (will add it to exclusion list)
06:49:46.85 -03:36:01.0 -- not an asteroid (will add it to exclusion list)
06:50:50.97 -02:36:25.9 -- not an asteroid (will add it to exclusion list)
07:10:18.85 -06:07:57.8 -- not an asteroid (will add it to exclusion list)
07:03:11.83 +01:45:15.4 -- not an asteroid (will add it to exclusion list)
07:01:59.85 -02:00:41.8 -- not an asteroid (will add it to exclusion list)
07:17:27.88 +00:52:46.6 -- not an asteroid (will add it to exclusion list)
06:54:07.36 -03:06:07.8 -- not an asteroid (will add it to exclusion list)
07:00:27.47 -00:07:02.7 -- not an asteroid (will add it to exclusion list)
07:04:33.60 -04:28:40.3 -- not an asteroid (will add it to exclusion list)
07:06:45.54 -01:30:49.7 -- not an asteroid (will add it to exclusion list)
06:54:15.22 -02:04:22.9 -- not an asteroid (will add it to exclusion list)
06:59:35.88 -05:28:09.7 -- not an asteroid (will add it to exclusion list)
07:12:56.91 +00:52:07.2 -- not an asteroid (will add it to exclusion list)
07:01:00.36 -00:27:54.0 -- not an asteroid (will add it to exclusion list)
06:44:39.52 +00:10:06.0 -- not an asteroid (will add it to exclusion list)
07:01:49.00 -03:26:19.2 -- not an asteroid (will add it to exclusion list)
06:50:00.14 -03:51:11.7 -- not an asteroid (will add it to exclusion list)
06:55:10.24 -02:56:00.4 -- not an asteroid (will add it to exclusion list)
06:56:49.12 +00:46:33.2 -- not an asteroid (will add it to exclusion list)
06:46:16.99 -05:17:46.5 -- not an asteroid (will add it to exclusion list)
06:58:24.59 -03:02:34.6 -- not an asteroid (will add it to exclusion list)
06:59:34.21 -02:33:57.8 -- not an asteroid (will add it to exclusion list)
06:52:51.61 -02:22:45.2 -- not an asteroid (will add it to exclusion list)
07:05:41.67 -01:29:58.7 -- not an asteroid (will add it to exclusion list)
06:51:08.17 -02:08:43.6 -- not an asteroid (will add it to exclusion list)
07:04:26.89 +00:59:22.0 -- not an asteroid (will add it to exclusion list)
06:54:00.04 -05:06:47.0 -- not an asteroid (will add it to exclusion list)
06:55:24.68 -00:53:53.6 -- not an asteroid (will add it to exclusion list)
06:57:24.07 -02:57:03.4 -- not an asteroid (will add it to exclusion list)
06:48:45.19 +01:09:19.8 -- not an asteroid (will add it to exclusion list)
07:00:54.96 -03:04:10.3 -- not an asteroid (will add it to exclusion list)
06:56:39.00 -01:28:50.8 -- not an asteroid (will add it to exclusion list)
07:05:06.30 -04:50:35.6 -- not an asteroid (will add it to exclusion list)
06:54:55.00 -01:21:36.2 -- not an asteroid (will add it to exclusion list)
07:06:11.11 -02:50:59.9 -- not an asteroid (will add it to exclusion list)
06:40:24.07 -03:51:05.6 -- not an asteroid (will add it to exclusion list)
07:09:21.54 +01:07:27.5 -- not an asteroid (will add it to exclusion list)
06:59:49.61 -06:00:34.9 -- not an asteroid (will add it to exclusion list)
06:51:34.23 -01:39:22.5 -- not an asteroid (will add it to exclusion list)
07:11:26.80 -03:39:48.3 -- not an asteroid (will add it to exclusion list)
06:51:37.36 +01:29:00.1 -- not an asteroid (will add it to exclusion list)
07:07:34.13 -03:14:12.8 -- not an asteroid (will add it to exclusion list)
06:44:56.87 +00:56:56.5 -- not an asteroid (will add it to exclusion list)
06:47:59.48 -01:20:54.9 -- not an asteroid (will add it to exclusion list)
06:57:44.45 -03:47:48.0 -- not an asteroid (will add it to exclusion list)
06:54:22.77 -02:36:36.8 -- not an asteroid (will add it to exclusion list)
06:51:16.10 -00:44:17.2 -- not an asteroid (will add it to exclusion list)
06:52:15.35 -01:03:58.8 -- not an asteroid (will add it to exclusion list)
06:57:50.56 -00:57:55.8 -- not an asteroid (will add it to exclusion list)
06:46:21.66 -00:23:11.6 -- not an asteroid (will add it to exclusion list)
06:47:48.31 -01:09:01.5 -- not an asteroid (will add it to exclusion list)
