This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0
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 08 06.3670 2461258.8670 9.15 06:04:44.45 +35:46:35.0
176.09558 6.91942 galactic Aur Second-epoch detections are separated by 1.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3453468479845590400 | 06:04:44.38 +35:46:35.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.751+/-0.050 (K)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:44.45 +35:46:35.0: 10.45 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:44.45 +35:46:35.0: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.49 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3453468479845590400,2461258.8670,9.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3453468479845590400 20260806.3670 9.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3670 2461258.8670 9.54 06:02:33.25 +35:36:39.7
176.02648 6.45065 galactic Aur Second-epoch detections are separated by 0.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.6301+35.6152 | 06:02:33.21 +35:36:39.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.765+/-0.035 (K)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:33.25 +35:36:39.7: 10.90 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:33.25 +35:36:39.7: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.6301+35.6152,2461258.8670,9.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.6301+35.6152 20260806.3670 9.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3670 2461258.8670 9.39 06:04:02.51 +35:39:34.5
176.13029 6.73891 galactic Aur Second-epoch detections are separated by 2.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.0174+35.6619 | 06:04:02.44 +35:39:35.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.644+/-0.041 (K)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:02.51 +35:39:34.5: 10.71 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:02.51 +35:39:34.5: 10.80 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.75 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.0174+35.6619,2461258.8670,9.39,0.05,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 J091.0174+35.6619 20260806.3670 9.39CV 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 08 06.3670 2461258.8670 9.46 06:05:01.51 +35:59:48.9
175.92820 7.07547 galactic Aur Second-epoch detections are separated by 3.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.2597+36.0035 | 06:05:01.65 +35:59:49.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.989+/-0.024 (M)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:05:01.51 +35:59:48.9: 11.10 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:05:01.51 +35:59:48.9: 11.20 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.2597+36.0035,2461258.8670,9.46,0.05,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 J091.2597+36.0035 20260806.3670 9.46CV 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 08 06.3670 2461258.8670 9.41 06:03:35.19 +35:43:41.4
176.02498 6.69082 galactic Aur Second-epoch detections are separated by 1.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.9016+35.7186 | 06:03:35.19 +35:43:41.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.686+/-0.038 (K)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:35.19 +35:43:41.4: 10.82 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:35.19 +35:43:41.4: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.85 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.9016+35.7186,2461258.8670,9.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.9016+35.7186 20260806.3670 9.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3670 2461258.8670 9.65 05:59:43.16 +35:20:41.8
175.97785 5.81698 galactic Aur Second-epoch detections are separated by 3.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3451995404845959040 | 05:59:43.15 +35:20:41.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.332+/-0.029 (G)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:59:43.16 +35:20:41.8: 10.81 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:59:43.16 +35:20:41.8: 10.84 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3451995404845959040,2461258.8670,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3451995404845959040 20260806.3670 9.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3670 2461258.8670 9.55 06:03:37.27 +36:03:21.7
175.73890 6.85463 galactic Aur Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.3300 McGlasson 286 -287 405 17.2 -0 0
ATTENTION: measured mag 9.55 is 7.6 mag brighter than the predicted asteroid brightness 17.2 - the transient may be an unrelated new object!
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:37.27 +36:03:21.7: 10.99 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:37.27 +36:03:21.7: 11.05 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461258.8670,9.55,0.05,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
VARIABLE_NAME 20260806.3670 9.55CV 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 08 06.3670 2461258.8670 9.64 04:58:23.55 +38:51:29.5
166.28444 -2.41091 galactic Aur Second-epoch detections are separated by 2.7" and 8.0 pix
The object was found in VSX 1" ASASSN-V J045823.57+385129.0
Type: L
# Max. Min./Amp. JD0 Period
10.990 V 11.140 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:58:23.55 +38:51:29.5: 10.60 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:58:23.55 +38:51:29.5: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.56 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045823.57+385129.0,2461258.8670,9.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045823.57+385129.0 20260806.3670 9.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3670 2461258.8670 10.01 05:51:51.07 +33:09:29.5
177.06549 3.31712 galactic Aur Second-epoch detections are separated by 4.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J087.9589+33.1472 | 05:51:52.10 +33:08:51.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.969+/-0.025 (M)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:51.07 +33:09:29.5: 11.06 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:51.07 +33:09:29.5: 11.08 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.07 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.9589+33.1472,2461258.8670,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.9589+33.1472 20260806.3670 10.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3670 2461258.8670 9.80 06:02:59.71 +35:39:44.6
176.02477 6.55392 galactic Aur Second-epoch detections are separated by 3.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3453474802037289344 | 06:02:59.70 +35:39:44.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.290+/-0.025 (F)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:59.71 +35:39:44.6: 10.76 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:59.71 +35:39:44.6: 10.80 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.78 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3453474802037289344,2461258.8670,9.80,0.05,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
Gaia DR3 3453474802037289344 20260806.3670 9.80CV 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 08 06.3670 2461258.8670 9.77 06:00:07.47 +34:45:26.1
176.53363 5.60153 galactic Aur Second-epoch detections are separated by 0.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.0359+34.7514 | 06:00:07.68 +34:45:27.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:07.47 +34:45:26.1: 10.66 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:07.47 +34:45:26.1: 10.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.68 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.0359+34.7514,2461258.8670,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.0359+34.7514 20260806.3670 9.77CV 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 08 06.3670 2461258.8670 9.18 06:02:00.75 +35:51:55.4
175.74893 6.47753 galactic Aur Second-epoch detections are separated by 2.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3453516132504333696 | 06:02:00.75 +35:51:54.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.721+/-0.027 (K)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:00.75 +35:51:55.4: 10.06 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:00.75 +35:51:55.4: 10.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.09 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3453516132504333696,2461258.8670,9.18,0.05,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 3453516132504333696 20260806.3670 9.18CV 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 08 06.3670 2461258.8670 8.79 06:04:25.93 +35:57:08.5
175.90979 6.94880 galactic Aur Second-epoch detections are separated by 2.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J091.1192+35.9520 | 06:04:25.99 +35:57:08.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.624+/-0.038 (K)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:25.93 +35:57:08.5: 9.70 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:25.93 +35:57:08.5: 9.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.73 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.1192+35.9520,2461258.8670,8.79,0.05,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 J091.1192+35.9520 20260806.3670 8.79CV 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 08 06.3670 2461258.8670 9.65 05:56:03.81 +34:11:18.5
176.61496 4.59284 galactic Aur Second-epoch detections are separated by 2.1" and 7.1 pix
The object was found in VSX 2" ASASSN-V J055603.95+341118.2
Type: SR
# Max. Min./Amp. JD0 Period
11.450 V 11.590 V 2457477.74700 33.450000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:03.81 +34:11:18.5: 10.93 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:03.81 +34:11:18.5: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.95 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055603.95+341118.2,2461258.8670,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J055603.95+341118.2 20260806.3670 9.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 06.3670 2461258.8670 9.46 06:03:19.73 +35:48:27.1
175.92961 6.68321 galactic Aur Second-epoch detections are separated by 1.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3453477482096840960 | 06:03:19.69 +35:48:26.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.623+/-0.032 (K)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:19.73 +35:48:27.1: 10.65 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:19.73 +35:48:27.1: 10.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.69 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3453477482096840960,2461258.8670,9.46,0.05,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 3453477482096840960 20260806.3670 9.46CV 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 08 06.3670 2461258.8670 10.06 05:32:40.72 +32:56:20.9
175.13459 -0.21305 galactic Aur Second-epoch detections are separated by 1.3" and 7.8 pix
The object was found in VSX 0" OV Aur
Type: LB
# Max. Min./Amp. JD0 Period
11.200 V 11.800 V C(R)
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:32:40.72 +32:56:20.9: 11.19 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:32:40.72 +32:56:20.9: 11.15 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
OV Aur,2461258.8670,10.06,0.05,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
OV Aur 20260806.3670 10.06CV 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 08 06.3670 2461258.8670 9.77 05:30:34.27 +33:01:09.3
174.82543 -0.53891 galactic Aur Second-epoch detections are separated by 0.4" and 7.8 pix
The object was found in VSX 1" ASASSN-V J053034.36+330108.5
Type: SR
# Max. Min./Amp. JD0 Period
12.080 g Y 0.260 g 2458820.91600 96.200000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:30:34.27 +33:01:09.3: 10.84 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:30:34.27 +33:01:09.3: 10.80 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.82 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053034.36+330108.5,2461258.8670,9.77,0.05,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
ASASSN-V J053034.36+330108.5 20260806.3670 9.77CV 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 08 06.3670 2461258.8670 9.34 05:38:48.48 +35:27:35.0
173.69537 2.21358 galactic Aur Second-epoch detections are separated by 1.2" and 7.7 pix
The object was found in VSX 1" ASASSN-V J053848.46+352736.3
Type: SR
# Max. Min./Amp. JD0 Period
11.570 g Y 0.420 g 2458356.95100 608.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:38:48.48 +35:27:35.0: 10.28 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:38:48.48 +35:27:35.0: 10.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.25 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053848.46+352736.3,2461258.8670,9.34,0.05,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
ASASSN-V J053848.46+352736.3 20260806.3670 9.34CV 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
WARNING: VaST exited with code 1 on the field Aur-03-Q1b1x1 after completing the measurements (memory cleanup crash); the transient search continues.
