This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK
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 28.1198 2461158.6198 12.63 07:09:59.87 +01:25:48.9
213.77489 4.78138 galactic CMi Second-epoch detections are separated by 1.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.5056+01.4407 | 07:09:59.87 +01:25:48.9 (user input) | DBH (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:09:59.87 +01:25:48.9: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:09:59.87 +01:25:48.9: 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 J107.5056+01.4407,2461158.6198,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.5056+01.4407 20260428.1198 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 28.1198 2461158.6198 12.47 06:56:09.30 +00:23:33.9
213.12010 1.22862 galactic Mon Second-epoch detections are separated by 6.9" 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 | target | 06:56:09.30 +00:23:33.9 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.584+/-0.079 (K)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:56:09.30 +00:23:33.9: 14.86 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:56:09.30 +00:23:33.9: 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,2461158.6198,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.56 06:45:22.68 -02:49:59.9
214.76487 -2.63886 galactic Mon Second-epoch detections are separated by 2.1" and 4.9 pix
The object was found in VSX17" Gaia DR3 3105762801031293952
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.020 G 13.060 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:45:22.68 -02:49:59.9: 14.09 +/- 0.16 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:45:22.68 -02:49:59.9: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105762801031293952,2461158.6198,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105762801031293952 20260428.1198 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 28.1198 2461158.6198 12.48 07:07:51.73 -05:46:55.5
219.94895 1.00063 galactic Mon Second-epoch detections are separated by 1.3" and 5.0 pix
The object was found in VSX11" Gaia DR3 3053304074782538880
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.210 G 13.240 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:51.73 -05:46:55.5: 14.57 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:51.73 -05:46:55.5: 13.63 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053304074782538880,2461158.6198,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3053304074782538880 20260428.1198 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 28.1198 2461158.6198 12.39 06:43:56.50 +01:29:48.1
210.74508 -0.98469 galactic Mon Second-epoch detections are separated by 3.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J100.9767+01.4937 | 06:43:56.50 +01:29:48.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:43:56.50 +01:29:48.1: 14.66 +/- 0.31 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:56.50 +01:29:48.1: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.49 +/- 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 J100.9767+01.4937,2461158.6198,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9767+01.4937 20260428.1198 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.31 07:09:20.84 +01:37:48.3
213.52207 4.72768 galactic CMi Second-epoch detections are separated by 5.0" 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 | ATO J107.3360+01.6358 | 07:09:20.84 +01:37:48.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:09:20.84 +01:37:48.3: 14.63 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:09:20.84 +01:37:48.3: 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 J107.3360+01.6358,2461158.6198,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3360+01.6358 20260428.1198 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 28.1198 2461158.6198 12.37 07:01:35.54 -07:10:47.4
220.47627 -1.02450 galactic Mon Second-epoch detections are separated by 6.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:01:35.54 -07:10:47.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:35.54 -07:10:47.4: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:35.54 -07:10:47.4: 14.08 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.08 +/- 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,2461158.6198,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.26 06:32:50.20 -03:46:06.9
214.17652 -5.85259 galactic Mon Second-epoch detections are separated by 2.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J098.2059-03.7644 | 06:32:49.42 -03:45:51.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:32:50.20 -03:46:06.9: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:32:50.20 -03:46:06.9: 13.15 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.2059-03.7644,2461158.6198,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.2059-03.7644 20260428.1198 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 28.1198 2461158.6198 12.20 07:08:29.29 -00:58:27.2
215.74644 3.34728 galactic Mon Second-epoch detections are separated by 3.1" and 5.6 pix
The object was found in VSX 2" 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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:29.29 -00:58:27.2: 14.70 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:29.29 -00:58:27.2: 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 3109604288498805632,2461158.6198,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109604288498805632 20260428.1198 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 28.1198 2461158.6198 12.35 07:07:06.86 +01:29:04.5
213.39709 4.16460 galactic Mon Second-epoch detections are separated by 0.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J106.7763+01.4873 | 07:07:06.86 +01:29:04.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:06.86 +01:29:04.5: 14.07 +/- 0.20 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:06.86 +01:29:04.5: 15.36 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.07 +/- 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 J106.7763+01.4873,2461158.6198,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.7763+01.4873 20260428.1198 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 28.1198 2461158.6198 12.31 06:54:34.58 +02:24:43.3
211.14214 1.79746 galactic Mon Second-epoch detections are separated by 0.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:54:34.58 +02:24:43.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:34.58 +02:24:43.3: 14.82 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:34.58 +02:24:43.3: 14.14 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.14 +/- 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,2461158.6198,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.12 07:03:22.35 -04:53:37.3
218.64650 0.41580 galactic Mon Second-epoch detections are separated by 2.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | 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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:22.35 -04:53:37.3: 14.70 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:22.35 -04:53:37.3: 15.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101509138446206464,2461158.6198,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101509138446206464 20260428.1198 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.06 06:24:52.04 -03:33:44.0
213.08521 -7.53219 galactic Mon Second-epoch detections are separated by 0.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J096.2199-03.5619 | 06:24:52.04 -03:33:44.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:24:52.04 -03:33:44.0: 12.88 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:24:52.04 -03:33:44.0: 13.55 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.29 +/- 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 J096.2199-03.5619,2461158.6198,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.2199-03.5619 20260428.1198 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 28.1198 2461158.6198 12.03 07:03:40.15 -01:07:50.1
215.33392 2.20464 galactic Mon Second-epoch detections are separated by 0.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3109541277034406144 | 07:03:40.37 -01:07:35.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:03:40.15 -01:07:50.1: 14.80 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:03:40.15 -01:07:50.1: 15.38 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3109541277034406144,2461158.6198,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3109541277034406144 20260428.1198 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.18 06:59:30.13 +00:22:10.1
213.52253 1.96272 galactic Mon Second-epoch detections are separated by 2.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3112954191193204096 | 06:59:30.10 +00:22:23.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:59:30.13 +00:22:10.1: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:59:30.13 +00:22:10.1: 13.24 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 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 3112954191193204096,2461158.6198,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112954191193204096 20260428.1198 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 28.1198 2461158.6198 12.04 06:53:55.00 +02:25:33.8
211.05459 1.65715 galactic Mon Second-epoch detections are separated by 1.2" and 5.4 pix
The object was found in VSX19" Gaia DR3 3126260828808492544
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
11.820 G 11.840 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:53:55.00 +02:25:33.8: 14.89 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:53:55.00 +02:25:33.8: 13.60 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.60 +/- 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 3126260828808492544,2461158.6198,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126260828808492544 20260428.1198 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 28.1198 2461158.6198 11.81 07:17:43.21 -05:40:05.0
220.98228 3.22776 galactic Mon Second-epoch detections are separated by 1.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J109.4339-05.6761 | 07:17:43.21 -05:40:05.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:17:43.21 -05:40:05.0: 14.31 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:17:43.21 -05:40:05.0: 14.71 +/- 0.24 detection
Forced photometry reference-image weighted average: 14.71 +/- 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 J109.4339-05.6761,2461158.6198,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.4339-05.6761 20260428.1198 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.02 07:12:01.86 -01:11:14.3
216.34287 4.03674 galactic Mon Second-epoch detections are separated by 1.1" and 5.4 pix
The object was found in ASASSN-V 4" ASASSN-V J071201.82-011118.1
Type: EA
MeanMag 12.68 m Amp. 0.27 m Period 3.3076416 d
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:01.86 -01:11:14.3: 14.62 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:01.86 -01:11:14.3: 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
VARIABLE_NAME,2461158.6198,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260428.1198 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 28.1198 2461158.6198 11.93 07:08:41.75 +01:18:43.1
213.73176 4.43782 galactic CMi Second-epoch detections are separated by 2.6" and 5.4 pix
The object was found in VSX 8" Gaia DR3 3114481210983029120
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.300 G 13.330 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:41.75 +01:18:43.1: 14.71 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:41.75 +01:18:43.1: 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 3114481210983029120,2461158.6198,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114481210983029120 20260428.1198 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.71 06:46:34.59 +01:47:57.8
210.77635 -0.26068 galactic Mon Second-epoch detections are separated by 2.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.391 Ingeborg -302 396 498 16.2 -0 0
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:46:34.59 +01:47:57.8: 14.55 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:46:34.59 +01:47:57.8: 12.50 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461158.6198,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260428.1198 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 28.1198 2461158.6198 11.58 06:23:23.70 -03:28:38.7
212.84110 -7.82139 galactic Mon Second-epoch detections are separated by 1.3" and 5.5 pix
The object was found in VSX 3" Gaia DR3 3116727307079971968
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.560 G 12.580 G A
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:23:23.70 -03:28:38.7: 13.36 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:23:23.70 -03:28:38.7: 13.94 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.69 +/- 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 3116727307079971968,2461158.6198,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3116727307079971968 20260428.1198 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.21 07:10:59.50 -03:55:09.7
218.65368 2.55028 galactic Mon Second-epoch detections are separated by 4.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3107635033119937152 | 07:11:00.24 -03:55:36.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:10:59.50 -03:55:09.7: 14.47 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:10:59.50 -03:55:09.7: 15.30 +/- 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 3107635033119937152,2461158.6198,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107635033119937152 20260428.1198 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 28.1198 2461158.6198 11.07 06:58:42.69 -03:39:02.5
217.00957 -0.04874 galactic Mon Second-epoch detections are separated by 1.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.6731-03.6647 | 06:58:42.32 -03:39:20.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.211+/-0.037 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:58:42.69 -03:39:02.5: 14.64 +/- 0.30 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:42.69 -03:39:02.5: 12.96 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 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 J104.6731-03.6647,2461158.6198,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6731-03.6647 20260428.1198 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 28.1198 2461158.6198 11.21 07:04:47.96 +02:23:27.9
212.32392 4.06198 galactic Mon Second-epoch detections are separated by 1.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3115564431795326208 | 07:04:47.23 +02:23:42.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:04:47.96 +02:23:27.9: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:04:47.96 +02:23:27.9: 15.44 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115564431795326208,2461158.6198,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115564431795326208 20260428.1198 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 28.1198 2461158.6198 11.06 07:08:44.23 -03:56:12.3
218.41017 2.04305 galactic Mon Second-epoch detections are separated by 2.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J107.1828-03.9366 | 07:08:44.38 -03:55:56.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:44.23 -03:56:12.3: 12.57 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:44.23 -03:56:12.3: 15.35 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.57 +/- 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 J107.1828-03.9366,2461158.6198,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1828-03.9366 20260428.1198 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 9.51 07:07:17.10 +01:47:31.0
213.14215 4.34252 galactic Mon Second-epoch detections are separated by 0.5" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3114743581946430208 | 07:07:18.40 +01:47:14.2 (Gaia DR3) | ACV/roAm/ (local) | (local) | Gaia3var=VARIABLE SpType: B8 1958PMcCO..13b....V AG+01 841 J-Ks=0.008+/-0.028 (A)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:17.10 +01:47:31.0: 12.89 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:17.10 +01:47:31.0: 15.42 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.89 +/- 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 3114743581946430208,2461158.6198,9.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114743581946430208 20260428.1198 9.51CV 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 28.1198 2461158.6198 10.66 06:39:40.54 +03:07:11.8
208.81387 -1.19019 galactic Mon Second-epoch detections are separated by 0.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3127154388164101504 | 06:39:38.62 +03:06:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B0: 1985CBVMS.C......0V NGC 2244 +03 245 J-Ks=0.171+/-0.051 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:39:40.54 +03:07:11.8: 11.96 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:39:40.54 +03:07:11.8: 11.60 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.65 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127154388164101504,2461158.6198,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127154388164101504 20260428.1198 10.66CV 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 28.1198 2461158.6198 11.04 06:21:43.87 -00:15:06.8
209.75571 -6.72137 galactic Mon Second-epoch detections are separated by 0.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J062141.32-001505.4 | 06:21:41.32 -00:15:05.5 (Gaia DR3) | SRS (local) | 25.838000000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.190+/-0.035 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:21:43.87 -00:15:06.8: 13.24 +/- 0.09 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:21:43.87 -00:15:06.8: 11.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062141.32-001505.4,2461158.6198,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062141.32-001505.4 20260428.1198 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.31 06:24:07.43 -00:16:09.1
210.04713 -6.19769 galactic Mon Second-epoch detections are separated by 1.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J096.0408-00.2752 | 06:24:07.43 -00:16:09.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.230+/-0.033 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:24:07.43 -00:16:09.1: 12.23 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:24:07.43 -00:16:09.1: 12.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.0408-00.2752,2461158.6198,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.0408-00.2752 20260428.1198 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.33 07:08:35.57 +01:46:45.8
213.30257 4.62779 galactic CMi Second-epoch detections are separated by 1.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3114716781350331648 | 07:08:36.38 +01:46:22.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1949AnHar.112....1C HD 289699
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:08:35.57 +01:46:45.8: 14.64 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:08:35.57 +01:46:45.8: 15.43 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114716781350331648,2461158.6198,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114716781350331648 20260428.1198 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.48 07:11:05.36 -04:42:12.1
219.36132 2.21062 galactic Mon Second-epoch detections are separated by 1.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3059411793155039360 | 07:11:05.21 -04:42:14.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:11:05.36 -04:42:12.1: 14.66 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:11:05.36 -04:42:12.1: 15.32 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059411793155039360,2461158.6198,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059411793155039360 20260428.1198 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 28.1198 2461158.6198 11.55 06:45:27.75 +00:57:44.3
211.39415 -0.89044 galactic Mon Second-epoch detections are separated by 1.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J101.3667+00.9753 | 06:45:29.55 +00:57:53.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K 1949AnHar.112....1C HD 289051
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:45:27.75 +00:57:44.3: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:45:27.75 +00:57:44.3: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3667+00.9753,2461158.6198,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.3667+00.9753 20260428.1198 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.66 06:29:05.56 +03:16:44.9
207.45774 -3.46344 galactic Mon Second-epoch detections are separated by 1.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.2625+03.2755 | 06:29:03.87 +03:16:43.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1985CBVMS.C......0V NGC 2244 +03 69
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:29:05.56 +03:16:44.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:29:05.56 +03:16:44.9: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.2625+03.2755,2461158.6198,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.2625+03.2755 20260428.1198 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.62 06:26:59.98 +00:24:40.8
209.77048 -5.24677 galactic Mon Second-epoch detections are separated by 2.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J096.7458+00.4137 | 06:26:58.48 +00:24:30.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5) J-Ks=0.415+/-0.030 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:26:59.98 +00:24:40.8: 12.26 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:26:59.98 +00:24:40.8: 12.81 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.7458+00.4137,2461158.6198,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.7458+00.4137 20260428.1198 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 28.1198 2461158.6198 11.62 06:58:31.26 -07:10:56.3
220.13043 -1.70335 galactic Mon Second-epoch detections are separated by 1.7" and 5.6 pix