07:12:49.82 -03:03:25.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:39:36.65 -04:34:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:24.07 -03:51:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:45.56 +00:35:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:01.87 -04:32:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:39.52 +00:10:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:56.87 +00:56:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:16.99 -05:17:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:21.66 -00:23:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:36.45 -03:38:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:48.31 -01:09:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:59.48 -01:20:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:45.19 +01:09:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:36.09 -00:19:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:46.85 -03:36:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:00.14 -03:51:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:18.43 -04:39:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:50.97 -02:36:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:56.01 -02:40:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:57.40 -01:59:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:58.14 -02:14:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:59.53 -02:47:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:08.17 -02:08:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:13.30 -01:21:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:14.95 -04:32:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:16.10 -00:44:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:17.40 -02:53:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:34.23 -01:39:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:34.68 -01:53:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:37.36 +01:29:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:43.68 -00:26:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:46.19 -05:25:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:03.56 -00:56:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:07.76 +00:28:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:15.35 -01:03:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:23.48 -02:34:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:46.10 -01:34:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:51.61 -02:22:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:53.59 +01:22:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:57.37 -03:04:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:05.71 +00:29:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:07.39 -01:35:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:25.72 -04:34:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:29.91 -01:56:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:30.53 -03:06:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:34.00 -00:32:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:42.56 -01:01:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:52.20 -02:12:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:00.04 -05:06:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:05.71 -03:49:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:07.36 -03:06:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:15.22 -02:04:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:22.77 -02:36:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:46.06 -00:27:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:48.32 +00:23:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:55.00 -01:21:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:57.30 -01:11:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:03.17 -01:02:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:10.24 -02:56:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:20.59 +00:53:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:24.68 -00:53:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:47.99 +01:18:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:12.23 +00:18:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:39.00 -01:28:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:49.12 +00:46:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:00.74 +00:17:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:11.88 -03:58:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:16.36 -02:12:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:24.07 -02:57:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:31.08 +00:41:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:33.41 -03:31:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:44.45 -03:47:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:47.57 +00:12:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:49.50 -00:05:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:50.56 -00:57:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:55.19 -04:37:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:03.49 -05:54:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:08.39 -01:38:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:09.65 +00:53:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:24.59 -03:02:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:26.68 -00:54:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:50.25 -01:53:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:01.82 -03:10:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:09.54 +00:41:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:25.58 -01:04:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:30.36 +00:22:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:32.97 -01:48:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:34.21 -02:33:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:35.88 -05:28:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:38.56 -06:13:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:40.22 -00:40:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:40.39 -00:39:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:49.61 -06:00:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:50.16 +00:16:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:56.95 +01:13:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:12.55 +00:10:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:14.73 -00:57:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:27.47 -00:07:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:35.32 -02:31:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:40.18 -02:26:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:54.96 -03:04:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:00.36 -00:27:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:00.95 -00:25:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:07.30 +00:37:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:24.07 +01:06:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:46.09 +01:19:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:49.00 -03:26:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:50.71 +01:44:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:52.57 -01:40:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:59.85 -02:00:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:00.71 +01:40:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:01.73 +00:22:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:02.02 +00:07:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:21.41 -04:03:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:32.22 +00:30:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:32.32 -00:13:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:34.25 -04:55:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:47.42 -03:11:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:02.18 +01:23:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:06.80 -04:06:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:11.83 +01:45:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:14.42 +01:07:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:22.27 -04:53:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:25.24 -00:05:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:26.98 -05:01:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:52.74 +00:49:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:55.55 -04:49:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:17.38 +01:02:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:20.49 -00:08:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:20.84 -04:41:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:26.89 +00:59:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:33.60 -04:28:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:36.92 +00:42:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:44.65 -03:46:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:57.17 -01:40:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:00.04 +01:38:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:06.30 -04:50:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:08.36 -04:26:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:24.98 -00:59:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:30.61 +01:36:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:38.79 -00:02:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:41.67 -01:29:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:49.13 +01:38:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:50.93 -02:05:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:55.55 -03:57:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:01.56 -02:28:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:11.11 -02:50:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:24.10 +00:20:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:24.61 -00:09:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:31.76 -04:48:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:45.54 -01:30:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:02.21 -01:54:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:11.39 -02:58:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:15.17 -04:18:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:20.90 -03:23:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:34.13 -03:14:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:54.99 -05:37:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:02.81 -03:23:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:12.41 -03:12:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:29.18 -00:58:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:30.45 -01:56:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:41.86 +01:18:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.17 -05:05:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.92 -03:56:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:05.32 -01:22:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:21.54 +01:07:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:39.86 -05:35:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:59.74 +01:25:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:02.16 -03:03:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:16.97 -04:37:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:18.85 -06:07:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:29.63 -04:23:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:30.43 -02:58:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:41.27 -05:05:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:55.70 -00:46:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:00.52 -02:53:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:26.80 -03:39:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:11.75 -01:59:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:16.06 -03:44:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:26.22 +01:50:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:39.25 -02:45:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:49.82 -03:03:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:56.91 +00:52:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:10.29 -05:21:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:11.72 +01:02:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:15.22 -00:27:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:23.19 +01:43:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:48.27 -00:49:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:02.03 -01:05:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:38.80 -03:56:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:41.20 -00:43:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:57.39 -05:11:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:26.79 -03:19:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:49.73 -00:37:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:07.40 +01:27:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:22.46 -02:57:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:33.73 -05:05:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:01.01 -00:19:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:13.03 -00:34:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:27.88 +00:52:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:43.83 -04:05:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:51.17 -01:41:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:56.41 -02:49:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:04.95 -01:25:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:17.99 -00:24:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:22.34 +00:01:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:49.57 -01:01:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:03.35 -04:45:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:13.98 -05:31:01.9 -- 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)