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 2
Ref. image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461093.61879604 22.02.2026 02:50:53.978 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 23823
Objects passed selection criteria: 23623
Measurements per detected object (mean, median, min, max): 2.0 2.0 2 2
Measurements per selected object (mean, median, min, max): 2.0 2.0 2 2
Average stars detected per image: 27325
Average stars matched: 25759 (94.269 %)
Memory usage VmPeak: 249956 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 03:53:44 CDT 2026
Host name: tau
***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461258.86728968 06.08.2026 08:48:43.828 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 214
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 19 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 178523
Objects passed selection criteria: 177727
Measurements per detected object (mean, median, min, max): 2.0 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.0 2.0 2 4
Average stars detected per image: 103988
Average stars matched: 95681 (92.0116 %)
Memory usage VmPeak: 649020 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Aug 5 15:05:04 CDT 2026
VaST build number 1.0rc89-189-g49d3cdfd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-05)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 03:54:05 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
Last image: 2461258.86672188 06.08.2026 08:47:54.770 UTC
WARNING: VaST exited with code 1 on the field Aur-03-Q1b1x1 AFTER completing the measurements. This is a memory-management crash during cleanup (a VaST bug to report), NOT a wrong field / clouds / bad focus. The lightcurves were written, so the transient search continues.
____ VaST output (crashed during memory cleanup; the measurements above are complete) ____
--==VaST 1.0rc90==--
Parsing command line arguments...
opt 'F': Will NOT create flag images for SExtractor
opt '5': 5.000000 pix is the new fixed star matching radius!
opt 'b': Using 500 reference stars for image matching!
opt '3': Will try to select best aperture for each source!
opt 'y': 0 SysRem iterations will be conducted!
opt 't 4': robust linear magnitude calibration (vary zero-point and slope)
opt 'x': 99 is the maximum acceptable SExtractor flag!
WARNING: disabling the mag-size filter in order not to reject blended stars.
opt 'u': Stick with UTC time system, no conversion to TT will be done!
opt 'f': Run ./find_candidates manually!
opt 'k': "JD" keyword in FITS image header will be ignored!
INFO from vast_remove_directory(): Could not open directory: symlinks_to_images
INFO from vast_remove_directory(): Could not open directory: converted_images
INFO from vast_remove_directory(): Could not open directory: unpacked_images
Checking the list of input images specified on the command line ...
Looking for the list of input images with time corrections in vast_list_of_input_images_with_time_corrections.txt ... list not found.
This is OK if you specify the input images on the command line, not through this text file.
Checking write permissions for the current directory (/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0)... OK
Found a system-wide installation of SExtractor
Cleaning old outNNNNN.dat files.
Done with cleaning!
VaST was started with the following command line:
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
Preparing to process 4 input FITS images...
######## Forcing special settings for the transient detection ########
transient search mode: disabling the mag-size filter as it should be switched off when running a transient search!
transient search mode: disabling the bad image filter as it will not help during the transient search!
transient search mode: will not try to gues image saturation limit
transient search mode: no UTC-to-TT time system conversion will be performed!!!
transient search mode: setting the maximum acceptable SExtractor flag to 3
transient search mode: disabling rejectin of images with elliptical stars
transient search mode: not discarding large sources
################
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
Setting the fixed star match radius of 5.00 pix
We have 4 images to process.
SExtractor catalog cache: restored Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits catalog from cache
SExtractor catalog cache: restored Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits catalog from cache
Running SExtractor in 3 parallel threads...
Using the catalog image00001.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Using the catalog image00002.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
The gain value (GAIN=0.370) from default.sex will be used for image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
The above guess is based on the non-default gain value specified in default.sex by user
Parent process says: we are done fork()ing.
Waiting for thread 2 to finish...
autodetect_aperture() is running SExtractor on /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
autodetect_aperture() is doing a preliminary SExtractor run to determine an appropriate aperture size
sex -c default.sex -PARAMETERS_NAME autodetect_aper.param -CATALOG_NAME autodetect_aper_image00003.cat /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits > image00003.cat.sex_log 2>&1
The gain value (GAIN=0.370) from default.sex will be used for image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
The above guess is based on the non-default gain value specified in default.sex by user
autodetect_aperture() is running SExtractor on /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
autodetect_aperture() is doing a preliminary SExtractor run to determine an appropriate aperture size
sex -c default.sex -PARAMETERS_NAME autodetect_aper.param -CATALOG_NAME autodetect_aper_image00004.cat /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits > image00004.cat.sex_log 2>&1
autodetect_aperture() is doing the main SExtractor run
sex -PARAMETERS_NAME default.param -PHOT_APERTURES 6.7,6.7,6.0,7.3,8.0,8.7 -VERBOSE_TYPE NORMAL -CATALOG_NAME image00004.cat /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits > image00004.cat.sex_log 2>&1
autodetect_aperture() is doing the main SExtractor run
sex -PARAMETERS_NAME default.param -PHOT_APERTURES 6.8,6.8,6.2,7.5,8.2,8.9 -VERBOSE_TYPE NORMAL -CATALOG_NAME image00003.cat /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits > image00003.cat.sex_log 2>&1
autodetect_aperture() is done with image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
Waiting for thread 1 to finish...
autodetect_aperture() is done with image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
Done with SExtractor!
TIMING SExtractor: 1 seconds
Matching stars between images!
No manually selected comparison stars file manually_selected_comparison_stars.lst which is fine.
Processing /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
9576x6388 FITS image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Trying to guess the time system by parsing the comment string 'Time of observation (UTC)'
Time system set from the comment to DATE-OBS keyword: 'Time of observation (UTC)'
The input time system is identified as: UTC (blank if unknown)
Setting observation date using DATE-OBS keyword: 2026-01-18T02:41:07.3186602
Setting observation time using DATE-OBS keyword: 2026-01-18T02:41:07.3186602
Observing time converted to the "standard" FITS header format:
DATE-OBS= 2026-01-18T02:41:07.318
EXPTIME = 20.000
Using the catalog image00001.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Exposure 20 sec, 18.01.2026 02:41:07.318 UTC = JD(UTC) 2461058.61200600 mid. exp.
SExtractor output filtering results:
* passed selection: 27695, (27692 good for image matching)
* rejected as having no flux measurement: 0
* rejected as having SNR<3.0: 0
* rejected inside rectangles defined in bad_region.lst: 0
* rejected close to frame edge: 137
* rejected as being too small (<1.6 pix): 0
* rejected as being too large (>6.2 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 11
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
Please note: the CCD position-dependent magnitude correction will be applied.
get_detection_limit_sn(): Detection limit: -7.70
Detection limit from the magnitude-SNR relation= -7.7 (5.0 sigma detection)
The simple faintest star detection limit= -9.8
80 percent brightest stars detection limit= -10.5
Selected detection limit= -10.5
Final detection limit= -10.5 (after subtracting MAG_TRANSIENT_ABOVE_THE_REFERENCE_FRAME_LIMIT=0.0)
Parameter box for transient search: 10.06.1 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 13
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
26955 * detected, using 486/ 500 * for reference/current image matching, fraction_of_ambiguous_matches= 0.013757, number_of_ambiguous_matches=381
refining the coordinate transformation... [CVPOLY iter 1: order=2 pairs=23837 inliers=23837 rms 1.36 -> 0.36 pix, max corner correction 5.3 pix] fraction_of_ambiguous_matches= 0.010182, number_of_ambiguous_matches=282
23839 * matched, [CVPOLY iter 2: order=1 pairs=23839 inliers=23839 rms 0.29 -> 0.29 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.006752, number_of_ambiguous_matches=187
23829 * matched (2nd iteration). [CVPOLY iter 3: order=1 pairs=23829 inliers=23829 rms 0.20 -> 0.20 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.003105, number_of_ambiguous_matches=86
23823 * matched (3rd iteration). Success!
rotation [degrees] = 174.730
26955 stars detected, 23823 stars matched
Performing magnitude calibration using automatically selected comparison stars
Expecting to find at least 40 * for magnitude calibration
We have N_good_stars = 20755, N_manually_selected_comparison_stars = 0
Using 20755 stars for magnitude calibration (before filtering).
Iteratively removing outliers from the linear mag-mag relation (unweighted fit)...
After removing outliers in (X,Y,dm) plane, we are left with 20754 stars for magnitude calibration.
Using the linear CCD position-dependent magnitude correction:
delta_m = -0.00002*X_pix -0.00001*Y_pix +0.09458
Iteratively removing outliers from the mag-mag relation (weighted linear/polynomial fit)...
Computing robust linear magnitude calibration.
Used 20729 stars for magnitude calibration (after filtering).
get_detection_limit_sn(): Detection limit: -7.72
30827 objects stored in memory (1000000 max.)
Magnitude calibration is performed successfully!