The object was found in VSX 3" Gaia DR3 3052678899341352064
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.590 G 12.610 G B
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:58:31.26 -07:10:56.3: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:58:31.26 -07:10:56.3: 15.10 +/- 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 3052678899341352064,2461158.6198,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3052678899341352064 20260428.1198 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 28.1198 2461158.6198 11.63 07:16:19.66 -06:57:24.2
221.96377 2.32260 galactic Mon Second-epoch detections are separated by 2.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3052008231606718336 | 07:16:19.08 -06:57:04.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:16:19.66 -06:57:24.2: 14.46 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:16:19.66 -06:57:24.2: 15.11 +/- 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 3052008231606718336,2461158.6198,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3052008231606718336 20260428.1198 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.79 07:19:20.23 -00:18:58.7
216.40746 6.05914 galactic Mon Second-epoch detections are separated by 1.1" and 5.3 pix
The object was found in VSX 5" Gaia DR3 3110277086535749248
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.720 G 13.760 G 0.047601500000 F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:19:20.23 -00:18:58.7: 14.57 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:19:20.23 -00:18:58.7: 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
Gaia DR3 3110277086535749248,2461158.6198,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110277086535749248 20260428.1198 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.79 06:51:37.46 -06:57:16.6
219.14876 -3.12379 galactic Mon Second-epoch detections are separated by 4.0" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J102.8995-06.9468 | 06:51:37.46 -06:57:16.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.325+/-0.033 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:51:37.46 -06:57:16.6: 14.74 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:37.46 -06:57:16.6: 13.46 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.8995-06.9468,2461158.6198,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.8995-06.9468 20260428.1198 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.79 06:22:05.04 -04:25:37.7
213.54781 -8.54219 galactic Mon Second-epoch detections are separated by 1.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3116515719811142400 | 06:22:02.56 -04:25:41.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1949AnHar.112....1C HD 294986 J-Ks=0.110+/-0.035 (A)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:22:05.04 -04:25:37.7: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:22:05.04 -04:25:37.7: 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
Gaia DR3 3116515719811142400,2461158.6198,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3116515719811142400 20260428.1198 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.71 07:06:24.13 +00:20:29.6
214.33530 3.48497 galactic Mon Second-epoch detections are separated by 1.6" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3114263159786050944 | 07:06:23.17 +00:20:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A 1949AnHar.112....1C HD 293175
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:06:24.13 +00:20:29.6: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:06:24.13 +00:20:29.6: 13.80 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.80 +/- 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 3114263159786050944,2461158.6198,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114263159786050944 20260428.1198 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 28.1198 2461158.6198 11.77 07:19:32.16 -03:36:33.6
219.36481 4.58390 galactic Mon Second-epoch detections are separated by 2.3" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:19:32.16 -03:36:33.6 (user input) | T | P | (position from user input) SpType: A1V (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:19:32.16 -03:36:33.6: 14.44 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:19:32.16 -03:36:33.6: 15.10 +/- 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,2461158.6198,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.96 07:00:56.90 -03:16:15.2
216.92693 0.62133 galactic Mon Second-epoch detections are separated by 2.5" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:00:56.90 -03:16:15.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:00:56.90 -03:16:15.2: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:00:56.90 -03:16:15.2: 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
target,2461158.6198,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.90 07:22:52.24 +01:09:04.4
215.50161 7.51683 galactic CMi Second-epoch detections are separated by 1.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:22:52.24 +01:09:04.4 (user input) | T | P | (position from user input) J-Ks=0.305+/-0.037 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:22:52.24 +01:09:04.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:22:52.24 +01:09:04.4: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.6198,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 11.96 06:22:32.51 -04:26:55.2
213.61926 -8.45004 galactic Mon Second-epoch detections are separated by 1.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3116517433500260224 | 06:22:30.58 -04:26:43.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1949AnHar.112....1C HD 294987
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:22:32.51 -04:26:55.2: 14.61 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:22:32.51 -04:26:55.2: 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 3116517433500260224,2461158.6198,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3116517433500260224 20260428.1198 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.08 06:22:54.82 +02:15:15.6
207.65533 -5.30519 galactic Mon Second-epoch detections are separated by 3.0" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3123804382390994304 | 06:22:54.94 +02:15:42.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M1 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:22:54.82 +02:15:15.6: 12.58 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:22:54.82 +02:15:15.6: 13.31 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3123804382390994304,2461158.6198,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3123804382390994304 20260428.1198 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.26 06:52:57.28 -03:04:53.3
215.84748 -1.06751 galactic Mon Second-epoch detections are separated by 2.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:52:57.28 -03:04:53.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:52:57.28 -03:04:53.3: 14.75 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:52:57.28 -03:04:53.3: 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
target,2461158.6198,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.19 07:13:53.87 -00:07:53.1
215.61604 4.93543 galactic Mon Second-epoch detections are separated by 2.0" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:13:53.87 -00:07:53.1 (user input) | T | P | (position from user input) J-Ks=0.847+/-0.033 (M)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:13:53.87 -00:07:53.1: 14.55 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:13:53.87 -00:07:53.1: 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,2461158.6198,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.09 06:30:25.55 -00:34:50.6
211.04960 -4.93925 galactic Mon Second-epoch detections are separated by 1.4" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3119916333177963648 | 06:30:24.78 -00:35:22.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.418+/-0.033 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:30:25.55 -00:34:50.6: 12.56 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:30:25.55 -00:34:50.6: 13.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119916333177963648,2461158.6198,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119916333177963648 20260428.1198 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.24 06:20:50.77 -04:58:33.6
213.90322 -9.06469 galactic Mon Second-epoch detections are separated by 1.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.2027-04.9838 | 06:20:48.79 -04:58:45.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:20:50.77 -04:58:33.6: 14.56 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:20:50.77 -04:58:33.6: 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 J095.2027-04.9838,2461158.6198,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.2027-04.9838 20260428.1198 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.31 06:23:37.14 +01:59:36.3
207.96946 -5.26935 galactic Mon Second-epoch detections are separated by 4.5" 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 | 06:23:37.14 +01:59:36.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:23:37.14 +01:59:36.3: 12.72 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:23:37.14 +01:59:36.3: 13.58 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.6198,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.19 06:54:29.98 -04:07:28.3
216.95182 -1.19974 galactic Mon Second-epoch detections are separated by 3.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:54:29.98 -04:07:28.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:54:29.98 -04:07:28.3: 14.72 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:54:29.98 -04:07:28.3: 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,2461158.6198,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.37 07:07:58.63 -00:56:38.9
215.66108 3.24749 galactic Mon Second-epoch detections are separated by 5.4" 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 | 07:07:58.63 -00:56:38.9 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:07:58.63 -00:56:38.9: 14.70 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:07:58.63 -00:56:38.9: 14.28 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.6198,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.47 07:05:49.64 +01:33:34.7
213.18327 3.91243 galactic Mon Second-epoch detections are separated by 1.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3114733097928881408 | 07:05:50.24 +01:33:09.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.356+/-0.032 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:05:49.64 +01:33:34.7: 14.65 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:05:49.64 +01:33:34.7: 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 3114733097928881408,2461158.6198,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114733097928881408 20260428.1198 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 28.1198 2461158.6198 12.38 06:57:00.73 +00:17:39.2
213.30555 1.37441 galactic Mon Second-epoch detections are separated by 0.4" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:00.73 +00:17:39.2: 14.93 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:00.73 +00:17:39.2: 15.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113688634901420928,2461158.6198,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113688634901420928 20260428.1198 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 28.1198 2461158.6198 12.49 06:26:10.53 +01:36:50.5
208.60302 -4.87723 galactic Mon Second-epoch detections are separated by 4.0" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:26:10.53 +01:36:50.5 (user input) | T | P | (position from user input) J-Ks=0.910+/-0.031 (M)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:26:10.53 +01:36:50.5: 13.30 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:26:10.53 +01:36:50.5: 13.61 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.51 +/- 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,2461158.6198,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.48 06:39:58.45 -01:44:23.9
213.17497 -3.34359 galactic Mon Second-epoch detections are separated by 2.2" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3106840670323834496 | 06:39:59.15 -01:43:54.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:39:58.45 -01:44:23.9: 14.18 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:39:58.45 -01:44:23.9: 13.28 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.32 +/- 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 3106840670323834496,2461158.6198,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106840670323834496 20260428.1198 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 28.1198 2461158.6198 12.46 06:24:57.34 +02:30:05.5
207.67167 -4.73862 galactic Mon Second-epoch detections are separated by 1.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J096.2316+02.5050 | 06:24:57.34 +02:30:05.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:24:57.34 +02:30:05.5: 13.00 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:24:57.34 +02:30:05.5: 13.37 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.2316+02.5050,2461158.6198,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.2316+02.5050 20260428.1198 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.46 06:24:53.83 -02:34:45.7
212.20546 -7.07983 galactic Mon Second-epoch detections are separated by 5.6" 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 | Gaia DR3 3117366466933708032 | 06:24:55.13 -02:34:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:24:53.83 -02:34:45.7: 12.89 +/- 0.07 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:24:53.83 -02:34:45.7: 14.18 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.23 +/- 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 3117366466933708032,2461158.6198,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3117366466933708032 20260428.1198 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.45 06:32:06.23 +03:17:17.2
207.79641 -2.79221 galactic Mon Second-epoch detections are separated by 0.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:32:06.23 +03:17:17.2 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:32:06.23 +03:17:17.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:32:06.23 +03:17:17.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.6198,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.45 07:02:19.58 -03:20:38.6
217.14937 0.89367 galactic Mon Second-epoch detections are separated by 3.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:02:19.58 -03:20:38.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:02:19.58 -03:20:38.6: 14.83 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:02:19.58 -03:20:38.6: 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
target,2461158.6198,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.46 06:48:48.53 +00:23:30.1
212.28360 -0.40634 galactic Mon Second-epoch detections are separated by 1.6" and 5.2 pix
The object was found in VSX 2" Gaia DR3 3113610294697190784
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.590 G 13.610 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:48:48.53 +00:23:30.1: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:48:48.53 +00:23:30.1: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 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 3113610294697190784,2461158.6198,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113610294697190784 20260428.1198 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.49 06:37:10.38 +03:05:45.9
208.54873 -1.75642 galactic Mon Second-epoch detections are separated by 0.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3127142808931895424 | 06:37:08.27 +03:05:31.7 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=VARIABLE SpType: A 1964PASP...76..165P Cl vdB 1 C
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:37:10.38 +03:05:45.9: 14.56 +/- 0.36 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:37:10.38 +03:05:45.9: 13.41 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127142808931895424,2461158.6198,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127142808931895424 20260428.1198 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 28.1198 2461158.6198 12.59 06:21:53.24 +01:15:50.1
208.41936 -5.98975 galactic Mon Second-epoch detections are separated by 1.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:21:53.24 +01:15:50.1 (user input) | T | P | (position from user input) SpType: A2V (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:21:53.24 +01:15:50.1: 13.63 +/- 0.13 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:21:53.24 +01:15:50.1: 13.35 +/- 0.06 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
target,2461158.6198,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.71 06:21:55.43 -01:41:34.6
211.06909 -7.33769 galactic Mon Second-epoch detections are separated by 2.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J095.4794-01.6935 | 06:21:55.43 -01:41:34.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:21:55.43 -01:41:34.6: 14.23 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:21:55.43 -01:41:34.6: 13.47 +/- 0.06 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
ATO J095.4794-01.6935,2461158.6198,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.4794-01.6935 20260428.1198 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.66 06:28:36.65 +01:48:24.0
208.71227 -4.24826 galactic Mon Second-epoch detections are separated by 2.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J097.1581+01.8183 | 06:28:37.73 +01:48:53.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:28:36.65 +01:48:24.0: 13.76 +/- 0.13 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:28:36.65 +01:48:24.0: 13.80 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.79 +/- 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 J097.1581+01.8183,2461158.6198,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.1581+01.8183 20260428.1198 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 28.1198 2461158.6198 12.53 06:56:36.36 +02:42:47.6
211.10462 2.38591 galactic Mon Second-epoch detections are separated by 3.9" 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 3127764887696264704 | 06:56:35.41 +02:42:58.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:56:36.36 +02:42:47.6: 14.85 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:56:36.36 +02:42:47.6: 15.54 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127764887696264704,2461158.6198,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127764887696264704 20260428.1198 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 28.1198 2461158.6198 12.73 06:25:41.40 +01:28:51.8
208.66547 -5.04614 galactic Mon Second-epoch detections are separated by 0.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3123506341722139904 | 06:25:39.96 +01:28:30.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:25:41.40 +01:28:51.8: 13.16 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:25:41.40 +01:28:51.8: 13.75 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.49 +/- 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 3123506341722139904,2461158.6198,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3123506341722139904 20260428.1198 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 28.1198 2461158.6198 12.66 06:45:54.97 +00:45:36.1
211.62591 -0.88183 galactic Mon Second-epoch detections are separated by 0.9" and 5.4 pix
The object was found in VSX 6" Gaia DR3 3125565662581474304
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
13.790 G 13.810 G F
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:45:54.97 +00:45:36.1: 13.66 +/- 0.14 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:45:54.97 +00:45:36.1: 13.52 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.54 +/- 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 3125565662581474304,2461158.6198,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125565662581474304 20260428.1198 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 28.1198 2461158.6198 12.80 06:40:28.24 +03:16:37.2
208.76508 -0.94186 galactic Mon Second-epoch detections are separated by 2.7" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:40:28.24 +03:16:37.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:40:28.24 +03:16:37.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:40:28.24 +03:16:37.2: 99.00 +/- 99.00 edge
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.6198,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.84 06:34:44.91 +01:53:00.9
209.34927 -2.85051 galactic Mon Second-epoch detections are separated by 4.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J098.6851+01.8816 | 06:34:44.27 +01:52:30.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:34:44.91 +01:53:00.9: 13.20 +/- 0.08 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:34:44.91 +01:53:00.9: 13.73 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.51 +/- 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 J098.6851+01.8816,2461158.6198,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.6851+01.8816 20260428.1198 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 28.1198 2461158.6198 13.07 06:22:06.26 +03:13:15.8
206.70092 -5.03706 galactic Mon Second-epoch detections are separated by 1.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:22:06.26 +03:13:15.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:22:06.26 +03:13:15.8: 13.75 +/- 0.16 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:22:06.26 +03:13:15.8: 14.29 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.06 +/- 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,2461158.6198,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 11.49 06:22:44.95 +01:50:00.9