06:39:36.65 -04:34:34.5 -- not a known variable star
06:40:24.07 -03:51:05.6 -- not a known variable star
06:43:45.56 +00:35:14.9 -- not a known variable star
06:44:01.87 -04:32:27.5 -- a known variable star
06:44:39.52 +00:10:06.0 -- a known variable star
06:44:56.87 +00:56:56.5 -- not a known variable star
06:46:16.99 -05:17:46.5 -- not a known variable star
06:46:21.66 -00:23:11.6 -- not a known variable star
06:46:36.45 -03:38:14.6 -- not a known variable star
06:47:48.31 -01:09:01.5 -- not a known variable star
06:47:59.48 -01:20:54.9 -- not a known variable star
06:48:45.19 +01:09:19.8 -- not a known variable star
06:49:36.09 -00:19:57.1 -- not a known variable star
06:49:46.85 -03:36:01.0 -- not a known variable star
06:50:00.14 -03:51:11.7 -- a known variable star
06:50:18.43 -04:39:46.6 -- not a known variable star
06:50:50.97 -02:36:25.9 -- not a known variable star
06:50:56.01 -02:40:07.2 -- not a known variable star
06:50:57.40 -01:59:58.4 -- not a known variable star
06:50:58.14 -02:14:41.0 -- a known variable star
06:50:59.53 -02:47:53.0 -- not a known variable star
06:51:08.17 -02:08:43.6 -- a known variable star
06:51:13.30 -01:21:59.2 -- a known variable star
06:51:14.95 -04:32:31.6 -- not a known variable star
06:51:16.10 -00:44:17.2 -- a known variable star
06:51:17.40 -02:53:49.8 -- not a known variable star
06:51:34.23 -01:39:22.5 -- not a known variable star
06:51:34.68 -01:53:51.6 -- a known variable star
06:51:37.36 +01:29:00.1 -- not a known variable star
06:51:43.68 -00:26:00.9 -- not a known variable star
06:51:46.19 -05:25:56.1 -- a known variable star
06:52:03.56 -00:56:53.2 -- not a known variable star
06:52:07.76 +00:28:19.8 -- not a known variable star
06:52:15.35 -01:03:58.8 -- not a known variable star
06:52:23.48 -02:34:55.9 -- a known variable star
06:52:46.10 -01:34:15.7 -- not a known variable star
06:52:51.61 -02:22:45.2 -- not a known variable star
06:52:53.59 +01:22:23.6 -- not a known variable star
06:52:57.37 -03:04:55.0 -- not a known variable star
06:53:05.71 +00:29:07.9 -- a known variable star
06:53:07.39 -01:35:07.7 -- not a known variable star
06:53:25.72 -04:34:19.7 -- not a known variable star
06:53:29.91 -01:56:22.6 -- not a known variable star
06:53:30.53 -03:06:06.5 -- a known variable star
06:53:34.00 -00:32:05.2 -- not a known variable star
06:53:42.56 -01:01:10.3 -- not a known variable star
06:53:52.20 -02:12:22.9 -- not a known variable star
06:54:00.04 -05:06:47.0 -- not a known variable star
06:54:05.71 -03:49:50.5 -- a known variable star
06:54:07.36 -03:06:07.8 -- not a known variable star
06:54:15.22 -02:04:22.9 -- a known variable star
06:54:22.77 -02:36:36.8 -- not a known variable star
06:54:46.06 -00:27:03.5 -- not a known variable star
06:54:48.32 +00:23:19.3 -- a known variable star
06:54:55.00 -01:21:36.2 -- not a known variable star
06:54:57.30 -01:11:47.8 -- not a known variable star
06:55:03.17 -01:02:50.6 -- not a known variable star
06:55:10.24 -02:56:00.4 -- not a known variable star
06:55:20.59 +00:53:19.7 -- not a known variable star
06:55:24.68 -00:53:53.6 -- a known variable star
06:55:47.99 +01:18:47.2 -- a known variable star
06:56:12.23 +00:18:26.3 -- not a known variable star
06:56:39.00 -01:28:50.8 -- a known variable star
06:56:49.12 +00:46:33.2 -- not a known variable star
06:57:00.74 +00:17:38.0 -- not a known variable star
06:57:11.88 -03:58:11.5 -- not a known variable star
06:57:16.36 -02:12:54.6 -- not a known variable star
06:57:24.07 -02:57:03.4 -- not a known variable star
06:57:31.08 +00:41:49.0 -- not a known variable star
06:57:33.41 -03:31:48.4 -- not a known variable star
06:57:44.45 -03:47:48.0 -- not a known variable star
06:57:47.57 +00:12:34.3 -- not a known variable star
06:57:49.50 -00:05:50.6 -- not a known variable star
06:57:50.56 -00:57:55.8 -- not a known variable star
06:57:55.19 -04:37:48.5 -- a known variable star
06:58:03.49 -05:54:02.5 -- not a known variable star
06:58:08.39 -01:38:52.7 -- not a known variable star
06:58:09.65 +00:53:07.1 -- not a known variable star
06:58:24.59 -03:02:34.6 -- not a known variable star