Saving observations to the cache... OK
memory: 211432 kB used, 249956 kB peak, 65263848 kB available RAM
processed 2 of 4 images ( 50.0%)
Processing /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
9576x6388 FITS image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
Trying to guess the time system by parsing the comment string 'Time of observation (UTC)'
Time system set from the comment to DATE-OBS keyword: 'Time of observation (UTC)'
The input time system is identified as: UTC (blank if unknown)
Setting observation date using DATE-OBS keyword: 2026-08-06T08:47:54.7708429
Setting observation time using DATE-OBS keyword: 2026-08-06T08:47:54.7708429
Observing time converted to the "standard" FITS header format:
DATE-OBS= 2026-08-06T08:47:54.770
EXPTIME = 20.000
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
SExtractor output filtering results:
* passed selection: 154
* rejected as having no flux measurement: 0
* rejected as having SNR<3.0: 0
* rejected inside rectangles defined in bad_region.lst: 0
* rejected close to frame edge: 0
* rejected as being too small (<1.7 pix): 0
* rejected as being too large (>6.8 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 0
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
154 * detected, using 100/ 154 * for reference/current image matching, fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
refining the coordinate transformation... [CVPOLY iter 1: order=3 pairs=148 inliers=148 rms 3.89 -> 0.80 pix, max corner correction 18.7 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
153 * matched, [CVPOLY iter 2: order=3 pairs=153 inliers=153 rms 0.55 -> 0.31 pix, max corner correction 4.0 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
153 * matched (2nd iteration). [CVPOLY iter 3: order=1 pairs=153 inliers=153 rms 0.31 -> 0.31 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
153 * matched (3rd iteration). Success!
rotation [degrees] = -6.417
154 stars detected, 153 stars matched
Performing magnitude calibration using automatically selected comparison stars
Expecting to find at least 40 * for magnitude calibration
We have N_good_stars = 13, N_manually_selected_comparison_stars = 0
get_detection_limit_sn(): Detection limit: -8.80
[01;31m ERROR!!! Magnitude calibration failure. Dropping image. [33;00m
30827 objects stored in memory (1000000 max.)
memory: 240992 kB used, 249956 kB peak, 65263848 kB available RAM
processed 3 of 4 images ( 75.0%)
Processing /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
9576x6388 FITS image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
Trying to guess the time system by parsing the comment string 'Time of observation (UTC)'
Time system set from the comment to DATE-OBS keyword: 'Time of observation (UTC)'
The input time system is identified as: UTC (blank if unknown)
Setting observation date using DATE-OBS keyword: 2026-08-06T08:48:43.8282620
Setting observation time using DATE-OBS keyword: 2026-08-06T08:48:43.8282620
Observing time converted to the "standard" FITS header format:
DATE-OBS= 2026-08-06T08:48:43.828
EXPTIME = 20.000
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
SExtractor output filtering results:
* passed selection: 143
* rejected as having no flux measurement: 0
* rejected as having SNR<3.0: 0
* rejected inside rectangles defined in bad_region.lst: 0
* rejected close to frame edge: 0
* rejected as being too small (<1.7 pix): 0
* rejected as being too large (>6.7 pix): 0
* rejected as outliers in mag-size plot: 0
* rejected as having SExtractor flags > 99 and <= 7: 0
* rejected as having hopelessly bad SExtractor flags (>7): 0
* rejected due to an external image flag: 0
* rejected as having bad PSF fit: 0
---
You may change some of the filtering parameters by editing src/vast_limits.h and re-running 'make'.
143 * detected, using 100/ 143 * for reference/current image matching, fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
refining the coordinate transformation... [CVPOLY iter 1: order=2 pairs=129 inliers=129 rms 3.18 -> 1.66 pix, max corner correction 13.4 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
141 * matched, [CVPOLY iter 2: order=3 pairs=141 inliers=141 rms 1.98 -> 0.30 pix, max corner correction 12.8 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
142 * matched (2nd iteration). [CVPOLY iter 3: order=1 pairs=142 inliers=142 rms 0.32 -> 0.32 pix, max corner correction 0.0 pix] fraction_of_ambiguous_matches= 0.000000, number_of_ambiguous_matches=0
142 * matched (3rd iteration). Success!
rotation [degrees] = -6.469
143 stars detected, 142 stars matched
Performing magnitude calibration using automatically selected comparison stars
Expecting to find at least 40 * for magnitude calibration
We have N_good_stars = 13, N_manually_selected_comparison_stars = 0
get_detection_limit_sn(): Detection limit: -8.79
[01;31m ERROR!!! Magnitude calibration failure. Dropping image. [33;00m
30827 objects stored in memory (1000000 max.)
memory: 248804 kB used, 249956 kB peak, 65263848 kB available RAM
processed 4 of 4 images (100.0%)
TIMING matching_and_photometry: 1 seconds
Done with measurements! =)
Total number of measurements 54650 (54650 measurements stored in RAM)
Freeing up some memory... Sorting the measurements cached in memory...
Writing lightcurve (outNNNNN.dat) files...
TIMING lightcurve_write: 1 seconds
The lightcurve files have been written, freeing up more memory...
Creating vast_image_details.log ...
Writing summary file: vast_summary.log ... OK
Selecting the best aperture for each source
Aperture with index 0 (REFERENCE_APERTURE_DIAMETER +0.00*REFERENCE_APERTURE_DIAMETER) seems best for 4952 stars
Aperture with index 1 (REFERENCE_APERTURE_DIAMETER +0.00*REFERENCE_APERTURE_DIAMETER) seems best for 0 stars
Aperture with index 2 (REFERENCE_APERTURE_DIAMETER -0.10*REFERENCE_APERTURE_DIAMETER) seems best for 8413 stars
Aperture with index 3 (REFERENCE_APERTURE_DIAMETER +0.10*REFERENCE_APERTURE_DIAMETER) seems best for 2630 stars
Aperture with index 4 (REFERENCE_APERTURE_DIAMETER +0.20*REFERENCE_APERTURE_DIAMETER) seems best for 2481 stars
Aperture with index 5 (REFERENCE_APERTURE_DIAMETER +0.30*REFERENCE_APERTURE_DIAMETER) seems best for 5347 stars
done! =)
TIMING select_aperture: 1 seconds
WARNING: Can't open candidates-transients.lst for reading! -- No candidates found?
Non-zero exit code of lib/transient_list
ERROR running lib/create_list_of_candidate_transients.sh
Computing lightcurve statistics... Will not compute variability indexes for objects having <1 points in lightcurve
You may disable this by commenting out the line '#define DROP_LIGHTCURVES_WITH_SMALL_NUMBER_OF_POINTS_FROM_ALL_PLOTS' in src/vast_limits.h an re-compiling VaST with 'make'
Computing, please wait a bit
............................................................................................................................................................................................................................................
vast_lightcurve_statistics.log: 23623 objects, the longest string is 385 bytes.
Allocating memory for resorting the file.
----***** VaST processing WARNING *****----
You asked VaST to process 4 images, but only 1 were actually matched to the reference one.
Please investigate this!
**************************************************************
This error might be a bug, but it is far more likely that it is caused by
inappropriate input data. A few simple things to check in the diagnostic
messages printed above (or the vast*.log files):
* How many of the input images are matched?
* Does the number of detected stars on each image look reasonable?
* Do images have a sufficient overlap of at least about 20 percent?
You may run
./sextract_single_image /path/to/my/image/file.fit
to see how well VaST detects stars with the current SExtractor settings
(star detection settings can be changed in the default.sex configuration
file, see various examples in the VaST directory).
If you cannot identify the problem, please e-mail Kirill Sokolovsky
Please try to describe the problem in details and, if possible, attach vast_summary.log
file and a few example images. If the images are too big to be sent by e-mail, please
upload them through a web-form http://scan.sai.msu.ru/upload/
**************************************************************
Low percentage of matched images - we'll declare this an unsuccessful VaST run (exit code 1)
_____________________
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.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/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
Last image: 2461258.86672188 06.08.2026 08:47:54.770 UTC
ERROR running VaST on the field Aur-03-Q1b1x1 (less than 4 images processed)
exp_start= 18.01.2026 02:41:07.318 exp= 20.000 JD= 2461058.61200600 ap= 6.2 rotation= 0.000 *detected= 27695 *matched= 27695 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
exp_start= 22.02.2026 02:50:53.978 exp= 20.000 JD= 2461093.61879604 ap= 6.1 rotation= 174.730 *detected= 26955 *matched= 23823 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
exp_start= 06.08.2026 08:47:54.770 exp= 20.000 JD= 2461258.86672188 ap= 6.8 rotation= -6.417 *detected= 154 *matched= 153 status=ERROR /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
exp_start= 06.08.2026 08:48:43.828 exp= 20.000 JD= 2461258.86728968 ap= 6.7 rotation= -6.469 *detected= 143 *matched= 142 status=ERROR /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.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: 2461258.86672188
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_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
NOT SAVING wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
NOT SAVING wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits exists and is non-empty
NOT SAVING wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits exists and is non-empty
NOT SAVING wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:16.998 +37:59:58.58 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:14.036 +37:59:22.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:16.998 +37:59:58.58
Second-epoch image center 05:27:14.036 +37:59:22.05
Angular distance between the image centers 0.0141 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
Image size: 944.9'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:16.897 +37:58:51.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:16.998 +37:59:58.58
Second-epoch image center 05:27:16.897 +37:58:51.56
Angular distance between the image centers 0.0186 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 05:27:14.036 +37:59:22.05
Second-epoch second image center 05:27:16.897 +37:58:51.56
Angular distance between the image centers 0.01265 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.6jgbWPhWri
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.Thw3gIf7ED
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits &> /tmp/tmp.A94f9liSSV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits &> /tmp/tmp.UHY9zeQeoa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.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_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
The reference image (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat) found
'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat' -> 'wcsmag.cat'
Read 202315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8143 to 92.1485 deg, Dec +31.9880 to +43.3918 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 70.8143 to 92.1485 deg, Dec 31.9880 to 43.3918 deg
Loaded 16061 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): 8339 out of 12799 total matches.