208.01116 -5.53591 galactic Mon Second-epoch detections are separated by 0.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3123727755875769728 | 06:22:44.96 +01:49:58.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5) J-Ks=0.252+/-0.032 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:22:44.95 +01:50:00.9: 12.05 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:22:44.95 +01:50:00.9: 12.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3123727755875769728,2461158.6198,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3123727755875769728 20260428.1198 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 28.1198 2461158.6198 12.19 06:57:00.74 -04:49:23.0
217.85922 -0.96091 galactic Mon Second-epoch detections are separated by 4.0" 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 J104.2548-04.8290 | 06:57:00.74 -04:49:23.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.296+/-0.033 (F)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:57:00.74 -04:49:23.0: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:57:00.74 -04:49:23.0: 13.62 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.62 +/- 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 J104.2548-04.8290,2461158.6198,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2548-04.8290 20260428.1198 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3124968142433583232,2461158.6198,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3124968142433583232 20260428.1198 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 28.1198 2461158.6198 12.21 06:21:22.28 +01:19:22.4
208.30695 -6.07700 galactic Mon Second-epoch detections are separated by 0.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:21:22.28 +01:19:22.4 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.035 (G)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:21:22.28 +01:19:22.4: 13.43 +/- 0.12 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:21:22.28 +01:19:22.4: 14.03 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.6198,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.34 06:22:45.78 +01:17:39.0
208.49376 -5.78157 galactic Mon Second-epoch detections are separated by 2.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:22:45.78 +01:17:39.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.483+/-0.035 (K)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:22:45.78 +01:17:39.0: 13.43 +/- 0.11 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:22:45.78 +01:17:39.0: 13.86 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.6198,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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 28.1198 2461158.6198 12.08 07:12:53.88 -06:13:46.5
220.92391 1.90503 galactic Mon Second-epoch detections are separated by 3.0" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:12:53.88 -06:13:46.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:12:53.88 -06:13:46.5: 13.70 +/- 0.17 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:12:53.88 -06:13:46.5: 15.18 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.70 +/- 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
target,2461158.6198,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1198 2461158.6198 12.21 06:27:21.55 +02:34:18.4
207.88688 -4.17361 galactic Mon Second-epoch detections are separated by 2.4" and 5.6 pix
The object was found in VSX13" Gaia DR3 3124249405426523008
Type: RS
# Max. Min./Amp. JD0 Period
16.230 G 16.320 G K
The object was not found in astcheck.
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:27:21.55 +02:34:18.4: 14.12 +/- 0.20 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:27:21.55 +02:34:18.4: 13.37 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.42 +/- 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 3124249405426523008,2461158.6198,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3124249405426523008 20260428.1198 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461158.6198,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AK Mon 20260428.1198 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461158.6198,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260428.1198 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
## 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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Last image: 2461158.62009587 28.04.2026 02:52:46.283 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.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.: -7.96
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: 15 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): 34854
Objects passed selection criteria: 34685
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 24733.5
Average stars matched: 24164 (97.6975 %)
Memory usage VmPeak: 136956 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 Mon Apr 27 22:04:39 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461120.60986138 21.03.2026 02:38:02.023 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Last image: 2461158.62009587 28.04.2026 02:52:46.283 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 379
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.69
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: 450 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): 205158
Objects passed selection criteria: 204698
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 161099
Average stars matched: 155656 (96.6216 %)
Memory usage VmPeak: 2088204 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 Mon Apr 27 22:19:03 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.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: 2461158.61942259
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits'
wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (1st reference image)
verification OK: wcs_Mon-02-Q1b1x1_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-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
Image size: 941.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:13.283 -01:56:48.95 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 06:51:13.283 -01:56:48.95
Angular distance between the image centers 0.0324 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
Image size: 941.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:11.325 -01:57:00.98 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 06:51:11.325 -01:57:00.98
Angular distance between the image centers 0.0346 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 06:51:13.283 -01:56:48.95
Second-epoch second image center 06:51:11.325 -01:57:00.98
Angular distance between the image centers 0.00881 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.cfunPluSaR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.CkCYiWPUYG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits &> /tmp/tmp.Sv4tnYoKxc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits &> /tmp/tmp.ZrQUtIclhz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits) and catalog (wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat) found
'wcs_Mon-02-Q1b1x1_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 22.838347
a=0.000000 b=1.000000 c=22.838347
From vast_summary.log: estimated ref. image limiting mag.: -7.96
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.88
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.88
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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -> calib.txt_param_ref_wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (aperture=6.5)
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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits (aperture=6.5)
____ 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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.5 pix Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
2.5 pix fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
2.5 pix fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
2.4 pix wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.5 pix wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Limiting magnitude estimates:
14.9 mag. Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
14.9 mag. Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
13.7 mag. fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
13.7 mag. fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.cfunPluSaR (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 437 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 321 matched stars entering correct_measured_positions(), 247 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 320 matched stars entering correct_measured_positions(), 9301 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.22"
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 470 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 376 matched stars entering correct_measured_positions(), 9339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.15"
Accuracy estimation diagnostic: 373 matched stars entering correct_measured_positions(), 11855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.97"
Excluding outliers - 373 stars left (next iteration limit 352)
The image catalog is written to wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Mon-02-Q1b1x1_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-Q1b1x1_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.CkCYiWPUYG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 636 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 577 matched stars entering correct_measured_positions(), 512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 577 matched stars entering correct_measured_positions(), 17754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.14"
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 686 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 643 matched stars entering correct_measured_positions(), 17768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.05"
Accuracy estimation diagnostic: 639 matched stars entering correct_measured_positions(), 19113 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.75"
Excluding outliers - 639 stars left (next iteration limit 634)
The image catalog is written to wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Mon-02-Q1b1x1_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-Q1b1x1_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.Sv4tnYoKxc (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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1148, passed=13286
Got 13286 stars (including 12123 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat
util/solve_plate_with_UCAC5 got 13286 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.8)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 12942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.8)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 12943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 12943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 933 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.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.ZrQUtIclhz (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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1112, passed=13218
Got 13218 stars (including 12091 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat
util/solve_plate_with_UCAC5 got 13218 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.8)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 12817 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.6 to 3.8)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 12814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 12814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 932 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits'
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52224.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 22s
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 51804_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 51804_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:17.05 +01:29:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.68, MAG_FAINT_SEARCH_LIMIT=11.66)GAIADR2_OUTPUT=# 1.175 3114511825510240128 107.57076222618 +01.49863681537 10.7072 9.9163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51954_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 51954_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:32:47.70 +03:17:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.21, MAG_FAINT_SEARCH_LIMIT=11.19)GAIADR2_OUTPUT=# 1.228 3130130143366555904 098.19884020933 +03.28611531056 10.2196 9.9595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51957_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 51957_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:17.11 +01:47:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.27, MAG_FAINT_SEARCH_LIMIT=11.25)GAIADR2_OUTPUT=# 0.755 3114743577647582208 106.82108278725 +01.79170244015 10.6530 10.6029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52058_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 52058_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:30.00 -04:27:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.69, MAG_FAINT_SEARCH_LIMIT=11.67)GAIADR2_OUTPUT=# 1.623 3104516062223185664 096.12473929750 -04.46042407041 10.6488 9.9317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52224_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 52224_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:39:40.40 +03:07:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 4.797 3127154486945506816 099.91894652190 +03.11987803650 11.9650 11.6781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06854_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 06854_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:31.10 +01:05:37.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 23s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (1st reference image)
verification OK: wcs_Mon-02-Q1b1x1_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-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
Image size: 941.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:13.283 -01:56:48.95 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 06:51:13.283 -01:56:48.95
Angular distance between the image centers 0.0324 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
Image size: 941.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:11.325 -01:57:00.98 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 06:51:11.325 -01:57:00.98
Angular distance between the image centers 0.0346 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 06:51:13.283 -01:56:48.95
Second-epoch second image center 06:51:11.325 -01:57:00.98
Angular distance between the image centers 0.00881 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.dX6EEHfk38
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.WjluywR4hM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits &> /tmp/tmp.u71kuCwZpq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits &> /tmp/tmp.3mBAEzvIB3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits and wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits) and catalog (wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat) found
'wcs_Mon-02-Q1b1x1_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 21.882709
a=0.000000 b=1.000000 c=21.882709
From vast_summary.log: estimated ref. image limiting mag.: -7.69
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.19
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.19
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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -> calib.txt_param_ref_wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits (aperture=5.1)
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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 338 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.4 pix Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
2.4 pix fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
2.4 pix fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
2.3 pix wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
2.4 pix wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Limiting magnitude estimates:
14.2 mag. Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
14.2 mag. Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
13.0 mag. fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
13.0 mag. fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 12.4 (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.dX6EEHfk38 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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=41, blended=38776, passed=220681
Got 220681 stars (including 181688 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 220681 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 420 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 314 matched stars entering correct_measured_positions(), 234 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.11"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 310 matched stars entering correct_measured_positions(), 49147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.24"
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 454 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(), 49178 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.24"
Accuracy estimation diagnostic: 365 matched stars entering correct_measured_positions(), 65991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 8.83"
Excluding outliers - 365 stars left (next iteration limit 341)
The image catalog is written to wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Mon-02-Q1b1x1_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-Q1b1x1_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.WjluywR4hM (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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=31, blended=38902, passed=220463
Got 220463 stars (including 181343 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 220463 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: 560 matched stars entering correct_measured_positions(), 492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.14"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 558 matched stars entering correct_measured_positions(), 100800 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.71"
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: 623 matched stars entering correct_measured_positions(), 100821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.69"
Accuracy estimation diagnostic: 622 matched stars entering correct_measured_positions(), 116754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.82"
Excluding outliers - 622 stars left (next iteration limit 613)
The image catalog is written to wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Mon-02-Q1b1x1_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-Q1b1x1_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.u71kuCwZpq (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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=10237, passed=105198
Got 105198 stars (including 94820 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat
util/solve_plate_with_UCAC5 got 105198 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 471 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 103952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 471 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 103957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 103957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 933 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.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.3mBAEzvIB3 (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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=9849, passed=102200
Got 102200 stars (including 92210 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat
util/solve_plate_with_UCAC5 got 102200 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 100958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 471 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 100957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 100957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 932 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-51-48_20.00sec_-5.00C_LIGHTs_0029.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-27_CI_Mon-02-Q1b1x1_215342_TTUQ1b1x1_3463020_ba4SB2rK/wcs_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030.fits
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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__out04797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out07633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out11910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out231285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out231666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out231870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out24010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248956.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out250997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out251012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out251196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out251202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out251212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out251286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out251338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out251429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out40050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out42576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out42663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out06227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out231699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out231888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out249953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out250990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out251844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50933.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 857s