06:58:26.68 -00:54:20.5 -- not a known variable star
06:58:50.25 -01:53:11.2 -- not a known variable star
06:59:01.82 -03:10:13.1 -- not a known variable star
06:59:09.54 +00:41:52.9 -- not a known variable star
06:59:25.58 -01:04:49.6 -- not a known variable star
06:59:30.36 +00:22:07.0 -- a known variable star
06:59:32.97 -01:48:18.9 -- a known variable star
06:59:34.21 -02:33:57.8 -- a known variable star
06:59:35.88 -05:28:09.7 -- not a known variable star
06:59:38.56 -06:13:04.0 -- not a known variable star
06:59:40.22 -00:40:25.3 -- not a known variable star
06:59:40.39 -00:39:47.1 -- not a known variable star
06:59:49.61 -06:00:34.9 -- not a known variable star
06:59:50.16 +00:16:20.9 -- not a known variable star
06:59:56.95 +01:13:10.5 -- a known variable star
07:00:12.55 +00:10:02.4 -- not a known variable star
07:00:14.73 -00:57:25.5 -- a known variable star
07:00:27.47 -00:07:02.7 -- not a known variable star
07:00:35.32 -02:31:06.9 -- not a known variable star
07:00:40.18 -02:26:31.6 -- not a known variable star
07:00:54.96 -03:04:10.3 -- not a known variable star
07:01:00.36 -00:27:54.0 -- a known variable star
07:01:00.95 -00:25:44.2 -- not a known variable star
07:01:07.30 +00:37:52.7 -- not a known variable star
07:01:24.07 +01:06:07.7 -- not a known variable star
07:01:46.09 +01:19:50.1 -- not a known variable star
07:01:49.00 -03:26:19.2 -- not a known variable star
07:01:50.71 +01:44:17.8 -- a known variable star
07:01:52.57 -01:40:51.6 -- not a known variable star
07:01:59.85 -02:00:41.8 -- not a known variable star
07:02:00.71 +01:40:09.6 -- not a known variable star
07:02:01.73 +00:22:42.0 -- not a known variable star
07:02:02.02 +00:07:46.9 -- not a known variable star
07:02:21.41 -04:03:30.8 -- a known variable star
07:02:32.22 +00:30:19.8 -- not a known variable star
07:02:32.32 -00:13:10.6 -- not a known variable star
07:02:34.25 -04:55:48.5 -- a known variable star
07:02:47.42 -03:11:46.8 -- not a known variable star
07:03:02.18 +01:23:58.0 -- not a known variable star
07:03:06.80 -04:06:44.4 -- not a known variable star
07:03:11.83 +01:45:15.4 -- not a known variable star
07:03:14.42 +01:07:06.3 -- not a known variable star
07:03:22.27 -04:53:37.4 -- not a known variable star
07:03:25.24 -00:05:26.4 -- a known variable star
07:03:26.98 -05:01:12.3 -- a known variable star
07:03:52.74 +00:49:48.2 -- not a known variable star
07:03:55.55 -04:49:26.2 -- not a known variable star
07:04:17.38 +01:02:40.1 -- not a known variable star
07:04:20.49 -00:08:22.7 -- not a known variable star
07:04:20.84 -04:41:01.3 -- not a known variable star
07:04:26.89 +00:59:22.0 -- not a known variable star
07:04:33.60 -04:28:40.3 -- not a known variable star
07:04:36.92 +00:42:05.6 -- not a known variable star
07:04:44.65 -03:46:31.1 -- not a known variable star
07:04:57.17 -01:40:50.3 -- a known variable star
07:05:00.04 +01:38:42.5 -- not a known variable star
07:05:06.30 -04:50:35.6 -- a known variable star
07:05:08.36 -04:26:25.2 -- a known variable star
07:05:24.98 -00:59:48.6 -- a known variable star
07:05:30.61 +01:36:36.6 -- not a known variable star
07:05:38.79 -00:02:18.3 -- not a known variable star
07:05:41.67 -01:29:58.7 -- not a known variable star
07:05:49.13 +01:38:16.9 -- not a known variable star
07:05:50.93 -02:05:13.9 -- not a known variable star
07:05:55.55 -03:57:45.4 -- not a known variable star
07:06:01.56 -02:28:21.7 -- not a known variable star
07:06:11.11 -02:50:59.9 -- not a known variable star
07:06:24.10 +00:20:28.4 -- not a known variable star
07:06:24.61 -00:09:13.5 -- not a known variable star
07:06:31.76 -04:48:14.7 -- not a known variable star
07:06:45.54 -01:30:49.7 -- a known variable star
07:07:02.21 -01:54:20.2 -- not a known variable star
07:07:11.39 -02:58:18.8 -- not a known variable star
07:07:15.17 -04:18:17.6 -- not a known variable star
07:07:20.90 -03:23:28.5 -- a known variable star
07:07:34.13 -03:14:12.8 -- not a known variable star
07:07:54.99 -05:37:21.2 -- a known variable star
07:08:02.81 -03:23:35.8 -- not a known variable star
07:08:12.41 -03:12:25.9 -- not a known variable star
07:08:29.18 -00:58:27.7 -- a known variable star
07:08:30.45 -01:56:44.1 -- a known variable star
07:08:41.86 +01:18:47.7 -- a known variable star
07:08:43.17 -05:05:29.3 -- a known variable star
07:08:43.92 -03:56:10.9 -- not a known variable star