Matched with Tycho-2 12799 out of 202315 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.787200
a=0.000000 b=1.000000 c=22.787200
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 202315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8143 to 92.1485 deg, Dec +31.9880 to +43.3918 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 70.8143 to 92.1485 deg, Dec 31.9880 to 43.3918 deg
Loaded 16061 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): 8339 out of 12799 total matches.
Matched with Tycho-2 12799 out of 202315 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (aperture=4.7)
Read 212259 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3331 to 92.7203 deg, Dec +32.1392 to +43.3198 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 71.3331 to 92.7203 deg, Dec 32.1392 to 43.3198 deg
Loaded 16048 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): 8212 out of 12990 total matches.
Matched with Tycho-2 12990 out of 212259 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 189 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
1.9 pix Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
2.6 pix fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
2.7 pix fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
Limiting magnitude estimates:
15.4 mag. Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
15.4 mag. Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
10.3 mag. fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
10.2 mag. fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
All-image limiting magnitude estimate: 10.2 (SNR ) 10.0 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.6jgbWPhWri (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_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/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_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_Aur-03-Q1b1x1_2026-01-17_20-41-07_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/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=30655, bad_region=1, passed=202260
Got 202260 stars (including 171302 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
util/solve_plate_with_UCAC5 got 202260 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 4824 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 202260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 202260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 202260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4823 stars left (next iteration limit 5306)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits N_match=4823 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.468 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.350 sigma_q4_arcsec=0.308 n_q1=927 n_q2=1360 n_q3=1306 n_q4=1230 worst_quadrant_to_overall_ratio=1.304
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Thw3gIf7ED (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=32150, bad_region=8, passed=212204
Got 212204 stars (including 179717 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
util/solve_plate_with_UCAC5 got 212204 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 4822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 212204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 212204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 212204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4819 stars left (next iteration limit 5303)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits N_match=4819 sigma_overall_arcsec=0.482 sigma_q1_arcsec=0.573 sigma_q2_arcsec=0.484 sigma_q3_arcsec=0.442 sigma_q4_arcsec=0.412 n_q1=1096 n_q2=1410 n_q3=1324 n_q4=989 worst_quadrant_to_overall_ratio=1.189
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.A94f9liSSV (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_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.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_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=30, bad_region=1, passed=1935
Got 1935 stars (including 1900 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat
util/solve_plate_with_UCAC5 got 1935 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 1838 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1797 matched stars entering correct_measured_positions(), 1774 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1797 matched stars entering correct_measured_positions(), 1904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.23"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 1837 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1797 matched stars entering correct_measured_positions(), 1905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.32"
Accuracy estimation diagnostic: 1797 matched stars entering correct_measured_positions(), 1905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.33"
Excluding outliers - 1797 stars left (next iteration limit 1976)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1797 robust_rms=7.230 arcsec worst_quadrant_rms=9.489 arcsec
SIP_REFIT: SIP order 3 trial: matched=1797 robust_rms=1.556 arcsec worst_quadrant_rms=1.976 arcsec
SIP_REFIT: SIP order 5 trial: matched=1797 robust_rms=1.207 arcsec worst_quadrant_rms=1.262 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1797 robust_rms_before=2.019 arcsec robust_rms_before_corrected=1.344 arcsec robust_rms_after=1.207 arcsec worst_quadrant_rms_before=1.453 worst_quadrant_rms_after=1.262
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
Image size: 945.4'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:14.195 +37:59:20.09 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1935 stars ###
'wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/correct_sextractor_wcs_catalog_usingxy2sky2680283.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 2.019 -> 1.207 arcsec)
WCS_QUALITY_DIAG: file=fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits N_match=1797 sigma_overall_arcsec=1.139 sigma_q1_arcsec=1.130 sigma_q2_arcsec=1.278 sigma_q3_arcsec=1.043 sigma_q4_arcsec=1.019 n_q1=561 n_q2=662 n_q3=425 n_q4=149 worst_quadrant_to_overall_ratio=1.121
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits -region wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.UHY9zeQeoa (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_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.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_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=31, bad_region=1, passed=1637
Got 1637 stars (including 1603 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat
util/solve_plate_with_UCAC5 got 1637 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.9'
Seting catalog search parameters based on the expected field of view 944.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013124 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010499 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 1545 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1511 matched stars entering correct_measured_positions(), 1492 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1511 matched stars entering correct_measured_positions(), 1610 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 1544 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1512 matched stars entering correct_measured_positions(), 1609 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.37"
Accuracy estimation diagnostic: 1511 matched stars entering correct_measured_positions(), 1609 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.37"
Excluding outliers - 1511 stars left (next iteration limit 1662)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1511 robust_rms=7.950 arcsec worst_quadrant_rms=9.934 arcsec
SIP_REFIT: SIP order 3 trial: matched=1511 robust_rms=1.473 arcsec worst_quadrant_rms=1.850 arcsec
SIP_REFIT: SIP order 5 trial: matched=1511 robust_rms=1.249 arcsec worst_quadrant_rms=1.382 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1511 robust_rms_before=2.002 arcsec robust_rms_before_corrected=1.426 arcsec robust_rms_after=1.249 arcsec worst_quadrant_rms_before=1.652 worst_quadrant_rms_after=1.382
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
Image size: 945.3'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:17.061 +37:58:49.46 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1637 stars ###
'wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/correct_sextractor_wcs_catalog_usingxy2sky2680326.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 2.002 -> 1.249 arcsec)
WCS_QUALITY_DIAG: file=fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits N_match=1511 sigma_overall_arcsec=1.159 sigma_q1_arcsec=1.138 sigma_q2_arcsec=1.335 sigma_q3_arcsec=0.925 sigma_q4_arcsec=1.224 n_q1=453 n_q2=620 n_q3=309 n_q4=129 worst_quadrant_to_overall_ratio=1.152
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits -region wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-47-54_20.00sec_-0.00C_LIGHTs_0354.fits'
Saving fully-calibrated image wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Aur-03-Q1b1x1_035035_TTUQ1b1x1_2626564_0PvfRzL0/wcs_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355.fits'
Preparing the HTML report for the field Aur-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:35.01 +35:49:53.0: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:04.82 +35:37:44.5: 9.25 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:10.96 +36:02:59.8: 9.22 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:58:08.47 +34:07:07.1: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:05:23.55 +36:21:51.1: 9.41 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:23.02 +35:35:37.5: 9.69 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:35.01 +35:49:53.0: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:03:35.01 +35:49:53.0: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:10.96 +36:02:59.8: 9.27 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:04.82 +35:37:44.5: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:58:08.47 +34:07:07.1: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:02:04.82 +35:37:44.5: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry filter REJECTED candidate at 05:58:08.47 +34:07:07.1: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry reference-image weighted average: 9.25 +/- 0.00
Forced photometry filter REJECTED candidate at 06:04:10.96 +36:02:59.8: ref_mag=9.25 +/- 0.00 new_mean_mag=8.5938 delta=0.66 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:21.49 +36:11:36.0: 9.65 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:47.87 +36:25:03.6: 9.18 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:55:53.50 +34:21:24.8: 9.51 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:44.66 +34:55:15.5: 9.56 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:05:23.55 +36:21:51.1: 9.47 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.44 +/- 0.00
Forced photometry filter REJECTED candidate at 06:05:23.55 +36:21:51.1: ref_mag=9.44 +/- 0.00 new_mean_mag=8.7690 delta=0.67 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:23.02 +35:35:37.5: 9.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.71 +/- 0.00
Forced photometry filter REJECTED candidate at 06:01:23.02 +35:35:37.5: ref_mag=9.71 +/- 0.00 new_mean_mag=8.8926 delta=0.82 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:21.49 +36:11:36.0: 9.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.68 +/- 0.00
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:47.87 +36:25:03.6: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:03:47.87 +36:25:03.6: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry filter REJECTED candidate at 06:03:21.49 +36:11:36.0: ref_mag=9.68 +/- 0.00 new_mean_mag=8.9018 delta=0.77 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:55:53.50 +34:21:24.8: 9.52 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:44.66 +34:55:15.5: 9.59 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.52 +/- 0.00
Forced photometry reference-image weighted average: 9.58 +/- 0.00