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: 52s
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Considering the candidate 248674_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248674_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:57:53.50 +01:02:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.406 3113890738881890304 104.47260089386 +01.03391094910 13.7975 13.4673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248685_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248685_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:29:04.54 +02:46:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248703_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248703_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248709_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248709_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248717_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248717_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248723_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248723_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248728_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248728_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 248736_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248736_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:30:54.05 +00:23:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.651 3120143043029397504 097.72548621068 +00.38582943364 13.4480 12.9041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248744_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248744_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:55:04.30 +01:01:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.546 3113996188918170624 103.76812450097 +01.03036562985 13.3729 12.4930 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248746_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248746_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:34:59.04 +02:18:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248747_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248747_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 248749_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248749_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248756_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248756_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:25:55.59 -03:05:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 3.764 3117142235280599936 096.48210324737 -03.09281896036 13.2284 12.7027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248761_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248761_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:34:11.77 -06:40:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248767_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248767_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:35:07.40 -03:03:02.9: 14.84 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:35:07.40 -03:03:02.9: 12.68 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.03
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Considering the candidate 248771_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248771_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:54.39 +00:24:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 4.357 3125538071712188032 101.47752985583 +00.41555722494 13.2647 12.4139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248773_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248773_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:21.28 -00:56:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.307 3119888162491054464 096.83844388456 -00.93682310505 13.1792 12.7100 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 248774_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248774_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:33.56 -05:37:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.933 3100991195446532736 104.88952340554 -05.62403198437 13.0176 12.5700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248776_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248776_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248777_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248777_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:25:43.21 -01:22:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 3.939 3118349322951154944 096.43040852203 -01.38266988268 13.1240 12.8485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248781_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248781_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:16.11 -02:52:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 3.992 3117141268909843456 096.81714043301 -02.87952534417 12.6169 11.6289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248791_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248791_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248794_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248794_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248800_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248800_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:41:00.31 +01:31:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 4.069 3125909088165152512 100.25148907420 +01.52108155709 13.0371 12.1796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248802_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248802_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248804_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248804_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248805_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248805_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:41:50.99 -01:29:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 2.738 3107222578817255040 100.46257646404 -01.49991807461 13.0180 12.6381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248806_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248806_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:53.60 +01:58:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 2.089 3125987939465644416 101.47341418875 +01.96834205219 13.0198 12.6427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248807_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248807_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:33:59.82 +01:45:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.546 3120911322481431936 098.49950014419 +01.75665840777 12.7992 11.9050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248811_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248811_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:35.72 +02:18:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 2.901 3126420184974980352 101.64920022722 +02.30722679378 13.0302 12.1880 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#
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Considering the candidate 248819_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248819_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:24.25 -06:59:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248824_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248824_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:56.87 -06:07:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248826_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248826_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248827_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248827_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 248829_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248829_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:10.32 -05:02:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248830_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248830_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:50.16 -06:14:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 1.835 3053053695369233536 107.95934833861 -06.23717944162 13.0158 12.5248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248831_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248831_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:38.72 +02:08:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 3.702 3126190734942256384 102.41140657414 +02.14275210285 13.0825 12.6575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248835_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248835_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:23.27 -06:18:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248836_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248836_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:36.75 +02:52:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248838_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248838_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248840_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248840_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:11.72 +01:02:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248843_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248843_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248846_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248846_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:32.15 -04:39:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248847_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248847_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:39.39 +00:09:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 2.752 3119555044829350784 100.66420572211 +00.15393415763 13.0766 12.6074 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 248848_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248848_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:02.08 +01:19:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248853_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248853_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:42.99 +03:02:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 3.195 3126570238251850112 102.42920394949 +03.04497718214 13.0964 12.6386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248856_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248856_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248857_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248857_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248860_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248860_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:24.36 +02:38:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 4.694 3124207353403229568 096.60133517935 +02.63367868492 12.8884 12.3056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248862_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248862_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:02.49 +01:07:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248863_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248863_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248864_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248864_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:51:33.26 +02:05:19.8: 14.49 +/- 0.30 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:51:33.26 +02:05:19.8: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.02
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Considering the candidate 248865_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248865_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248866_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248866_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:08.12 -05:53:01.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248869_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248869_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:24.57 -04:54:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248870_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248870_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248872_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248872_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:13.29 -00:19:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248875_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248875_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:28:10.34 +00:28:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 2.211 3120323878334356864 097.04301929435 +00.46997264023 12.8985 12.3984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248876_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248876_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:57.55 +00:44:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248878_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248878_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:38.23 +01:13:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248879_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248879_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:24.05 +01:22:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 3.517 3114102218772312704 104.10002976772 +01.37115075284 12.7076 11.9544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248881_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248881_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:09.24 +00:34:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.664 3113585005929929984 103.03834255055 +00.57848204790 12.7509 11.9519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248882_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248882_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:31:44.17 +02:19:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 3.471 3124003737594234112 097.93421866346 +02.31894121745 12.7129 12.3528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248883_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248883_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:12.29 -03:41:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 3.255 3116629141306773632 095.55087699549 -03.69111939156 12.5883 12.0407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248886_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248886_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:42.95 -05:31:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.898 3053375852277606400 106.42947623677 -05.53038847122 12.7258 12.0098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248887_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248887_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:34.78 +03:03:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248888_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248888_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:48.98 +01:04:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248889_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248889_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:20.11 +02:12:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248890_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248890_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248893_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248893_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:33:39.56 -04:17:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 3.226 3104702356426628992 098.41476641393 -04.28756035562 12.5318 11.7509 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 248895_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248895_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 248896_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248896_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:38:12.42 +00:44:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248897_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248897_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:45.12 +02:12:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 3.703 3115663971961467264 104.93780112879 +02.20801858093 12.7631 12.4648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248899_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248899_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:07.39 -01:01:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 3.750 3118608159158686848 095.53063777983 -01.01814139744 12.7302 12.2009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248900_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248900_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:41.38 -06:04:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248901_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248901_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:30:32.02 +01:34:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 2.343 3120843535017204992 097.63310652797 +01.57317770479 12.4953 11.5274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248903_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248903_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:01:37.06 -04:14:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 5.367 3101747972982311552 105.40574746029 -04.24506783820 12.7532 12.0169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248905_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248905_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248906_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248906_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:33.16 +00:36:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 4.126 3119819408654913152 099.38863803077 +00.60489964142 12.7958 12.2404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248908_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248908_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:22.31 +02:53:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 2.773 3126340852638302208 103.34266454132 +02.89362107197 12.7107 12.4047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248911_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248911_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:39:13.97 -00:00:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.319 3119633999207612288 099.80793936405 -00.00911312420 12.2573 11.1859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248912_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248912_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:30:26.74 +02:32:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 2.538 3124061290155460608 097.61144438808 +02.53499006566 11.7058 10.4596 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#
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Considering the candidate 248914_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248914_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:36:38.15 +00:49:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248915_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248915_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:49.70 +01:05:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 2.746 3114600881653061376 105.95718131582 +01.09466021958 12.6217 12.1501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248920_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248920_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:48.56 +02:23:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 3.060 3115174521784855552 107.20244186956 +02.39154584664 12.5442 11.8041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248921_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248921_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:31:17.29 -04:38:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 0.888 3104355048190428800 097.82213440917 -04.63795101070 12.4437 11.9313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248922_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248922_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:44:55.66 +02:40:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 3.686 3127195718630485760 101.23188430493 +02.66628225100 12.6756 12.3243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248923_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248923_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:35.70 -00:13:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 1.661 3120174821489528576 096.14863871658 -00.22886437423 12.1222 11.2822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248924_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248924_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:30:06.03 +01:52:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 3.194 3123861174741853824 097.52553551119 +01.86876882140 12.3556 11.8113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248925_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248925_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:23.33 -01:12:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 3.663 3118404951367552384 096.09722628480 -01.20248964363 12.3781 11.7166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248926_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248926_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:03.27 -02:17:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.311 3108998320154606464 104.76311203704 -02.29796996872 12.4004 11.6148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248929_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248929_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248930_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248930_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:26.19 +00:44:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248931_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248931_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:32:43.41 -05:34:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248934_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248934_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:11.65 +00:30:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248935_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248935_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:21.28 +02:14:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 3.048 3115156963958576256 107.33847751877 +02.23567456553 12.4681 12.0482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248937_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248937_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:35.86 +01:32:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248939_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248939_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:02.94 +02:51:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 1.962 3127220010965515904 101.26230554041 +02.85029127039 12.2976 11.5567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248941_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248941_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:44:09.08 +01:49:47.6: 14.81 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:09.08 +01:49:47.6: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.01