07:09:05.32 -01:22:05.7 -- a known variable star
07:09:21.54 +01:07:27.5 -- a known variable star
07:09:39.86 -05:35:35.0 -- a known variable star
07:09:59.74 +01:25:46.8 -- not a known variable star
07:10:02.16 -03:03:52.9 -- not a known variable star
07:10:16.97 -04:37:52.6 -- a known variable star
07:10:18.85 -06:07:57.8 -- not a known variable star
07:10:29.63 -04:23:43.2 -- a known variable star
07:10:30.43 -02:58:56.4 -- not a known variable star
07:10:41.27 -05:05:04.7 -- a known variable star
07:10:55.70 -00:46:12.4 -- a known variable star
07:11:00.52 -02:53:38.9 -- not a known variable star
07:11:26.80 -03:39:48.3 -- not a known variable star
07:12:11.75 -01:59:49.6 -- not a known variable star
07:12:16.06 -03:44:42.7 -- not a known variable star
07:12:26.22 +01:50:34.1 -- not a known variable star
07:12:39.25 -02:45:30.3 -- not a known variable star
07:12:49.82 -03:03:25.7 -- a known variable star
07:12:56.91 +00:52:07.2 -- a known variable star
07:13:10.29 -05:21:11.2 -- a known variable star
07:13:11.72 +01:02:12.9 -- not a known variable star
07:13:15.22 -00:27:59.6 -- a known variable star
07:13:23.19 +01:43:05.5 -- a known variable star
07:13:48.27 -00:49:58.0 -- not a known variable star
07:14:02.03 -01:05:48.1 -- not a known variable star
07:14:38.80 -03:56:24.7 -- not a known variable star
07:14:41.20 -00:43:06.9 -- not a known variable star
07:14:57.39 -05:11:43.0 -- not a known variable star
07:15:26.79 -03:19:53.3 -- not a known variable star
07:15:49.73 -00:37:01.5 -- a known variable star
07:16:07.40 +01:27:14.8 -- not a known variable star
07:16:22.46 -02:57:52.8 -- not a known variable star
07:16:33.73 -05:05:45.9 -- a known variable star
07:17:01.01 -00:19:59.4 -- not a known variable star
07:17:13.03 -00:34:59.2 -- not a known variable star
07:17:27.88 +00:52:46.6 -- not a known variable star
07:17:43.83 -04:05:30.0 -- a known variable star
07:17:51.17 -01:41:37.6 -- a known variable star
07:17:56.41 -02:49:58.3 -- not a known variable star
07:18:04.95 -01:25:37.0 -- not a known variable star
07:18:17.99 -00:24:26.0 -- not a known variable star
07:18:22.34 +00:01:08.7 -- not a known variable star
07:18:49.57 -01:01:56.9 -- not a known variable star
07:19:03.35 -04:45:19.8 -- not a known variable star
07:19:13.98 -05:31:01.9 -- a known variable star
Found 150 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
208 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 208 (excluding asteroids and hot pixels, 150 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461155.60897248 -observatory V36
00:59:24.81 +03:42:44.3 Mercury (-0.4mag)
03:53:55.96 +20:55:47.1 Venus (-3.9mag)
00:43:39.86 +03:41:13.4 Mars (1.2mag)
07:17:11.75 +22:38:26.8 Jupiter (-2.0mag)
00:33:10.41 +01:13:40.9 Saturn (0.9mag)
03:49:40.93 +19:53:46.9 Uranus (5.8mag)
00:11:59.81 -00:08:07.3 Neptune (7.8mag)
20:34:04.27 -22:53:19.3 Pluto (14.5mag)
09:20:21.44 +17:04:03.0 Moon (-10.7mag)
-rw-r--r-- 1 apache apache 363 Apr 24 21:40 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461155.60897248:
07:17:16.71 +22:38:17.9 Io (5.8mag)
07:17:05.29 +22:38:39.0 Europa (6.0mag)
07:17:01.42 +22:38:43.6 Ganymede (5.4mag)
07:16:39.18 +22:39:38.5 Callisto (6.6mag)
07:20:05.67 +22:22:10.8 Himalia (15.4mag)
07:17:10.14 +22:38:32.4 Thebe (16.3mag)
07:20:27.12 +22:52:19.4 Elara (17.3mag)
07:16:41.62 +23:13:41.2 Pasiphae (17.5mag)
07:25:18.33 +22:37:16.1 Carme (18.6mag)
00:33:16.75 +01:13:27.2 Titan (8.8mag)
00:33:08.53 +01:13:44.7 Rhea (10.1mag)
00:32:40.80 +01:12:26.8 Iapetus (11.5mag)
00:33:03.49 +01:13:36.2 Hyperion (14.8mag)
00:34:39.66 +01:21:27.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 24 21:40 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461155.60897248:
16:13:30.62 -21:54:44.0 JWST
17:41:27.51 +37:57:44.9 Chandra
17:03:29.48 -50:21:50.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 24 21:40 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461155.60897248 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
05:48:29.63 +30:42:18.0 17.9mag P/2009 WX51 (Catalina)
18:54:50.12 -29:20:43.2 13.8mag P/2010 H2 (Vales)
05:13:36.92 -69:15:18.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:34:37.60 +31:30:17.0 17.3mag C/2017 K2 (PANSTARRS)
17:29:07.53 +11:35:59.6 17.7mag C/2021 G2 (ATLAS)
23:12:20.95 +29:36:41.2 17.1mag C/2022 E2 (ATLAS)
04:40:00.19 +26:16:28.2 16.1mag C/2022 N2 (PANSTARRS)
09:05:54.13 +32:01:25.4 16.3mag C/2022 QE78 (ATLAS)