Forced photometry filter REJECTED candidate at 05:55:53.50 +34:21:24.8: ref_mag=9.52 +/- 0.00 new_mean_mag=9.0399 delta=0.48 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:57:44.66 +34:55:15.5: ref_mag=9.58 +/- 0.00 new_mean_mag=9.0836 delta=0.49 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:59:31.31 +34:30:09.0: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:44.53 +34:38:46.8: 9.50 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:55.00 +34:54:40.1: 10.22 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:54.71 +35:44:30.6: 9.58 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:03.71 +34:03:25.1: 9.12 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:59:31.31 +34:30:09.0: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:59:31.31 +34:30:09.0: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:44.53 +34:38:46.8: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:44.80 +35:25:19.3: 9.07 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 05:57:44.53 +34:38:46.8: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:28.10 +36:11:43.7: 10.19 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:53:34.26 +34:18:19.3: 9.70 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:28.45 +36:08:41.3: 10.06 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:55.00 +34:54:40.1: 10.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.23 +/- 0.00
Forced photometry filter KEPT candidate at 05:57:55.00 +34:54:40.1: ref_mag=10.23 +/- 0.00 new_mean_mag=9.0846 delta=1.14 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:54.71 +35:44:30.6: 9.65 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.61 +/- 0.00
Forced photometry filter REJECTED candidate at 06:01:54.71 +35:44:30.6: ref_mag=9.61 +/- 0.00 new_mean_mag=9.0031 delta=0.61 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:03.71 +34:03:25.1: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:51:03.71 +34:03:25.1: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:52:36.24 +33:51:27.2: 9.42 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:44.80 +35:25:19.3: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:04:44.80 +35:25:19.3: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:28.10 +36:11:43.7: 10.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.21 +/- 0.00
Forced photometry filter KEPT candidate at 06:01:28.10 +36:11:43.7: ref_mag=10.21 +/- 0.00 new_mean_mag=9.0824 delta=1.13 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:53:34.26 +34:18:19.3: 9.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.70 +/- 0.00
Forced photometry filter REJECTED candidate at 05:53:34.26 +34:18:19.3: ref_mag=9.70 +/- 0.00 new_mean_mag=9.2500 delta=0.45 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:28.45 +36:08:41.3: 10.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.08 +/- 0.00
Forced photometry filter KEPT candidate at 06:04:28.45 +36:08:41.3: ref_mag=10.08 +/- 0.00 new_mean_mag=9.1370 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:52.97 +33:49:42.1: 9.46 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:04.79 +34:01:48.5: 9.58 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:52:36.24 +33:51:27.2: 9.44 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.43 +/- 0.00
Forced photometry filter REJECTED candidate at 05:52:36.24 +33:51:27.2: ref_mag=9.43 +/- 0.00 new_mean_mag=9.3001 delta=0.13 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:43.18 +34:05:49.9: 9.48 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:47:07.62 +33:00:39.7: 9.83 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:52.97 +33:49:42.1: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:57:52.97 +33:49:42.1: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:04.79 +34:01:48.5: 9.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.64 +/- 0.00
Forced photometry filter REJECTED candidate at 05:54:04.79 +34:01:48.5: ref_mag=9.64 +/- 0.00 new_mean_mag=9.3656 delta=0.27 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:56.10 +33:41:17.3: 9.85 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:43.18 +34:05:49.9: 9.49 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.48 +/- 0.00
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:47:07.62 +33:00:39.7: 9.81 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 05:51:43.18 +34:05:49.9: ref_mag=9.48 +/- 0.00 new_mean_mag=9.2633 delta=0.22 (need > 0.90)
Forced photometry reference-image weighted average: 9.82 +/- 0.00
Forced photometry filter REJECTED candidate at 05:47:07.62 +33:00:39.7: ref_mag=9.82 +/- 0.00 new_mean_mag=9.4814 delta=0.34 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:13.76 +33:52:37.4: 10.36 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:30.57 +35:08:40.5: 10.67 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:56.10 +33:41:17.3: 9.85 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.85 +/- 0.00
Forced photometry filter REJECTED candidate at 05:51:56.10 +33:41:17.3: ref_mag=9.85 +/- 0.00 new_mean_mag=9.3979 delta=0.45 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:52.91 +36:53:44.9: 10.19 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:13.76 +33:52:37.4: 10.41 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.39 +/- 0.00
Forced photometry filter KEPT candidate at 05:56:13.76 +33:52:37.4: ref_mag=10.39 +/- 0.00 new_mean_mag=9.3176 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:30.57 +35:08:40.5: 10.66 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.66 +/- 0.00
Forced photometry filter KEPT candidate at 05:56:30.57 +35:08:40.5: ref_mag=10.66 +/- 0.00 new_mean_mag=9.3063 delta=1.36 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:49:27.54 +33:38:21.1: 10.08 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:05:08.33 +36:24:15.1: 10.12 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:45:56.64 +32:55:52.9: 10.16 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:52.91 +36:53:44.9: 10.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.23 +/- 0.00
Forced photometry filter KEPT candidate at 06:04:52.91 +36:53:44.9: ref_mag=10.23 +/- 0.00 new_mean_mag=9.1813 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:54.02 +34:44:46.5: 9.92 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:44.45 +35:46:35.0: 10.45 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:49:27.54 +33:38:21.1: 10.08 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:05:08.33 +36:24:15.1: 10.18 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.08 +/- 0.00
Forced photometry reference-image weighted average: 10.15 +/- 0.00
Forced photometry filter REJECTED candidate at 05:49:27.54 +33:38:21.1: ref_mag=10.08 +/- 0.00 new_mean_mag=9.4717 delta=0.61 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:05:08.33 +36:24:15.1: ref_mag=10.15 +/- 0.00 new_mean_mag=9.2606 delta=0.89 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:45:56.64 +32:55:52.9: 10.17 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.17 +/- 0.00
Forced photometry filter REJECTED candidate at 05:45:56.64 +32:55:52.9: ref_mag=10.17 +/- 0.00 new_mean_mag=9.6582 delta=0.51 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:48.83 +33:36:50.7: 10.28 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:08.97 +34:37:37.6: 10.21 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:54.02 +34:44:46.5: 9.96 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:44.45 +35:46:35.0: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.94 +/- 0.00
Forced photometry filter REJECTED candidate at 05:57:54.02 +34:44:46.5: ref_mag=9.94 +/- 0.00 new_mean_mag=9.2411 delta=0.70 (need > 0.90)
Forced photometry reference-image weighted average: 10.49 +/- 0.00
Forced photometry filter KEPT candidate at 06:04:44.45 +35:46:35.0: ref_mag=10.49 +/- 0.00 new_mean_mag=9.1369 delta=1.35 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:48.83 +33:36:50.7: 10.36 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.32 +/- 0.00
Forced photometry filter REJECTED candidate at 05:51:48.83 +33:36:50.7: ref_mag=10.32 +/- 0.00 new_mean_mag=9.5129 delta=0.81 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:08.97 +34:37:37.6: 10.23 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:55:13.40 +34:02:54.5: 10.85 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:58:57.15 +34:57:59.1: 10.00 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.22 +/- 0.00
Forced photometry filter REJECTED candidate at 05:56:08.97 +34:37:37.6: ref_mag=10.22 +/- 0.00 new_mean_mag=9.5020 delta=0.72 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:43.51 +34:12:53.3: 10.09 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:52:58.56 +34:15:22.2: 9.74 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:55:13.40 +34:02:54.5: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry filter KEPT candidate at 05:55:13.40 +34:02:54.5: ref_mag=10.83 +/- 0.00 new_mean_mag=9.3568 delta=1.47 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:58:57.15 +34:57:59.1: 10.05 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.03 +/- 0.00
Forced photometry filter REJECTED candidate at 05:58:57.15 +34:57:59.1: ref_mag=10.03 +/- 0.00 new_mean_mag=9.3211 delta=0.71 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:43.51 +34:12:53.3: 10.14 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.12 +/- 0.00
Forced photometry filter REJECTED candidate at 05:56:43.51 +34:12:53.3: ref_mag=10.12 +/- 0.00 new_mean_mag=9.4708 delta=0.65 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:59:42.94 +35:21:51.5: 10.76 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:31.50 +34:33:26.8: 9.78 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:52:58.56 +34:15:22.2: 9.74 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.74 +/- 0.00
Forced photometry filter REJECTED candidate at 05:52:58.56 +34:15:22.2: ref_mag=9.74 +/- 0.00 new_mean_mag=9.4652 delta=0.28 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:47.20 +33:04:44.3: 9.18 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:58:45.16 +34:36:01.4: 10.17 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:59:42.94 +35:21:51.5: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.79 +/- 0.00
Forced photometry filter KEPT candidate at 05:59:42.94 +35:21:51.5: ref_mag=10.79 +/- 0.00 new_mean_mag=9.4222 delta=1.36 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:17.73 +33:10:01.6: 9.66 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:31.50 +34:33:26.8: 9.80 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:50:38.56 +33:02:45.9: 10.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.79 +/- 0.00
Forced photometry filter REJECTED candidate at 05:54:31.50 +34:33:26.8: ref_mag=9.79 +/- 0.00 new_mean_mag=9.3573 delta=0.43 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:09.82 +34:31:18.2: 9.89 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:58:45.16 +34:36:01.4: 10.24 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:47.20 +33:04:44.3: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:54:47.20 +33:04:44.3: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry reference-image weighted average: 10.21 +/- 0.00
Forced photometry filter REJECTED candidate at 05:58:45.16 +34:36:01.4: ref_mag=10.21 +/- 0.00 new_mean_mag=9.3873 delta=0.82 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:17.73 +33:10:01.6: 9.67 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.66 +/- 0.00
Forced photometry filter REJECTED candidate at 05:54:17.73 +33:10:01.6: ref_mag=9.66 +/- 0.00 new_mean_mag=9.3569 delta=0.31 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:50:38.56 +33:02:45.9: 10.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.23 +/- 0.00
Forced photometry filter REJECTED candidate at 05:50:38.56 +33:02:45.9: ref_mag=10.23 +/- 0.00 new_mean_mag=9.6409 delta=0.59 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:09.82 +34:31:18.2: 9.90 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.90 +/- 0.00
Forced photometry filter REJECTED candidate at 05:54:09.82 +34:31:18.2: ref_mag=9.90 +/- 0.00 new_mean_mag=9.4770 delta=0.42 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:11.32 +40:22:16.7: 9.13 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:17.20 +34:09:46.3: 9.25 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:55:13.82 +35:00:44.8: 9.79 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:29.19 +34:05:14.8: 9.74 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:11.32 +40:22:16.7: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:00:11.32 +40:22:16.7: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:22.26 +34:47:27.4: 9.31 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:17.20 +34:09:46.3: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:00:17.20 +34:09:46.3: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:45.24 +34:34:52.9: 11.09 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:50:10.77 +33:08:46.9: 10.03 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:50.97 +34:06:09.8: 10.36 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:55:13.82 +35:00:44.8: 9.82 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:29.19 +34:05:14.8: 9.76 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.81 +/- 0.00