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Considering the candidate 248942_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248942_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:02:29.52 +02:56:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248943_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248943_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:21:50.60 +00:06:45.1: 12.49 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:21:50.60 +00:06:45.1: 11.68 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.72 +/- 0.01
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Considering the candidate 248946_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248946_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:29:43.41 -05:15:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248951_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248951_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:19.21 -03:13:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 3.736 3116984107467073920 095.33040827698 -03.23166562821 12.2511 11.8559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248952_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248952_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:57:05.78 +01:24:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 2.376 3114108059926391040 104.27346090126 +01.41316855347 12.1037 11.3783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248953_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248953_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:17.64 +01:47:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248955_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248955_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:06.57 -03:25:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 2.517 3116840586838020736 095.27741913764 -03.42508664379 12.0580 11.3332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248956_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248956_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:20:30.43 -01:20:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 2.467 3118502262445067904 095.12670599267 -01.33956872448 11.9975 11.5311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248957_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248957_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:07.15 -07:00:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248959_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248959_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248962_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248962_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248964_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248964_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248965_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248965_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:26.14 -06:06:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248967_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 248967_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 248968_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248968_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:36.30 -04:17:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 2.175 3116524168008979840 095.65141131398 -04.28861021971 11.6231 10.8651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248970_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248970_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:33.30 -04:58:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248971_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248971_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:24.38 +01:15:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248974_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248974_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:33.80 -06:18:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248975_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248975_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:50.51 +01:11:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248976_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248976_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:55:49.30 +02:46:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248978_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248978_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:40:44.30 +02:31:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.28, MAG_FAINT_SEARCH_LIMIT=11.26)GAIADR2_OUTPUT=# 0.807 3126866655417089792 100.18447903099 +02.52907927769 10.2604 9.0665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248979_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248979_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:53.83 -03:37:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.26, MAG_FAINT_SEARCH_LIMIT=11.24)GAIADR2_OUTPUT=# 2.327 3116724249063340800 095.72445018313 -03.62351568513 11.0480 10.4830 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 248982_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248982_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:46.36 +02:38:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248983_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248983_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:26.57 +01:11:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248984_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248984_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:17.06 +01:29:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.86, MAG_FAINT_SEARCH_LIMIT=10.84)GAIADR2_OUTPUT=# 1.469 3114511825510240128 107.57076222618 +01.49863681537 10.7072 9.9163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 248985_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 248985_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:22:36.71 +01:09:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249127_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249127_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:32:47.70 +03:17:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.45, MAG_FAINT_SEARCH_LIMIT=10.43)GAIADR2_OUTPUT=# 1.422 3130130143366555904 098.19884020933 +03.28611531056 10.2196 9.9595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249151_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 249151_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 249183_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249183_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:52.65 +03:09:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249233_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249233_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:29.97 -04:27:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.95, MAG_FAINT_SEARCH_LIMIT=10.93)GAIADR2_OUTPUT=# 1.320 3104516062223185664 096.12473929750 -04.46042407041 10.6488 9.9317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249247_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249247_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:36.57 +03:14:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.08, MAG_FAINT_SEARCH_LIMIT=11.06)GAIADR2_OUTPUT=# 3.212 3125048372421454848 095.65273992730 +03.23304658101 10.9340 10.4801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249342_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249342_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:34.50 +02:28:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.39, MAG_FAINT_SEARCH_LIMIT=11.37)GAIADR2_OUTPUT=# 1.154 3124936123454402176 095.64373097581 +02.47351334742 11.2055 10.7313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249373_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249373_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:33.31 -05:56:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249421_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249421_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:30:09.76 +02:51:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 2.933 3124275763642323456 097.54106658012 +02.86295651709 11.4969 11.2133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249438_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249438_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:30.78 +03:16:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.52, MAG_FAINT_SEARCH_LIMIT=11.50)GAIADR2_OUTPUT=# 2.064 3127306361288156032 101.37827611184 +03.26687173214 11.1083 10.2952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249457_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249457_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:43.14 +03:17:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.61, MAG_FAINT_SEARCH_LIMIT=11.59)GAIADR2_OUTPUT=# 1.551 3125097201907653888 096.17952338142 +03.29118897745 11.1100 10.2922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249475_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249475_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:36:50.61 +02:39:06.0: 12.41 +/- 0.04 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:36:50.61 +02:39:06.0: 11.11 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.14 +/- 0.01
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Considering the candidate 249509_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 249509_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 249586_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249586_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:55.00 +00:33:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249646_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249646_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:01.73 -05:27:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249665_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249665_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:46.39 -01:47:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 2.376 3118227487616653696 096.19309580556 -01.78546359999 11.7468 11.3648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249758_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 249758_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 249852_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249852_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:48.91 +03:04:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 2.345 3124341489524536832 096.95386515440 +03.07604713453 11.9588 11.3947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 249885_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249885_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:10.70 +01:53:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249917_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249917_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:39:00.19 +01:56:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249921_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 249921_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 249953_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 249953_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 249964_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 249964_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:16.75 +02:09:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250018_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250018_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:16.89 -02:24:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250064_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250064_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:44:53.88 +02:41:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250067_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250067_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:05.49 +00:44:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250078_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250078_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250112_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250112_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:15.86 -05:27:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250118_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250118_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:44:55.18 +01:43:59.5: 12.33 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:55.18 +01:43:59.5: 11.79 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.83 +/- 0.01
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Considering the candidate 250122_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250122_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:36.78 +00:50:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 1.928 3120395754609202432 096.65323164964 +00.83699259619 12.3172 11.7704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250123_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250123_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:43:38.85 +03:16:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 3.293 3127292441295623680 100.91198513718 +03.26967521483 12.2987 11.8841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250130_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250130_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:27:27.06 +01:11:15.7: 10.56 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:27:27.06 +01:11:15.7: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.76 +/- 0.01
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Considering the candidate 250131_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250131_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:14.98 +01:44:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 3.236 3123890075579240320 096.81270479471 +01.74878738407 12.4627 11.9763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250137_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250137_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:33:06.43 +01:14:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 4.119 3120764095302536320 098.27668814582 +01.24558265169 12.4587 11.9747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250156_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250156_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:47.05 -00:50:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 2.297 3118617225829997184 095.69590518347 -00.84742897272 12.1740 11.3883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250168_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250168_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:20:50.77 -02:56:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 3.109 3117005204351825920 095.21167292767 -02.93640902133 12.5787 11.8120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250174_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250174_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250176_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250176_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250191_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250191_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250194_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250194_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:20.27 -01:34:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 1.371 3118893104469502592 099.33473063189 -01.57021074993 12.3993 11.5750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250201_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250201_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:27.32 +01:26:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250220_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250220_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:35:58.34 -01:03:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 2.477 3118994804996036992 098.99297754764 -01.05256885649 12.5494 12.0660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250243_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250243_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:43.35 +02:22:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250264_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250264_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:04.76 -05:42:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 2.267 3008193208631841920 095.26969520729 -05.71566998985 12.5375 11.9419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250276_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250276_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:02:00.71 +01:40:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250289_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250289_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:26:29.86 +00:40:37.5: 12.08 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:26:29.86 +00:40:37.5: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.02
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Considering the candidate 250296_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250296_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:36:41.02 -05:13:19.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 250302_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250302_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:41.89 -01:43:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.754 3106304276146697728 102.42464614919 -01.72289255606 12.6059 11.8271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250304_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250304_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250309_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250309_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:34:10.24 -00:59:28.5: 11.45 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:34:10.24 -00:59:28.5: 12.52 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.85 +/- 0.01
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Considering the candidate 250326_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250326_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:29:09.45 -05:33:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250331_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250331_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:08.98 +02:02:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250338_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250338_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:34:16.08 -00:47:45.4: 11.82 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:34:16.08 -00:47:45.4: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.02
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Considering the candidate 250343_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250343_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250365_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250365_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:38:39.41 -01:31:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 4.147 3106905262331173632 099.66491829980 -01.52429610039 12.4571 11.4111 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#
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Considering the candidate 250378_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250378_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:40:59.63 +00:10:05.6: 14.40 +/- 0.24 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:40:59.63 +00:10:05.6: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.02