08:32:52.41 +00:45:56.3 17.4mag C/2022 R6 (PANSTARRS)
18:51:06.76 +19:16:21.2 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:37:26.64 -11:23:14.4 17.5mag P/2023 B1 (PANSTARRS)
09:04:03.18 -10:29:03.5 17.7mag C/2023 F3 (ATLAS)
22:02:26.21 +63:28:22.8 17.6mag C/2023 H5 (Lemmon)
19:09:57.51 -03:55:49.0 14.0mag C/2023 R1 (PANSTARRS)
20:55:49.51 +87:11:10.8 17.8mag C/2023 X2 (Lemmon)
06:23:12.14 +63:30:12.9 17.3mag C/2024 A1 (ATLAS)
05:31:55.61 +20:57:52.0 11.6mag C/2024 E1 (Wierzchos)
16:12:59.81 +07:51:47.5 17.3mag C/2024 G6 (ATLAS)
20:22:47.51 +17:48:57.7 14.5mag C/2024 J3 (ATLAS)
03:34:43.58 -21:02:50.3 16.3mag C/2024 T5 (ATLAS)
05:24:40.94 +43:07:42.1 17.8mag C/2025 J1 (Borisov)
13:02:25.92 +49:59:36.1 15.6mag C/2025 L1 (ATLAS)
03:40:16.75 -27:42:49.7 17.9mag C/2025 Q3 (ATLAS)
02:01:00.61 +10:05:30.1 7.8mag C/2025 R3 (PANSTARRS)
12:50:17.35 +03:31:52.5 17.4mag C/2025 Y1 (ATLAS)
04:25:56.74 +01:58:11.4 15.4mag C/2026 A1 (MAPS)
00:24:27.34 +38:44:52.1 14.9mag C/2026 B2 (Sun-Gao)
19:00:35.70 -09:13:18.4 11.3mag 10P/Tempel
14:47:56.45 +02:08:33.3 14.8mag 24P/Schaumasse
11:00:45.52 -01:15:39.8 15.7mag 29P/Schwassmann-Wachmann
10:38:06.57 -03:27:36.3 17.1mag 43P/Wolf-Harrington
02:02:49.60 +19:00:57.4 17.3mag 47P/Ashbrook-Jackson
07:28:08.61 +35:00:28.0 17.0mag 63P/Wild
23:40:24.40 -10:23:19.2 15.7mag 65P/Gunn
04:28:14.41 +24:13:16.5 16.0mag 76P/West-Kohoutek-Ikemura
01:25:54.90 +09:59:32.2 14.2mag 78P/Gehrels
23:29:49.21 -06:42:06.8 14.7mag 88P/Howell
02:36:43.02 +22:58:03.6 15.0mag 93P/Lovas
05:12:34.00 +32:43:35.1 16.1mag 123P/West-Hartley
08:40:00.51 +34:10:30.7 16.2mag 124P/Mrkos
02:47:26.82 +15:21:40.0 16.4mag 128P/Shoemaker-Holt
03:05:30.30 +15:33:12.9 17.6mag 131P/Mueller
02:14:56.43 +16:02:52.3 10.5mag 141P/Machholz
02:22:19.67 +08:12:54.8 10.5mag 141P-A/Machholz
01:04:03.57 +03:56:32.8 11.8mag 141P-D/Machholz
02:52:57.44 +09:55:04.3 18.0mag 141P-I/Machholz
01:27:58.62 +03:04:37.5 15.0mag 162P/SidingSpring
14:35:36.00 +00:43:20.0 17.9mag 210P/Christensen
22:03:41.06 -09:17:29.3 17.8mag 218P/LINEAR
17:17:20.62 -12:48:58.7 16.1mag 235P/LINEAR
05:54:28.34 +35:17:08.3 16.9mag 240P/NEAT
07:43:28.38 -04:14:44.2 17.8mag 242P/Spahr
22:39:43.17 -18:25:16.0 17.6mag 260P/McNaught
02:17:15.12 +22:43:42.5 17.9mag 295P/LINEAR
15:38:38.66 +07:32:22.9 17.5mag 391P/Kowalski
07:38:09.99 +21:22:09.2 17.7mag 450P/LONEOS
05:49:28.67 +44:30:02.4 17.6mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 24 21:40 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.52 -16:06:06.00 ASASSN-26cz 2026-04-22.28 16.29
14:21:40.08 +13:13:46.30 2026-04-22.16 15.12
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:21:40.08 +13:13:46.30 2026-04-22.16 15.12
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 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
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
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
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
-rw-r--r-- 1 apache apache 5.8K Apr 24 21:40 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
-rw-r--r-- 1 apache apache 188K Apr 24 21:40 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
03:58:37.523 -47:58:27.05 AT 2026jyc 2026-03-10.04 22.794
04:19:14.199 -48:07:43.84 AT 2026jyb 2026-03-22.02 23.509
04:14:48.000 -48:01:04.00 AT 2026jya 2026-03-07.06 22.906
04:17:07.910 -49:07:16.08 AT 2026jxz 2026-03-13.03 23.78
04:14:22.630 -48:22:12.14 AT 2026jxy 2026-03-07.06 21.712
04:01:07.229 -47:46:52.90 AT 2026jxx 2026-03-07.07 23.052
04:09:53.881 -47:38:41.66 AT 2026jxw 2026-03-16.05 23.624
04:08:49.695 -48:00:04.57 AT 2026jxv 2026-03-13.14 23.598
04:10:45.076 -47:56:49.63 AT 2026jxu 2026-03-10.04 23.502
04:14:31.399 -46:42:43.71 AT 2026jxt 2026-03-10.18 21.706
04:11:12.235 -45:58:40.33 AT 2026jxs 2026-03-25.100 22.751
03:55:48.361 -50:00:22.74 AT 2026jxr 2026-03-13.04 23.431
03:52:20.927 -49:00:26.83 AT 2026jxq 2026-04-03.01 21.127
03:45:32.951 -49:53:47.26 AT 2026jxp 2026-03-16.05 22.986
14:06:31.160 +25:41:16.06 AT 2026jxo 2026-04-17.40 19.74
15:04:50.183 +06:52:09.46 AT 2026jxn 2026-04-15.48 20.43
15:54:08.337 +01:23:10.14 AT 2026jxm 2026-04-15.47 20.9
16:51:56.725 +00:24:09.11 AT 2026jxl 2026-04-15.54 21.12
16:40:46.820 -23:21:05.30 AT 2026jxk 2026-04-17.18 16.1
11:40:08.766 +27:39:36.84 AT 2026jxj 2026-04-17.74 19.72
-rw-r--r-- 1 apache apache 30K Apr 24 21:40 tns_transients_list.txt