Forced photometry filter REJECTED candidate at 05:55:13.82 +35:00:44.8: ref_mag=9.81 +/- 0.00 new_mean_mag=9.4514 delta=0.35 (need > 0.90)
Forced photometry reference-image weighted average: 9.75 +/- 0.00
Forced photometry filter REJECTED candidate at 05:51:29.19 +34:05:14.8: ref_mag=9.75 +/- 0.00 new_mean_mag=9.5141 delta=0.24 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:22.26 +34:47:27.4: 9.34 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.32 +/- 0.00
Forced photometry filter REJECTED candidate at 06:02:22.26 +34:47:27.4: ref_mag=9.32 +/- 0.00 new_mean_mag=9.1410 delta=0.18 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:45.24 +34:34:52.9: 11.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.10 +/- 0.00
Forced photometry filter KEPT candidate at 05:56:45.24 +34:34:52.9: ref_mag=11.10 +/- 0.00 new_mean_mag=9.5511 delta=1.55 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:50:10.77 +33:08:46.9: 10.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.03 +/- 0.00
Forced photometry filter REJECTED candidate at 05:50:10.77 +33:08:46.9: ref_mag=10.03 +/- 0.00 new_mean_mag=9.7629 delta=0.27 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:50.97 +34:06:09.8: 10.38 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.37 +/- 0.00
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:18.23 +35:58:01.6: 10.39 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 05:54:50.97 +34:06:09.8: ref_mag=10.37 +/- 0.00 new_mean_mag=9.4720 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:51.24 +36:13:11.2: 10.65 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:33.25 +35:36:39.7: 10.90 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:18.23 +35:58:01.6: 10.42 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.41 +/- 0.00
Forced photometry filter KEPT candidate at 06:00:18.23 +35:58:01.6: ref_mag=10.41 +/- 0.00 new_mean_mag=9.4728 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:52:34.61 +33:11:05.2: 10.52 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:51.24 +36:13:11.2: 10.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.69 +/- 0.00
Forced photometry filter KEPT candidate at 06:01:51.24 +36:13:11.2: ref_mag=10.69 +/- 0.00 new_mean_mag=9.4754 delta=1.21 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:02.51 +35:39:34.5: 10.71 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:53:45.81 +33:17:12.0: 10.24 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:52:59.42 +34:13:32.8: 10.18 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:05:01.51 +35:59:48.9: 11.10 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:33.25 +35:36:39.7: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.93 +/- 0.00
Forced photometry filter KEPT candidate at 06:02:33.25 +35:36:39.7: ref_mag=10.93 +/- 0.00 new_mean_mag=9.5272 delta=1.40 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:52:34.61 +33:11:05.2: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.52 +/- 0.00
Forced photometry filter REJECTED candidate at 05:52:34.61 +33:11:05.2: ref_mag=10.52 +/- 0.00 new_mean_mag=9.7051 delta=0.82 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:53:45.81 +33:17:12.0: 10.23 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:02.51 +35:39:34.5: 10.80 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.23 +/- 0.00
Forced photometry reference-image weighted average: 10.75 +/- 0.00
Forced photometry filter REJECTED candidate at 05:53:45.81 +33:17:12.0: ref_mag=10.23 +/- 0.00 new_mean_mag=9.7186 delta=0.52 (need > 0.90)
Forced photometry filter KEPT candidate at 06:04:02.51 +35:39:34.5: ref_mag=10.75 +/- 0.00 new_mean_mag=9.3910 delta=1.36 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:52:59.42 +34:13:32.8: 10.18 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:05:01.51 +35:59:48.9: 11.20 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.18 +/- 0.00
Forced photometry reference-image weighted average: 11.15 +/- 0.00
Forced photometry filter REJECTED candidate at 05:52:59.42 +34:13:32.8: ref_mag=10.18 +/- 0.00 new_mean_mag=9.5805 delta=0.60 (need > 0.90)
Forced photometry filter KEPT candidate at 06:05:01.51 +35:59:48.9: ref_mag=11.15 +/- 0.00 new_mean_mag=9.4645 delta=1.68 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:42.85 +35:32:35.6: 10.37 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:23.02 +35:16:32.0: 10.52 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:07.33 +36:03:44.2: 10.43 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:42.85 +35:32:35.6: 10.42 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.40 +/- 0.00
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:58:16.03 +35:24:08.4: 10.53 +/- 0.00 detection
Forced photometry filter KEPT candidate at 06:02:42.85 +35:32:35.6: ref_mag=10.40 +/- 0.00 new_mean_mag=9.3789 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:23.02 +35:16:32.0: 10.57 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.54 +/- 0.00
Forced photometry filter KEPT candidate at 05:57:23.02 +35:16:32.0: ref_mag=10.54 +/- 0.00 new_mean_mag=9.5873 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:07.33 +36:03:44.2: 10.48 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.45 +/- 0.00
Forced photometry filter KEPT candidate at 06:01:07.33 +36:03:44.2: ref_mag=10.45 +/- 0.00 new_mean_mag=9.4920 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:58:16.03 +35:24:08.4: 10.61 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.57 +/- 0.00
Forced photometry filter KEPT candidate at 05:58:16.03 +35:24:08.4: ref_mag=10.57 +/- 0.00 new_mean_mag=9.5598 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:35.19 +35:43:41.4: 10.82 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:31.31 +33:53:26.8: 9.84 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:35.19 +35:43:41.4: 10.87 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.85 +/- 0.00
Forced photometry filter KEPT candidate at 06:03:35.19 +35:43:41.4: ref_mag=10.85 +/- 0.00 new_mean_mag=9.4027 delta=1.45 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:31.31 +33:53:26.8: 9.88 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.86 +/- 0.00
Forced photometry filter REJECTED candidate at 05:57:31.31 +33:53:26.8: ref_mag=9.86 +/- 0.00 new_mean_mag=9.3947 delta=0.47 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:59:43.16 +35:20:41.8: 10.81 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:52.66 +35:13:24.3: 10.53 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:53:46.01 +33:37:21.0: 10.39 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:18.81 +33:32:29.5: 10.17 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:59:43.16 +35:20:41.8: 10.84 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry filter KEPT candidate at 05:59:43.16 +35:20:41.8: ref_mag=10.83 +/- 0.00 new_mean_mag=9.6317 delta=1.19 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:52.66 +35:13:24.3: 10.56 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.55 +/- 0.00
Forced photometry filter KEPT candidate at 05:57:52.66 +35:13:24.3: ref_mag=10.55 +/- 0.00 new_mean_mag=9.5610 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:53:46.01 +33:37:21.0: 10.43 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.41 +/- 0.00
Forced photometry filter REJECTED candidate at 05:53:46.01 +33:37:21.0: ref_mag=10.41 +/- 0.00 new_mean_mag=9.7493 delta=0.66 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:05:52.01 +37:01:08.4: 10.38 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:18.81 +33:32:29.5: 10.18 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.17 +/- 0.00
Forced photometry filter REJECTED candidate at 05:54:18.81 +33:32:29.5: ref_mag=10.17 +/- 0.00 new_mean_mag=9.5832 delta=0.59 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:05:52.01 +37:01:08.4: 10.44 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.41 +/- 0.00
Forced photometry filter REJECTED candidate at 06:05:52.01 +37:01:08.4: ref_mag=10.41 +/- 0.00 new_mean_mag=9.5226 delta=0.89 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:37.27 +36:03:21.7: 10.99 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:58.59 +34:57:23.2: 10.49 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:37.27 +36:03:21.7: 11.05 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.02 +/- 0.00
Forced photometry filter KEPT candidate at 06:03:37.27 +36:03:21.7: ref_mag=11.02 +/- 0.00 new_mean_mag=9.5483 delta=1.47 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:46:17.09 +32:52:23.7: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:58.59 +34:57:23.2: 10.50 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.50 +/- 0.00
Forced photometry filter REJECTED candidate at 05:54:58.59 +34:57:23.2: ref_mag=10.50 +/- 0.00 new_mean_mag=9.7422 delta=0.76 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:46:17.09 +32:52:23.7: 10.42 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 05:46:17.09 +32:52:23.7: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:52.05 +33:08:52.9: 10.79 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:03.07 +34:34:33.6: 10.67 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:17.50 +34:52:04.9: 10.83 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:52.05 +33:08:52.9: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.80 +/- 0.00
Forced photometry filter KEPT candidate at 05:51:52.05 +33:08:52.9: ref_mag=10.80 +/- 0.00 new_mean_mag=9.8755 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:03.07 +34:34:33.6: 10.66 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.66 +/- 0.00
Forced photometry filter KEPT candidate at 05:56:03.07 +34:34:33.6: ref_mag=10.66 +/- 0.00 new_mean_mag=9.7467 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:17.50 +34:52:04.9: 10.85 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.84 +/- 0.00
Forced photometry filter KEPT candidate at 05:57:17.50 +34:52:04.9: ref_mag=10.84 +/- 0.00 new_mean_mag=9.8319 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:53:02.03 +33:16:19.0: 10.53 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:50.38 +34:27:28.2: 10.50 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:53:02.03 +33:16:19.0: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.53 +/- 0.00
Forced photometry filter REJECTED candidate at 05:53:02.03 +33:16:19.0: ref_mag=10.53 +/- 0.00 new_mean_mag=9.8427 delta=0.69 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:49:50.82 +33:27:31.3: 10.30 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:50.38 +34:27:28.2: 10.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.51 +/- 0.00
Forced photometry filter REJECTED candidate at 05:56:50.38 +34:27:28.2: ref_mag=10.51 +/- 0.00 new_mean_mag=9.7606 delta=0.74 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:49:50.82 +33:27:31.3: 10.32 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.31 +/- 0.00
Forced photometry filter REJECTED candidate at 05:49:50.82 +33:27:31.3: ref_mag=10.31 +/- 0.00 new_mean_mag=9.8804 delta=0.43 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:50:59.27 +33:00:40.1: 10.33 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:58:52.68 +32:50:12.3: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:55:00.08 +34:30:33.2: 10.98 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:50:59.27 +33:00:40.1: 10.32 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.32 +/- 0.00
Forced photometry filter REJECTED candidate at 05:50:59.27 +33:00:40.1: ref_mag=10.32 +/- 0.00 new_mean_mag=9.8955 delta=0.43 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:58:52.68 +32:50:12.3: 9.30 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 05:58:52.68 +32:50:12.3: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:55:00.08 +34:30:33.2: 11.02 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.00 +/- 0.00