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Considering the candidate 250381_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250381_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:35.20 +02:08:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 2.926 3126413587904481024 101.64649901088 +02.14737146485 12.4455 11.6476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250385_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250385_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:11.70 -01:59:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250395_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250395_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:53.77 +02:20:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250402_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250402_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:01.76 -04:00:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 3.155 3116594369251745792 095.25675509571 -04.01329854486 12.4374 11.6884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250404_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250404_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:41.99 +03:01:20.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 250434_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250434_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250444_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250444_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:00:33.11 +02:31:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250457_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250457_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250459_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250459_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:08.08 +01:43:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 3.033 3123889933841657216 096.78338712030 +01.72806638578 12.4753 11.6110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250474_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250474_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:21:07.58 +00:00:04.9: 14.03 +/- 0.19 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:21:07.58 +00:00:04.9: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.02
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Considering the candidate 250479_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250479_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250486_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250486_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:33.49 -04:45:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250490_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250490_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:34.24 +00:45:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 3.064 3123346332718185344 095.39283471344 +00.75716570291 12.5189 11.5521 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 250498_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250498_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:39.14 -03:44:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250500_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250500_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:35:12.62 +03:04:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 3.667 3130065001599482368 098.80286701115 +03.07360501401 12.7654 12.3780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250515_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250515_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:05.01 -01:36:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 3.338 3118294484807385728 095.77105015332 -01.61032713033 12.7703 12.2774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.338#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250533_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250533_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:29:40.83 -03:31:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.188 3105047843593789056 097.42031958439 -03.53218350145 12.3976 11.5672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250537_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250537_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:20.28 -06:31:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250548_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250548_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250552_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250552_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:00.45 +02:38:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 2.972 3124955326250621696 095.50210923806 +02.64740261874 12.5604 12.1035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250555_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250555_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:51.43 -04:38:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250561_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250561_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:08.16 -04:35:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 3.687 3102106791729894272 103.28369873380 -04.59861811590 12.6605 12.1037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250577_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250577_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:44:33.46 -01:39:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 5.215 3107031126354300032 101.14073851257 -01.66087173871 12.8835 12.1345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250582_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250582_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:46:11.32 +01:58:09.5: 14.77 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:46:11.32 +01:58:09.5: 12.67 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.03
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Considering the candidate 250587_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250587_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:30:33.72 +01:43:56.4: 11.66 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:30:33.72 +01:43:56.4: 13.05 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.02
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Considering the candidate 250607_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250607_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250620_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250620_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:25:19.09 -02:06:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 2.389 3117449578840863616 096.32955013751 -02.11216369272 12.2289 11.1765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250622_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250622_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:29:04.19 +03:16:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250628_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250628_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250630_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250630_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:11.17 -05:09:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250632_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250632_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:41:59.30 +02:35:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250644_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250644_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250649_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250649_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:53.29 -05:36:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250654_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250654_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250657_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250657_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:38:26.41 +03:16:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 3.238 3127174660409232000 099.61010471476 +03.27940825298 12.8633 12.4456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250677_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250677_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:30:34.29 -01:06:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 3.771 3119134172392234880 097.64253952744 -01.10732560499 12.9977 12.4676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250681_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250681_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:52.86 +02:53:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 4.492 3124309023868842112 096.72061389882 +02.88327857815 12.8832 12.3118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250697_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250697_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:29:58.64 +01:50:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 2.804 3123859564131743616 097.49458859140 +01.83709749230 13.0557 12.6392 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250703_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250703_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:21:48.88 +01:53:56.8: 12.69 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:21:48.88 +01:53:56.8: 12.75 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.03
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Considering the candidate 250708_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250708_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:12.92 -01:34:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250712_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250712_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:48.45 -00:02:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 1.752 3120229109876133248 095.95181755751 -00.03481660213 12.9137 12.4243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250719_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250719_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:04.34 +01:10:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250744_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250744_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:04.77 +00:12:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 2.900 3123256275844422912 095.76938556187 +00.21033242062 12.6177 11.8084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250750_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250750_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:09.40 -05:52:25.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 250767_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250767_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:58.06 +03:13:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 3.588 3124345204673161600 096.99205727455 +03.22659657395 13.0024 12.4934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250786_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250786_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:18.82 +03:10:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 3.595 3124334621873602944 096.57798218595 +03.16776731049 12.7307 12.1738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250791_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250791_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:43:22.17 +03:08:18.3: 12.12 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:22.17 +03:08:18.3: 12.50 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.02
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Considering the candidate 250798_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250798_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250805_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250805_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:10.48 -02:58:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 1.762 3116996202094970880 095.54359426635 -02.96962291745 12.8456 12.3477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250817_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250817_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:25:18.56 -00:35:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 3.863 3118461236915966080 096.32762234728 -00.59914448554 13.1251 12.6126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250823_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250823_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:30.85 -00:36:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.534 3118637158777592320 095.62842358438 -00.60818715532 12.8739 12.3828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250828_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250828_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:28:21.44 -03:50:04.7: 14.70 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:28:21.44 -03:50:04.7: 12.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.03
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Considering the candidate 250838_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250838_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:25:02.61 -00:31:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 4.588 3120151495527205504 096.26114476413 -00.53424556472 12.7732 11.9458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250841_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250841_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:35:16.27 -04:45:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.448 3103909715920100864 098.81776045801 -04.76603712068 12.8544 12.1285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250849_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250849_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:31:00.85 +00:54:11.8: 12.68 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:31:00.85 +00:54:11.8: 13.56 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.04
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Considering the candidate 250859_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250859_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:03.87 +02:19:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.866 3124557754015463936 095.51635352643 +02.32039673035 12.7866 11.7439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250865_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250865_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:34:11.00 -00:21:48.0: 11.75 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:34:11.00 -00:21:48.0: 12.40 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
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Considering the candidate 250870_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250870_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:20:58.63 -04:26:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 2.026 3116561654485044736 095.24410862340 -04.43739340267 12.7797 12.3830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250897_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250897_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:40:54.93 -00:31:59.5: 13.48 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:40:54.93 -00:31:59.5: 12.72 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.03
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Considering the candidate 250912_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250912_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:20:39.65 -01:23:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 4.336 3118501124274367104 095.16572793169 -01.39214209648 12.8505 12.2049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250917_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250917_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:59.09 +03:16:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 3.417 3127480840039702144 100.74626646809 +03.27049709040 12.9793 12.5639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250926_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250926_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:43:35.22 -01:19:39.6: 12.74 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:35.22 -01:19:39.6: 12.98 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
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Considering the candidate 250940_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250940_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:09.68 -03:11:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 3.420 3116930270055073280 095.79067308598 -03.18827612738 13.0664 12.6289 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 250945_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250945_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:29:36.58 +02:17:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 4.507 3124027235358636928 097.40239131721 +02.28791493777 13.1086 12.6717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250946_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250946_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:58.37 -01:25:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 3.594 3118919183510887040 099.49400345973 -01.42388158330 12.8781 12.2501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250950_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250950_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:59.05 -01:56:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 2.674 3118212094454247424 095.49651627201 -01.93465502195 12.9557 12.1112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250955_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250955_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250961_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250961_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:39:03.52 +02:15:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 1.515 3126762068671414016 099.76480933457 +02.25288170162 12.9715 12.0770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 250970_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250970_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250990_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 250990_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 250991_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250991_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:26.12 +01:37:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250997_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 250997_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:07.36 +00:15:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 3.516 3120266257052470400 096.53097334990 +00.25529490151 13.1364 12.5768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 251012_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251012_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:02:39.65 -04:37:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 3.403 3101534633371804672 105.66529147356 -04.63116397367 12.8393 12.0875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 251035_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251035_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:43:00.60 +00:23:42.2: 14.37 +/- 0.25 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:00.60 +00:23:42.2: 12.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.03
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Considering the candidate 251054_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251054_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:37:29.68 +01:45:47.6: 12.07 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:37:29.68 +01:45:47.6: 12.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.02
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Considering the candidate 251084_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251084_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251124_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251124_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251141_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251141_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251153_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251153_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:44:31.49 +00:07:36.3: 14.69 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:44:31.49 +00:07:36.3: 13.16 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.05
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Considering the candidate 251157_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251157_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251166_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251166_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:39:25.90 -02:50:59.1: 12.06 +/- 0.03 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:39:25.90 -02:50:59.1: 12.75 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.02
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Considering the candidate 251171_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251171_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:40:13.53 +01:34:07.3: 12.71 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:40:13.53 +01:34:07.3: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
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Considering the candidate 251187_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251187_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:44.17 +02:41:00.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 251195_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251195_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:26:20.64 -03:09:53.0: 10.83 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:26:20.64 -03:09:53.0: 14.09 +/- 0.11 detection
Forced photometry reference-image weighted average: 10.86 +/- 0.01