Forced photometry filter KEPT candidate at 05:55:00.08 +34:30:33.2: ref_mag=11.00 +/- 0.00 new_mean_mag=9.8413 delta=1.16 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:53:57.54 +34:35:54.6: 10.79 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:59:41.24 +35:13:05.3: 10.48 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:53:57.54 +34:35:54.6: 10.81 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.80 +/- 0.00
Forced photometry filter KEPT candidate at 05:53:57.54 +34:35:54.6: ref_mag=10.80 +/- 0.00 new_mean_mag=9.8246 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:59:41.24 +35:13:05.3: 10.51 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.50 +/- 0.00
Forced photometry filter REJECTED candidate at 05:59:41.24 +35:13:05.3: ref_mag=10.50 +/- 0.00 new_mean_mag=9.6221 delta=0.87 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:32.84 +34:39:20.2: 10.45 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:58.13 +36:36:15.0: 10.42 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:32.84 +34:39:20.2: 10.48 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.46 +/- 0.00
Forced photometry filter REJECTED candidate at 05:54:32.84 +34:39:20.2: ref_mag=10.46 +/- 0.00 new_mean_mag=9.7701 delta=0.69 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:58.13 +36:36:15.0: 10.47 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.45 +/- 0.00
Forced photometry filter KEPT candidate at 06:03:58.13 +36:36:15.0: ref_mag=10.45 +/- 0.00 new_mean_mag=9.3472 delta=1.10 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:24.21 +35:00:37.0: 10.93 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:12.07 +33:07:20.0: 10.40 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:24.21 +35:00:37.0: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.95 +/- 0.00
Forced photometry filter KEPT candidate at 05:56:24.21 +35:00:37.0: ref_mag=10.95 +/- 0.00 new_mean_mag=9.8170 delta=1.13 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:12.07 +33:07:20.0: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.40 +/- 0.00
Forced photometry filter REJECTED candidate at 05:51:12.07 +33:07:20.0: ref_mag=10.40 +/- 0.00 new_mean_mag=9.9110 delta=0.49 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:59:55.37 +34:54:11.0: 10.79 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:59:55.37 +34:54:11.0: 10.83 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.81 +/- 0.00
Forced photometry filter KEPT candidate at 05:59:55.37 +34:54:11.0: ref_mag=10.81 +/- 0.00 new_mean_mag=9.7933 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:43.13 +35:02:07.8: 10.51 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:43.13 +35:02:07.8: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.53 +/- 0.00
Forced photometry filter REJECTED candidate at 05:57:43.13 +35:02:07.8: ref_mag=10.53 +/- 0.00 new_mean_mag=9.7913 delta=0.74 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:42.34 +34:26:17.7: 10.61 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:42.34 +34:26:17.7: 10.62 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:59:45.86 +34:51:34.8: 10.62 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.62 +/- 0.00
Forced photometry filter REJECTED candidate at 05:54:42.34 +34:26:17.7: ref_mag=10.62 +/- 0.00 new_mean_mag=9.8506 delta=0.77 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:52.03 +34:09:17.3: 11.33 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:59:45.86 +34:51:34.8: 10.67 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.65 +/- 0.00
Forced photometry filter KEPT candidate at 05:59:45.86 +34:51:34.8: ref_mag=10.65 +/- 0.00 new_mean_mag=9.7067 delta=0.94 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:00.34 +36:34:23.8: 10.80 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:52.03 +34:09:17.3: 11.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.33 +/- 0.00
Forced photometry filter KEPT candidate at 05:51:52.03 +34:09:17.3: ref_mag=11.33 +/- 0.00 new_mean_mag=9.8036 delta=1.52 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:02.97 +33:48:27.2: 10.51 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:00.34 +36:34:23.8: 10.85 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.83 +/- 0.00
Forced photometry filter KEPT candidate at 06:03:00.34 +36:34:23.8: ref_mag=10.83 +/- 0.00 new_mean_mag=9.6526 delta=1.17 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:02.97 +33:48:27.2: 10.53 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.52 +/- 0.00
Forced photometry filter REJECTED candidate at 05:51:02.97 +33:48:27.2: ref_mag=10.52 +/- 0.00 new_mean_mag=9.9111 delta=0.61 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:41.03 +35:24:16.7: 10.63 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:41.03 +35:24:16.7: 10.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.66 +/- 0.00
Forced photometry filter KEPT candidate at 06:00:41.03 +35:24:16.7: ref_mag=10.66 +/- 0.00 new_mean_mag=9.6993 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:32.00 +35:03:33.9: 10.68 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:48:27.03 +33:23:05.6: 11.02 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:32.00 +35:03:33.9: 10.69 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.69 +/- 0.00
Forced photometry filter REJECTED candidate at 05:57:32.00 +35:03:33.9: ref_mag=10.69 +/- 0.00 new_mean_mag=9.8336 delta=0.85 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:48:27.03 +33:23:05.6: 11.04 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.03 +/- 0.00
Forced photometry filter KEPT candidate at 05:48:27.03 +33:23:05.6: ref_mag=11.03 +/- 0.00 new_mean_mag=9.9488 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:32.84 +36:20:22.2: 9.28 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:58:23.55 +38:51:29.5: 10.60 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:32.84 +36:20:22.2: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:02:32.84 +36:20:22.2: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:58:23.55 +38:51:29.5: 10.52 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.56 +/- 0.00
Forced photometry filter KEPT candidate at 04:58:23.55 +38:51:29.5: ref_mag=10.56 +/- 0.00 new_mean_mag=9.6441 delta=0.91 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:46.19 +32:29:28.8: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:46.19 +32:29:28.8: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:56:46.19 +32:29:28.8: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:51.07 +33:09:29.5: 11.06 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:51.07 +33:09:29.5: 11.08 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.07 +/- 0.00
Forced photometry filter KEPT candidate at 05:51:51.07 +33:09:29.5: ref_mag=11.07 +/- 0.00 new_mean_mag=10.0088 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:54.16 +33:17:52.2: 9.19 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:59.71 +35:39:44.6: 10.76 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:54.16 +33:17:52.2: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:51:54.16 +33:17:52.2: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:59.71 +35:39:44.6: 10.80 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.78 +/- 0.00
Forced photometry filter KEPT candidate at 06:02:59.71 +35:39:44.6: ref_mag=10.78 +/- 0.00 new_mean_mag=9.7413 delta=1.04 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:52:29.47 +33:28:17.5: 10.79 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:52:55.03 +33:27:05.0: 10.37 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:52:29.47 +33:28:17.5: 10.79 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.79 +/- 0.00
Forced photometry filter REJECTED candidate at 05:52:29.47 +33:28:17.5: ref_mag=10.79 +/- 0.00 new_mean_mag=9.9482 delta=0.84 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:52:55.03 +33:27:05.0: 10.38 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.38 +/- 0.00
Forced photometry filter REJECTED candidate at 05:52:55.03 +33:27:05.0: ref_mag=10.38 +/- 0.00 new_mean_mag=9.6302 delta=0.75 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:55:04.66 +34:51:20.3: 10.28 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:58:19.26 +34:18:34.8: 9.62 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:55:04.66 +34:51:20.3: 10.27 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.27 +/- 0.00
Forced photometry filter REJECTED candidate at 05:55:04.66 +34:51:20.3: ref_mag=10.27 +/- 0.00 new_mean_mag=9.5327 delta=0.74 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:57:11.69 +33:42:59.5: 9.75 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:58:19.26 +34:18:34.8: 9.67 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.64 +/- 0.00
Forced photometry filter REJECTED candidate at 05:58:19.26 +34:18:34.8: ref_mag=9.64 +/- 0.00 new_mean_mag=9.1154 delta=0.53 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:57:11.69 +33:42:59.5: 9.79 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.77 +/- 0.00
Forced photometry filter REJECTED candidate at 05:57:11.69 +33:42:59.5: ref_mag=9.77 +/- 0.00 new_mean_mag=9.4825 delta=0.29 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:49:02.97 +32:48:51.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:50:37.56 +33:48:28.3: 10.41 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:49:02.97 +32:48:51.2: 9.94 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 05:49:02.97 +32:48:51.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:52:46.45 +32:34:07.6: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:28.72 +32:39:48.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:50:37.56 +33:48:28.3: 10.54 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.47 +/- 0.00
Forced photometry filter KEPT candidate at 05:50:37.56 +33:48:28.3: ref_mag=10.47 +/- 0.00 new_mean_mag=9.2330 delta=1.24 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:53:02.81 +33:09:27.3: 9.26 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:52:46.45 +32:34:07.6: 10.02 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 05:52:46.45 +32:34:07.6: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:28.72 +32:39:48.4: 9.39 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:52:40.60 +32:32:14.4: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 05:56:28.72 +32:39:48.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:53:02.81 +33:09:27.3: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:53:02.81 +33:09:27.3: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:52:40.60 +32:32:14.4: 10.13 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 05:52:40.60 +32:32:14.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:52:47.84 +32:33:00.8: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:51:09.22 +32:51:29.9: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:52:18.74 +32:33:09.6: 99.00 +/- 99.00 edge
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:07.47 +34:45:26.1: 10.66 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:52:47.84 +32:33:00.8: 9.85 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 05:52:47.84 +32:33:00.8: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:51:09.22 +32:51:29.9: 10.04 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 05:51:09.22 +32:51:29.9: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:52:18.74 +32:33:09.6: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 05:52:18.74 +32:33:09.6: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:07.47 +34:45:26.1: 10.70 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.68 +/- 0.00
Forced photometry filter KEPT candidate at 06:00:07.47 +34:45:26.1: ref_mag=10.68 +/- 0.00 new_mean_mag=9.7660 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:02:00.75 +35:51:55.4: 10.06 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:02:00.75 +35:51:55.4: 10.11 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.09 +/- 0.00
Forced photometry filter KEPT candidate at 06:02:00.75 +35:51:55.4: ref_mag=10.09 +/- 0.00 new_mean_mag=9.1686 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:12.10 +35:16:21.0: 9.14 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:09.94 +35:43:18.9: 9.57 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:04:25.93 +35:57:08.5: 9.70 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:23.52 +33:17:38.6: 10.35 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:34.92 +35:05:55.6: 9.34 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:12.10 +35:16:21.0: 9.20 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.17 +/- 0.00