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Considering the candidate 251196_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251196_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:44.54 -01:00:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.515 3118422754009128704 095.93564713393 -01.01455474343 13.2187 12.7614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 251202_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251202_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:46.49 -06:35:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 3.764 3099461675990326400 101.94351256233 -06.58947165956 12.9937 12.1472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 251212_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251212_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:20:29.12 -02:05:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 4.099 3117875506456271360 095.12199878096 -02.09261883113 13.1275 12.6159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 251227_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251227_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:20:29.37 -02:05:09.4: 13.15 +/- 0.10 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:20:29.37 -02:05:09.4: 12.95 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.04
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Considering the candidate 251241_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251241_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:04.83 -01:02:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251263_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251263_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 07:01:32.45 -05:17:13.9: 13.43 +/- 0.11 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 07:01:32.45 -05:17:13.9: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.03
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Considering the candidate 251286_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251286_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:20:44.73 -01:54:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 3.063 3118256315437038080 095.18653475231 -01.90769691307 13.2954 12.7666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 251319_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251319_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:39:04.45 +02:33:51.4: 11.78 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:39:04.45 +02:33:51.4: 13.01 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.02
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Considering the candidate 251338_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251338_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:33:37.03 +03:17:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 3.706 3130127841264085376 098.40444445605 +03.28584292741 12.9938 12.4710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 251345_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251345_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:43:50.39 -01:04:07.2: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:43:50.39 -01:04:07.2: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.03
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Considering the candidate 251359_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251359_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251391_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251391_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251420_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251420_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:47:59.93 +00:36:57.7: 14.90 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:47:59.93 +00:36:57.7: 13.03 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.03
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Considering the candidate 251429_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251429_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:14.78 -00:07:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.926 3118740134913015936 095.56134412545 -00.12694335465 13.1763 12.6213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 251452_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251452_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:46:11.40 +01:50:35.1: 14.78 +/- 99.00 upperlimit
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:46:11.40 +01:50:35.1: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.03
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Considering the candidate 251454_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251454_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251468_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251468_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251470_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251470_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251475_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251475_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:40:17.51 -04:25:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251508_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251508_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251513_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251513_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251514_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251514_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251538_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251538_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251543_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251543_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251552_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251552_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251581_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251581_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 251588_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251588_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251645_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251645_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:34:53.96 -00:09:47.5: 12.83 +/- 0.05 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:34:53.96 -00:09:47.5: 13.41 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.04
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Considering the candidate 251659_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251659_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251694_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251694_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251705_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251705_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251741_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 251741_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:30:11.55 +03:02:32.7: 10.57 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:30:11.55 +03:02:32.7: 13.96 +/- 0.09 detection
Forced photometry reference-image weighted average: 10.60 +/- 0.01
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Considering the candidate 251761_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251761_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251789_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251789_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251815_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251815_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 251844_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 251844_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 24558_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 24558_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 07680_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 07680_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:22:36.49 +02:48:59.3: 11.63 +/- 0.02 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:22:36.49 +02:48:59.3: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.02
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Considering the candidate 231699_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 231699_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 232448_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232448_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:22:49.44 +02:17:38.1: 10.79 +/- 0.01 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:22:49.44 +02:17:38.1: 11.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.16 +/- 0.01
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Considering the candidate 06227_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 06227_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 34640_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 34640_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 34850_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 34850_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 61851_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 61851_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:04.49 -00:00:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 2.783 3121745649946896896 095.51861547226 -00.00979524879 12.8290 12.3185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 42663_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 42663_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:18.88 +00:55:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 1.927 3123375877797010688 095.32867191748 +00.92607573456 11.9105 11.5004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 17626_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 17626_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:37.87 +02:13:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24010_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 24010_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:51.77 +01:51:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.948 3123731402307022592 095.96577591141 +01.86454655040 12.9186 12.3769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 11910_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 11910_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:32.53 +02:33:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.78, MAG_FAINT_SEARCH_LIMIT=11.76)GAIADR2_OUTPUT=# 2.104 3124213980534601984 096.13553121241 +02.55830453887 11.5286 11.0860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 170770_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 170770_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 219202_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 219202_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:11.81 -06:08:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 2.359 3008161833894189056 095.29935500637 -06.13527780853 12.6175 12.2472 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 04797_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 04797_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:55.11 +02:59:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.64, MAG_FAINT_SEARCH_LIMIT=11.62)GAIADR2_OUTPUT=# 2.427 3125018140149322368 095.47983967612 +02.99849983636 11.2669 10.7861 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 232932_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232932_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:20:35.55 -03:15:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 2.713 3116890511539679744 095.14827465598 -03.26190530859 11.9495 11.7175 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 07633_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 07633_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:14.35 +02:49:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.310 3124973060172903040 096.05987213680 +02.81705775237 12.6628 12.1388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 232478_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232478_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:33.58 +03:05:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.89, MAG_FAINT_SEARCH_LIMIT=10.87)GAIADR2_OUTPUT=# 1.483 3125001269518056448 095.88997867783 +03.08692611323 10.5370 10.0493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 232445_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232445_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:38.78 +00:36:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 2.058 3123330900899496576 095.41153748194 +00.61234682557 11.6005 11.0281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 232418_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232418_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:20:44.17 -06:24:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 2.652 3007944512844886528 095.18397385819 -06.40540032417 11.7322 11.2192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 232414_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232414_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:49.88 +01:41:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 2.637 3123713118627231744 096.20781563977 +01.68893431157 11.9456 11.5043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 232275_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232275_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:13.37 +01:08:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 2.587 3123386357517211008 095.55578166062 +01.13420173102 12.5605 12.0066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 232209_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232209_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:44.30 +00:45:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 2.757 3123355403689030272 095.68434690516 +00.74991034752 12.5698 12.0214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 26937_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 26937_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-02_20.00sec_-14.90C_LIGHT_0048.fits at 06:23:26.26 +01:42:25.8: 12.63 +/- 0.06 detection
Forced photometry on wcs_Mon-02-Q1b1x1_2026-03-20_21-38-48_20.00sec_-15.00C_LIGHT_0049.fits at 06:23:26.26 +01:42:25.8: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.04
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Considering the candidate 232126_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232126_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:25:54.01 +02:48:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 3.292 3124213744314179456 096.47504402705 +02.80978008404 12.7409 12.3795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 232119_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232119_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:37.15 +02:08:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 3.199 3124115372383526784 096.15487999714 +02.13394913627 12.5851 12.0031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 232118_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232118_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:40.68 +01:10:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 2.864 3123477861796929920 095.91958516442 +01.18173682799 12.8092 12.1585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 232081_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 232081_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:43.02 +02:39:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231888_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 231888_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 231870_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 231870_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:25:22.26 +02:45:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 3.856 3124223601261332096 096.34297602631 +02.76167505504 12.9306 12.4191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 231666_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 231666_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:12.35 +02:45:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 3.025 3124962958410006400 095.55131810696 +02.75178260297 13.0106 12.5312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 231285_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 231285_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:45.85 +01:45:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 3.450 3123712332652595200 095.94109530706 +01.75045981645 13.2644 12.7268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 23318_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 23318_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:47.22 +01:54:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40050_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 40050_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:47.44 +01:02:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 2.274 3123381757608261632 095.69747324177 +01.04353764860 11.7233 11.2167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 42576_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 42576_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:14.78 +00:55:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 2.448 3123375504136024064 095.31147972831 +00.92391138666 12.1837 11.8065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 37203_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
The candidate 37203_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:31.04 +01:05:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129332_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 129332_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 50933_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 50933_fd_Mon-02-Q1b1x1_2026-04-27_21-52-46_20.00sec_-4.90C_LIGHTs_0030
make_report_in_HTML.sh Phase 2 (HTML assembly): 8s
make_report_in_HTML.sh TOTAL: 917s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:22:08.91 +02:54:31.9
07:12:49.91 -03:03:26.7
07:12:53.88 -06:13:46.5
06:57:00.74 -04:49:23.0
06:27:21.55 +02:34:18.4
06:22:44.95 +01:50:00.9
07:09:59.87 +01:25:48.9
06:56:09.30 +00:23:33.9
06:45:22.68 -02:49:59.9
07:07:51.73 -05:46:55.5
06:43:56.50 +01:29:48.1
07:09:20.84 +01:37:48.3
07:01:35.54 -07:10:47.4
06:32:50.20 -03:46:06.9
07:08:29.29 -00:58:27.2
07:07:06.86 +01:29:04.5
06:54:34.58 +02:24:43.3
07:03:22.35 -04:53:37.3
06:24:52.04 -03:33:44.0
07:03:40.15 -01:07:50.1
06:59:30.13 +00:22:10.1
06:53:55.00 +02:25:33.8
07:17:43.21 -05:40:05.0
07:12:01.86 -01:11:14.3
07:08:41.75 +01:18:43.1
06:46:34.59 +01:47:57.8
06:23:23.70 -03:28:38.7
07:10:59.50 -03:55:09.7
06:58:42.69 -03:39:02.5
07:04:47.96 +02:23:27.9
07:08:44.23 -03:56:12.3
07:07:17.10 +01:47:31.0
06:39:40.54 +03:07:11.8
06:21:43.87 -00:15:06.8
06:24:07.43 -00:16:09.1
07:08:35.57 +01:46:45.8
07:11:05.36 -04:42:12.1
06:45:27.75 +00:57:44.3
06:29:05.56 +03:16:44.9
06:26:59.98 +00:24:40.8
06:58:31.26 -07:10:56.3
07:16:19.66 -06:57:24.2
07:19:20.23 -00:18:58.7
06:51:37.46 -06:57:16.6
06:22:05.04 -04:25:37.7
07:06:24.13 +00:20:29.6
07:19:32.16 -03:36:33.6
07:00:56.90 -03:16:15.2
07:22:52.24 +01:09:04.4
06:22:32.51 -04:26:55.2
06:22:54.82 +02:15:15.6
06:52:57.28 -03:04:53.3
07:13:53.87 -00:07:53.1
06:30:25.55 -00:34:50.6
06:20:50.77 -04:58:33.6
06:23:37.14 +01:59:36.3
06:54:29.98 -04:07:28.3
07:07:58.63 -00:56:38.9
07:05:49.64 +01:33:34.7
06:57:00.73 +00:17:39.2
06:26:10.53 +01:36:50.5
06:39:58.45 -01:44:23.9
06:24:57.34 +02:30:05.5
06:24:53.83 -02:34:45.7
06:32:06.23 +03:17:17.2
07:02:19.58 -03:20:38.6
06:48:48.53 +00:23:30.1
06:37:10.38 +03:05:45.9
06:21:53.24 +01:15:50.1
06:21:55.43 -01:41:34.6
06:28:36.65 +01:48:24.0
06:56:36.36 +02:42:47.6
06:25:41.40 +01:28:51.8
06:45:54.97 +00:45:36.1
06:40:28.24 +03:16:37.2
06:34:44.91 +01:53:00.9
06:22:06.26 +03:13:15.8
06:21:22.28 +01:19:22.4
06:22:45.78 +01:17:39.0
06:21:21.90 +00:30:33.9
########### Completed Mon-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
07:09:59.87 +01:25:48.9
06:56:09.30 +00:23:33.9
06:45:22.68 -02:49:59.9
07:07:51.73 -05:46:55.5
06:43:56.50 +01:29:48.1
07:09:20.84 +01:37:48.3
07:01:35.54 -07:10:47.4
06:32:50.20 -03:46:06.9
07:08:29.29 -00:58:27.2
07:07:06.86 +01:29:04.5
06:54:34.58 +02:24:43.3
07:03:22.35 -04:53:37.3
06:24:52.04 -03:33:44.0
07:03:40.15 -01:07:50.1
06:59:30.13 +00:22:10.1
06:53:55.00 +02:25:33.8
07:17:43.21 -05:40:05.0
07:12:01.86 -01:11:14.3
07:08:41.75 +01:18:43.1
06:46:34.59 +01:47:57.8
06:23:23.70 -03:28:38.7
07:10:59.50 -03:55:09.7
06:58:42.69 -03:39:02.5
07:04:47.96 +02:23:27.9
07:08:44.23 -03:56:12.3
07:07:17.10 +01:47:31.0
06:39:40.54 +03:07:11.8
06:21:43.87 -00:15:06.8
06:24:07.43 -00:16:09.1
07:08:35.57 +01:46:45.8
07:11:05.36 -04:42:12.1
06:45:27.75 +00:57:44.3
06:29:05.56 +03:16:44.9
06:26:59.98 +00:24:40.8
06:58:31.26 -07:10:56.3
07:16:19.66 -06:57:24.2
07:19:20.23 -00:18:58.7
06:51:37.46 -06:57:16.6
06:22:05.04 -04:25:37.7
07:06:24.13 +00:20:29.6
07:19:32.16 -03:36:33.6
07:00:56.90 -03:16:15.2
07:22:52.24 +01:09:04.4
06:22:32.51 -04:26:55.2
06:22:54.82 +02:15:15.6
06:52:57.28 -03:04:53.3
07:13:53.87 -00:07:53.1
06:30:25.55 -00:34:50.6
06:20:50.77 -04:58:33.6
06:23:37.14 +01:59:36.3
06:54:29.98 -04:07:28.3
07:07:58.63 -00:56:38.9
07:05:49.64 +01:33:34.7
06:57:00.73 +00:17:39.2
06:26:10.53 +01:36:50.5
06:39:58.45 -01:44:23.9
06:24:57.34 +02:30:05.5
06:24:53.83 -02:34:45.7
06:32:06.23 +03:17:17.2
07:02:19.58 -03:20:38.6
06:48:48.53 +00:23:30.1
06:37:10.38 +03:05:45.9
06:21:53.24 +01:15:50.1
06:21:55.43 -01:41:34.6
06:28:36.65 +01:48:24.0
06:56:36.36 +02:42:47.6
06:25:41.40 +01:28:51.8
06:45:54.97 +00:45:36.1
06:40:28.24 +03:16:37.2
06:34:44.91 +01:53:00.9
06:22:06.26 +03:13:15.8
06:22:44.95 +01:50:00.9
06:57:00.74 -04:49:23.0
06:22:08.91 +02:54:31.9
06:21:22.28 +01:19:22.4
06:22:45.78 +01:17:39.0
07:12:53.88 -06:13:46.5
06:27:21.55 +02:34:18.4
07:12:49.91 -03:03:26.7
06:21:21.90 +00:30:33.9
###################################################################################
07:09:59.87 +01:25:48.9 -- not an asteroid (will add it to exclusion list)
06:56:09.30 +00:23:33.9 -- not an asteroid (will add it to exclusion list)
06:45:22.68 -02:49:59.9 -- not an asteroid (will add it to exclusion list)
07:07:51.73 -05:46:55.5 -- not an asteroid (will add it to exclusion list)
06:43:56.50 +01:29:48.1 -- not an asteroid (will add it to exclusion list)
07:09:20.84 +01:37:48.3 -- not an asteroid (will add it to exclusion list)
07:01:35.54 -07:10:47.4 -- not an asteroid (will add it to exclusion list)
06:32:50.20 -03:46:06.9 -- not an asteroid (will add it to exclusion list)
07:08:29.29 -00:58:27.2 -- not an asteroid (will add it to exclusion list)
07:07:06.86 +01:29:04.5 -- not an asteroid (will add it to exclusion list)
06:54:34.58 +02:24:43.3 -- not an asteroid (will add it to exclusion list)
07:03:22.35 -04:53:37.3 -- not an asteroid (will add it to exclusion list)
06:24:52.04 -03:33:44.0 -- not an asteroid (will add it to exclusion list)
07:03:40.15 -01:07:50.1 -- not an asteroid (will add it to exclusion list)
06:59:30.13 +00:22:10.1 -- not an asteroid (will add it to exclusion list)
06:53:55.00 +02:25:33.8 -- not an asteroid (will add it to exclusion list)
07:17:43.21 -05:40:05.0 -- not an asteroid (will add it to exclusion list)
07:12:01.86 -01:11:14.3 -- not an asteroid (will add it to exclusion list)
07:08:41.75 +01:18:43.1 -- not an asteroid (will add it to exclusion list)
06:46:34.59 +01:47:57.8 -- asteroid (will NOT add it to exclusion list)
06:23:23.70 -03:28:38.7 -- not an asteroid (will add it to exclusion list)
07:10:59.50 -03:55:09.7 -- not an asteroid (will add it to exclusion list)
06:58:42.69 -03:39:02.5 -- not an asteroid (will add it to exclusion list)
07:04:47.96 +02:23:27.9 -- not an asteroid (will add it to exclusion list)
07:08:44.23 -03:56:12.3 -- not an asteroid (will add it to exclusion list)
07:07:17.10 +01:47:31.0 -- not an asteroid (will add it to exclusion list)
06:39:40.54 +03:07:11.8 -- not an asteroid (will add it to exclusion list)
06:21:43.87 -00:15:06.8 -- not an asteroid (will add it to exclusion list)
06:24:07.43 -00:16:09.1 -- not an asteroid (will add it to exclusion list)
07:08:35.57 +01:46:45.8 -- not an asteroid (will add it to exclusion list)
07:11:05.36 -04:42:12.1 -- not an asteroid (will add it to exclusion list)
06:45:27.75 +00:57:44.3 -- not an asteroid (will add it to exclusion list)
06:29:05.56 +03:16:44.9 -- not an asteroid (will add it to exclusion list)
06:26:59.98 +00:24:40.8 -- not an asteroid (will add it to exclusion list)
06:58:31.26 -07:10:56.3 -- not an asteroid (will add it to exclusion list)
07:16:19.66 -06:57:24.2 -- not an asteroid (will add it to exclusion list)
07:19:20.23 -00:18:58.7 -- not an asteroid (will add it to exclusion list)
06:51:37.46 -06:57:16.6 -- not an asteroid (will add it to exclusion list)
06:22:05.04 -04:25:37.7 -- not an asteroid (will add it to exclusion list)
07:06:24.13 +00:20:29.6 -- not an asteroid (will add it to exclusion list)
07:19:32.16 -03:36:33.6 -- not an asteroid (will add it to exclusion list)
07:00:56.90 -03:16:15.2 -- not an asteroid (will add it to exclusion list)
07:22:52.24 +01:09:04.4 -- not an asteroid (will add it to exclusion list)
06:22:32.51 -04:26:55.2 -- not an asteroid (will add it to exclusion list)
06:22:54.82 +02:15:15.6 -- not an asteroid (will add it to exclusion list)
06:52:57.28 -03:04:53.3 -- not an asteroid (will add it to exclusion list)
07:13:53.87 -00:07:53.1 -- not an asteroid (will add it to exclusion list)
06:30:25.55 -00:34:50.6 -- not an asteroid (will add it to exclusion list)
06:20:50.77 -04:58:33.6 -- not an asteroid (will add it to exclusion list)
06:23:37.14 +01:59:36.3 -- not an asteroid (will add it to exclusion list)
06:54:29.98 -04:07:28.3 -- not an asteroid (will add it to exclusion list)
07:07:58.63 -00:56:38.9 -- not an asteroid (will add it to exclusion list)
07:05:49.64 +01:33:34.7 -- not an asteroid (will add it to exclusion list)
06:57:00.73 +00:17:39.2 -- not an asteroid (will add it to exclusion list)
06:26:10.53 +01:36:50.5 -- not an asteroid (will add it to exclusion list)
06:39:58.45 -01:44:23.9 -- not an asteroid (will add it to exclusion list)
06:24:57.34 +02:30:05.5 -- not an asteroid (will add it to exclusion list)
06:24:53.83 -02:34:45.7 -- not an asteroid (will add it to exclusion list)
06:32:06.23 +03:17:17.2 -- not an asteroid (will add it to exclusion list)
07:02:19.58 -03:20:38.6 -- not an asteroid (will add it to exclusion list)
06:48:48.53 +00:23:30.1 -- not an asteroid (will add it to exclusion list)
06:37:10.38 +03:05:45.9 -- not an asteroid (will add it to exclusion list)
06:21:53.24 +01:15:50.1 -- not an asteroid (will add it to exclusion list)
06:21:55.43 -01:41:34.6 -- not an asteroid (will add it to exclusion list)
06:28:36.65 +01:48:24.0 -- not an asteroid (will add it to exclusion list)
06:56:36.36 +02:42:47.6 -- not an asteroid (will add it to exclusion list)
06:25:41.40 +01:28:51.8 -- not an asteroid (will add it to exclusion list)
06:45:54.97 +00:45:36.1 -- not an asteroid (will add it to exclusion list)
06:40:28.24 +03:16:37.2 -- not an asteroid (will add it to exclusion list)
06:34:44.91 +01:53:00.9 -- not an asteroid (will add it to exclusion list)
06:22:06.26 +03:13:15.8 -- not an asteroid (will add it to exclusion list)
06:22:44.95 +01:50:00.9 -- not an asteroid (will add it to exclusion list)
06:57:00.74 -04:49:23.0 -- not an asteroid (will add it to exclusion list)
06:22:08.91 +02:54:31.9 -- not an asteroid (will add it to exclusion list)
06:21:22.28 +01:19:22.4 -- not an asteroid (will add it to exclusion list)
06:22:45.78 +01:17:39.0 -- not an asteroid (will add it to exclusion list)
07:12:53.88 -06:13:46.5 -- not an asteroid (will add it to exclusion list)
06:27:21.55 +02:34:18.4 -- not an asteroid (will add it to exclusion list)
07:12:49.91 -03:03:26.7 -- not an asteroid (will add it to exclusion list)
06:21:21.90 +00:30:33.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:20:50.77 -04:58:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:21.90 +00:30:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:22.28 +01:19:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:43.87 -00:15:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:53.24 +01:15:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:55.43 -01:41:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:05.04 -04:25:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:06.26 +03:13:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:08.91 +02:54:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:32.51 -04:26:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:44.95 +01:50:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:45.78 +01:17:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:54.82 +02:15:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:23.70 -03:28:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:37.14 +01:59:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:07.43 -00:16:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:52.04 -03:33:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:53.83 -02:34:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:57.34 +02:30:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:41.40 +01:28:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:10.53 +01:36:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:59.98 +00:24:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:21.55 +02:34:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:36.65 +01:48:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:05.56 +03:16:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:25.55 -00:34:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:06.23 +03:17:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:50.20 -03:46:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:44.91 +01:53:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:10.38 +03:05:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:40.54 +03:07:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:58.45 -01:44:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:28.24 +03:16:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:56.50 +01:29:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:22.68 -02:49:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:27.75 +00:57:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:54.97 +00:45:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:48.53 +00:23:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:37.46 -06:57:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:57.28 -03:04:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:55.00 +02:25:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:29.98 -04:07:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:34.58 +02:24:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:09.30 +00:23:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:36.36 +02:42:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:00.73 +00:17:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:00.74 -04:49:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:31.26 -07:10:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:42.69 -03:39:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:30.13 +00:22:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:56.90 -03:16:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:35.54 -07:10:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:19.58 -03:20:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:22.35 -04:53:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:40.15 -01:07:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:47.96 +02:23:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:49.64 +01:33:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:24.13 +00:20:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:06.86 +01:29:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:17.10 +01:47:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:51.73 -05:46:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:58.63 -00:56:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:29.29 -00:58:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:35.57 +01:46:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:41.75 +01:18:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:44.23 -03:56:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:20.84 +01:37:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:59.87 +01:25:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:59.50 -03:55:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:05.36 -04:42:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:01.86 -01:11:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:49.91 -03:03:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:53.88 -06:13:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:53.87 -00:07:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:19.66 -06:57:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:43.21 -05:40:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:20.23 -00:18:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:32.16 -03:36:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:52.24 +01:09:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
06:20:50.77 -04:58:33.6 -- not a known variable star
06:21:21.90 +00:30:33.9 -- not a known variable star
06:21:22.28 +01:19:22.4 -- not a known variable star
06:21:43.87 -00:15:06.8 -- not a known variable star
06:21:53.24 +01:15:50.1 -- not a known variable star
06:21:55.43 -01:41:34.6 -- not a known variable star
06:22:05.04 -04:25:37.7 -- not a known variable star
06:22:06.26 +03:13:15.8 -- not a known variable star
06:22:08.91 +02:54:31.9 -- not a known variable star
06:22:32.51 -04:26:55.2 -- not a known variable star
06:22:44.95 +01:50:00.9 -- not a known variable star
06:22:45.78 +01:17:39.0 -- not a known variable star
06:22:54.82 +02:15:15.6 -- not a known variable star
06:23:23.70 -03:28:38.7 -- a known variable star
06:23:37.14 +01:59:36.3 -- not a known variable star
06:24:07.43 -00:16:09.1 -- not a known variable star
06:24:52.04 -03:33:44.0 -- not a known variable star
06:24:53.83 -02:34:45.7 -- not a known variable star
06:24:57.34 +02:30:05.5 -- not a known variable star
06:25:41.40 +01:28:51.8 -- not a known variable star
06:26:10.53 +01:36:50.5 -- not a known variable star
06:26:59.98 +00:24:40.8 -- not a known variable star
06:27:21.55 +02:34:18.4 -- a known variable star
06:28:36.65 +01:48:24.0 -- not a known variable star
06:29:05.56 +03:16:44.9 -- not a known variable star
06:30:25.55 -00:34:50.6 -- not a known variable star
06:32:06.23 +03:17:17.2 -- not a known variable star
06:32:50.20 -03:46:06.9 -- not a known variable star
06:34:44.91 +01:53:00.9 -- not a known variable star
06:37:10.38 +03:05:45.9 -- not a known variable star
06:39:40.54 +03:07:11.8 -- not a known variable star
06:39:58.45 -01:44:23.9 -- not a known variable star
06:40:28.24 +03:16:37.2 -- not a known variable star
06:43:56.50 +01:29:48.1 -- not a known variable star
06:45:22.68 -02:49:59.9 -- a known variable star
06:45:27.75 +00:57:44.3 -- not a known variable star
06:45:54.97 +00:45:36.1 -- a known variable star
06:48:48.53 +00:23:30.1 -- a known variable star
06:51:37.46 -06:57:16.6 -- not a known variable star
06:52:57.28 -03:04:53.3 -- not a known variable star
06:53:55.00 +02:25:33.8 -- a known variable star
06:54:29.98 -04:07:28.3 -- not a known variable star
06:54:34.58 +02:24:43.3 -- not a known variable star
06:56:09.30 +00:23:33.9 -- not a known variable star
06:56:36.36 +02:42:47.6 -- not a known variable star
06:57:00.73 +00:17:39.2 -- not a known variable star
06:57:00.74 -04:49:23.0 -- not a known variable star
06:58:31.26 -07:10:56.3 -- a known variable star
06:58:42.69 -03:39:02.5 -- not a known variable star
06:59:30.13 +00:22:10.1 -- not a known variable star
07:00:56.90 -03:16:15.2 -- not a known variable star
07:01:35.54 -07:10:47.4 -- not a known variable star
07:02:19.58 -03:20:38.6 -- not a known variable star
07:03:22.35 -04:53:37.3 -- not a known variable star
07:03:40.15 -01:07:50.1 -- not a known variable star
07:04:47.96 +02:23:27.9 -- not a known variable star
07:05:49.64 +01:33:34.7 -- not a known variable star
07:06:24.13 +00:20:29.6 -- not a known variable star
07:07:06.86 +01:29:04.5 -- not a known variable star
07:07:17.10 +01:47:31.0 -- not a known variable star
07:07:51.73 -05:46:55.5 -- a known variable star
07:07:58.63 -00:56:38.9 -- not a known variable star
07:08:29.29 -00:58:27.2 -- a known variable star
07:08:35.57 +01:46:45.8 -- not a known variable star
07:08:41.75 +01:18:43.1 -- a known variable star
07:08:44.23 -03:56:12.3 -- not a known variable star
07:09:20.84 +01:37:48.3 -- not a known variable star
07:09:59.87 +01:25:48.9 -- not a known variable star
07:10:59.50 -03:55:09.7 -- not a known variable star
07:11:05.36 -04:42:12.1 -- not a known variable star
07:12:01.86 -01:11:14.3 -- a known variable star
07:12:49.91 -03:03:26.7 -- a known variable star
07:12:53.88 -06:13:46.5 -- not a known variable star
07:13:53.87 -00:07:53.1 -- not a known variable star
07:16:19.66 -06:57:24.2 -- not a known variable star
07:17:43.21 -05:40:05.0 -- not a known variable star
07:19:20.23 -00:18:58.7 -- a known variable star
07:19:32.16 -03:36:33.6 -- not a known variable star
07:22:52.24 +01:09:04.4 -- not a known variable star
Found 66 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
79 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 79 (excluding asteroids and hot pixels, 66 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)2461158.61942259 -observatory V36
01:18:30.14 +05:54:15.7 Mercury (-0.6mag)
04:09:12.58 +21:46:52.1 Venus (-3.9mag)
00:52:11.25 +04:36:20.3 Mars (1.2mag)
07:18:52.79 +22:35:26.1 Jupiter (-2.0mag)
00:34:27.59 +01:21:33.3 Saturn (0.9mag)
03:50:21.84 +19:55:55.2 Uranus (5.8mag)
00:12:21.74 -00:05:50.9 Neptune (7.8mag)
20:34:08.42 -22:53:41.6 Pluto (14.5mag)
11:45:11.16 -00:37:23.3 Moon (-11.7mag)
-rw-r--r-- 1 apache apache 363 Apr 27 22:04 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461158.61942259:
07:18:46.10 +22:35:41.7 Io (5.8mag)
07:18:57.56 +22:35:12.6 Europa (6.0mag)
07:18:54.90 +22:35:28.1 Ganymede (5.4mag)
07:18:45.92 +22:35:49.8 Callisto (6.7mag)
07:21:37.19 +22:18:02.2 Himalia (15.4mag)
07:18:56.16 +22:35:16.6 Thebe (16.3mag)
07:22:01.11 +22:47:52.5 Elara (17.4mag)
07:18:34.74 +23:09:05.7 Pasiphae (17.5mag)
07:26:54.62 +22:34:29.1 Carme (18.6mag)
00:34:39.60 +01:21:34.1 Titan (8.8mag)
00:34:27.19 +01:21:49.3 Rhea (10.1mag)
00:33:57.86 +01:19:57.6 Iapetus (11.5mag)
00:34:30.96 +01:21:15.0 Hyperion (14.8mag)
00:35:54.14 +01:28:58.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 27 22:04 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461158.61942259:
16:23:27.98 -23:31:19.4 JWST
18:14:28.82 +31:05:15.3 Chandra
07:55:25.68 -36:28:29.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 27 22:04 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461158.61942259 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
06:07:59.92 +30:22:14.0 17.9mag P/2009 WX51 (Catalina)
18:55:23.46 -29:32:45.6 13.8mag P/2010 H2 (Vales)
05:16:01.29 -69:07:52.5 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:35:25.70 +31:31:45.2 17.3mag C/2017 K2 (PANSTARRS)
17:28:31.64 +11:56:03.6 17.7mag C/2021 G2 (ATLAS)
23:12:55.29 +29:44:42.8 17.1mag C/2022 E2 (ATLAS)
04:43:36.90 +26:20:49.7 16.1mag C/2022 N2 (PANSTARRS)
09:06:55.98 +32:00:25.9 16.3mag C/2022 QE78 (ATLAS)
08:33:37.69 +01:03:00.1 17.4mag C/2022 R6 (PANSTARRS)
18:50:03.70 +19:30:17.7 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:36:16.67 -11:20:37.9 17.5mag P/2023 B1 (PANSTARRS)
09:03:07.26 -10:02:54.1 17.8mag C/2023 F3 (ATLAS)
22:04:45.90 +63:40:19.8 17.6mag C/2023 H5 (Lemmon)
19:06:18.65 -04:01:05.1 14.0mag C/2023 R1 (PANSTARRS)
20:30:24.18 +87:35:00.8 17.8mag C/2023 X2 (Lemmon)
06:25:21.81 +63:30:49.2 17.3mag C/2024 A1 (ATLAS)
05:37:46.02 +21:42:24.3 11.8mag C/2024 E1 (Wierzchos)
16:10:45.91 +08:20:16.7 17.3mag C/2024 G6 (ATLAS)
20:23:11.81 +18:40:55.5 14.5mag C/2024 J3 (ATLAS)
03:37:33.23 -20:37:30.7 16.3mag C/2024 T5 (ATLAS)
05:27:23.83 +42:27:03.2 17.8mag C/2025 J1 (Borisov)
12:51:25.37 +50:57:40.1 15.7mag C/2025 L1 (ATLAS)
03:45:29.38 -28:14:43.7 17.9mag C/2025 Q3 (ATLAS)
03:01:38.98 +04:57:19.4 8.0mag C/2025 R3 (PANSTARRS)
12:49:05.52 +03:41:09.8 17.3mag C/2025 Y1 (ATLAS)
04:40:02.59 +01:50:08.8 16.0mag C/2026 A1 (MAPS)
00:32:17.17 +39:11:48.2 15.0mag C/2026 B2 (Sun-Gao)
19:06:24.23 -09:03:33.0 11.1mag 10P/Tempel
14:44:00.52 +01:44:41.6 15.1mag 24P/Schaumasse
11:00:14.99 -01:11:11.1 15.8mag 29P/Schwassmann-Wachmann
10:38:39.31 -03:17:08.4 17.2mag 43P/Wolf-Harrington
02:07:31.31 +19:30:38.3 17.3mag 47P/Ashbrook-Jackson
07:34:05.02 +34:19:27.1 17.0mag 63P/Wild
23:44:02.73 -10:03:05.6 15.7mag 65P/Gunn
04:36:45.45 +25:07:51.6 16.0mag 76P/West-Kohoutek-Ikemura
01:32:43.01 +10:33:43.5 14.2mag 78P/Gehrels
23:38:22.54 -05:49:17.6 14.8mag 88P/Howell
02:45:37.45 +23:41:21.1 15.0mag 93P/Lovas
05:18:39.75 +32:50:59.4 16.1mag 123P/West-Hartley
08:44:10.63 +32:48:02.4 16.3mag 124P/Mrkos
02:52:12.39 +15:40:39.0 16.4mag 128P/Shoemaker-Holt
03:11:28.54 +15:52:56.0 17.6mag 131P/Mueller
02:31:17.94 +16:49:03.5 10.6mag 141P/Machholz
02:38:06.22 +09:15:55.4 10.6mag 141P-A/Machholz
01:19:02.74 +04:59:59.4 11.5mag 141P-D/Machholz
01:36:31.82 +04:35:56.2 14.9mag 162P/SidingSpring
22:11:17.82 -08:36:01.3 17.9mag 218P/LINEAR
17:16:59.94 -12:26:38.6 16.1mag 235P/LINEAR
06:01:11.12 +35:26:15.0 16.9mag 240P/NEAT
07:45:18.51 -03:58:04.3 17.8mag 242P/Spahr
22:47:16.72 -17:31:09.9 17.5mag 260P/McNaught
02:23:45.95 +23:28:05.4 17.9mag 295P/LINEAR
15:37:09.72 +07:41:48.4 17.4mag 391P/Kowalski
07:39:39.59 +21:21:36.7 17.7mag 450P/LONEOS
05:54:05.16 +44:19:26.1 17.6mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 27 22:04 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:34:34.94 -54:34:58.20 ASASSN-26da 2026-04-25.14 15.99
10:06:55.04 -01:13:49.70 SN2026jsg 2026-04-24.99 16.28
15:15:57.17 +56:18:32.80 SN2026kid 2026-04-24.52 -3.65
07:58:28.45 +57:03:42.40 AT2026kcf 2026-04-24.2 16.89
11:38:21.80 -50:43:06.50 SN2026jkb 2026-04-24.24 15.38
10:06:11.41 -39:41:04.20 AT2026dil 2026-04-24.2 16.85
14:21:40.08 +13:13:46.30 SN2026jlm 2026-04-22.16 15.12
10:53:55.47 -16:06:07.00 ASASSN-26cz 2026-04-22.24 16.32
16:34:34.94 -54:34:58.20 2026-04-25.14 15.99
13:45:02.03 +15:17:14.50 ASASSN-26cy 2026-04-21.27 15.78
13:20:52.22 -35:57:03.60 AT2026jcm 2026-04-19.01 16.65
13:36:15.66 -36:53:48.40 SN 2026iqy 2026-04-18.92 17.31
06:34:01.33 -40:07:34.00 ASASSN-26cx 2026-04-19.07 16.16
23:33:57.97 -45:12:11.90 SN 2026idu 2026-04-19.41 15.9
12:10:50.92 +66:55:31.20 SN 2026icv 2026-04-17.14 16.03
21:36:59.06 -60:43:35.90 ASASSN-26cv 2026-04-17.35 -1.18
08:13:26.26 -27:07:30.50 ASASSN-26cw 2026-04-17.07 -1.01
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
16:34:34.94 -54:34:58.20 2026-04-25.14 15.99
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.14 13.64
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
00:43:35.02 +41:46:28.0 PNV J00433502+4146280 2026-04-23.056 15.9mag
00:42:55.64 +41:14:12.2 PNV J00425564+4114122 2026-04-24.042 16.2mag
-rw-r--r-- 1 apache apache 188K Apr 27 22:04 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
19:23:59.111 -12:30:36.58 AT 2026kgc 2026-04-15.48 18.635
18:39:37.719 +06:55:20.96 AT 2026kgb 2026-04-17.43 16.308
15:06:42.954 -01:17:07.82 AT 2026kga 2026-04-20.40 19.507
17:53:09.200 +11:02:30.70 AT 2026kfz 2026-04-16.84 18.68
16:03:08.437 +31:48:52.12 AT 2026kfy 2026-04-15.37 20.9066
12:40:00.450 -17:44:25.00 AT 2026kfx 2026-04-21.19 17.9
09:56:52.772 +01:49:59.18 AT 2026kfw 2026-04-21.04 22.5328
09:59:02.400 +01:44:31.96 AT 2026kfv 2026-04-16.08 23.04
13:20:14.744 +79:52:47.47 AT 2026kfu 2026-04-20.39 20.1588
15:56:36.952 +46:26:50.20 AT 2026kft 2026-04-15.37 20.5825
14:36:13.311 -40:29:09.08 AT 2026kfs 2026-04-17.20 19.109
17:55:24.804 -72:52:42.49 AT 2026kfr 2026-04-19.04 19.559
14:53:17.557 +07:16:56.07 AT 2026kfq 2026-04-20.44 20.1681
14:23:33.083 +17:33:13.27 AT 2026kfp 2026-04-15.41 20.3946
11:23:12.007 -46:35:10.13 AT 2026kfo 2026-04-18.14 19.338
09:22:59.874 +10:47:32.59 AT 2026kfn 2026-04-15.92 20.064
08:41:46.826 -08:01:26.25 AT 2026kfm 2026-04-20.87 19.199
08:23:28.067 -08:48:36.88 AT 2026kfl 2026-04-19.02 18.681
14:03:29.355 +22:20:30.16 AT 2026kfk 2026-04-15.41 20.4393
16:25:23.534 -76:28:24.80 AT 2026kfj 2026-04-19.01 19.458
-rw-r--r-- 1 apache apache 29K Apr 27 22:04 tns_transients_list.txt