Forced photometry filter REJECTED candidate at 06:01:12.10 +35:16:21.0: ref_mag=9.17 +/- 0.00 new_mean_mag=8.7373 delta=0.44 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:04:25.93 +35:57:08.5: 9.76 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:09.94 +35:43:18.9: 9.61 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.73 +/- 0.00
Forced photometry filter KEPT candidate at 06:04:25.93 +35:57:08.5: ref_mag=9.73 +/- 0.00 new_mean_mag=8.7912 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 9.59 +/- 0.00
Forced photometry filter REJECTED candidate at 06:00:09.94 +35:43:18.9: ref_mag=9.59 +/- 0.00 new_mean_mag=9.1053 delta=0.48 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:23.52 +33:17:38.6: 10.30 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.32 +/- 0.00
Forced photometry filter REJECTED candidate at 05:56:23.52 +33:17:38.6: ref_mag=10.32 +/- 0.00 new_mean_mag=9.6889 delta=0.63 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:34.92 +35:05:55.6: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:01:34.92 +35:05:55.6: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:56:03.81 +34:11:18.5: 10.93 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:03:19.73 +35:48:27.1: 10.65 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:49:12.38 +33:22:41.3: 10.17 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:01:01.64 +35:49:22.5: 10.03 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:56:03.81 +34:11:18.5: 10.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.95 +/- 0.00
Forced photometry filter KEPT candidate at 05:56:03.81 +34:11:18.5: ref_mag=10.95 +/- 0.00 new_mean_mag=9.6273 delta=1.32 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:03:19.73 +35:48:27.1: 10.73 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.69 +/- 0.00
Forced photometry filter KEPT candidate at 06:03:19.73 +35:48:27.1: ref_mag=10.69 +/- 0.00 new_mean_mag=9.4519 delta=1.24 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:49:12.38 +33:22:41.3: 10.15 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.16 +/- 0.00
Forced photometry filter REJECTED candidate at 05:49:12.38 +33:22:41.3: ref_mag=10.16 +/- 0.00 new_mean_mag=9.6598 delta=0.50 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:01:01.64 +35:49:22.5: 10.07 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.05 +/- 0.00
Forced photometry filter REJECTED candidate at 06:01:01.64 +35:49:22.5: ref_mag=10.05 +/- 0.00 new_mean_mag=9.2549 delta=0.79 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 06:00:46.17 +34:54:33.1: 9.90 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 06:00:46.17 +34:54:33.1: 9.94 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.92 +/- 0.00
Forced photometry filter REJECTED candidate at 06:00:46.17 +34:54:33.1: ref_mag=9.92 +/- 0.00 new_mean_mag=9.3393 delta=0.58 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:32:40.72 +32:56:20.9: 11.19 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:32:40.72 +32:56:20.9: 11.15 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.17 +/- 0.00
Forced photometry filter KEPT candidate at 05:32:40.72 +32:56:20.9: ref_mag=11.17 +/- 0.00 new_mean_mag=10.0537 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:30:34.27 +33:01:09.3: 10.84 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:54:50.33 +33:30:45.8: 9.75 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:30:34.27 +33:01:09.3: 10.80 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.82 +/- 0.00
Forced photometry filter KEPT candidate at 05:30:34.27 +33:01:09.3: ref_mag=10.82 +/- 0.00 new_mean_mag=9.7528 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:54:50.33 +33:30:45.8: 9.78 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.77 +/- 0.00
Forced photometry filter REJECTED candidate at 05:54:50.33 +33:30:45.8: ref_mag=9.77 +/- 0.00 new_mean_mag=9.3271 delta=0.44 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:38:48.48 +35:27:35.0: 10.28 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:38:48.48 +35:27:35.0: 10.23 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.25 +/- 0.00
Forced photometry filter KEPT candidate at 05:38:48.48 +35:27:35.0: ref_mag=10.25 +/- 0.00 new_mean_mag=9.3392 delta=0.91 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out226471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245367.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54756.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 36s
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: 11s
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Considering the candidate 245220_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245220_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:52:40.11 +33:55:03.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245224_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245224_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:52:39.04 +34:16:05.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245226_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245226_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:56:08.94 +35:14:12.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245227_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245227_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:00:28.51 +35:18:43.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245229_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245229_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:52:52.71 +34:26:40.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245233_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245233_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:01:04.97 +35:15:31.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245235_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245235_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:56:01.10 +35:10:07.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245236_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245236_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:00:14.41 +33:08:12.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245237_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245237_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:59:47.59 +36:02:41.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245238_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245238_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:56:31.61 +35:04:44.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245242_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245242_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:57:59.59 +34:01:34.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245243_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245243_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:51:45.28 +33:20:46.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245244_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245244_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:02:18.58 +35:20:05.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245245_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245245_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245246_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245246_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:01:28.77 +35:12:27.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245248_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245248_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:49:06.38 +33:01:09.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245249_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245249_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:03:05.16 +36:31:17.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245252_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245252_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:49:51.02 +32:58:23.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245255_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245255_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:05:44.71 +36:56:01.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245256_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245256_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:52:03.20 +33:42:15.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245258_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245258_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:51:47.01 +33:37:14.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245259_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245259_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:53:39.81 +33:44:12.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245260_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245260_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245261_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245261_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:45:06.70 +33:37:32.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245262_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245262_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245263_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245263_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245265_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245265_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:57:39.66 +33:15:34.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245269_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245269_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:48:14.25 +33:17:24.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245272_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245272_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:03:35.51 +33:52:57.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245274_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245274_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245275_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245275_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:50:25.09 +32:52:49.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245276_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245276_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:07:26.60 +41:51:14.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245277_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245277_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:02:28.80 +36:18:29.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245280_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245280_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245281_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245281_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:52:00.85 +33:33:13.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245282_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245282_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245286_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245286_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245287_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245287_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245288_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245288_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245289_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245289_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:59:24.16 +35:08:06.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245290_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245290_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245294_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245294_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245295_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245295_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:57:23.21 +34:09:11.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245296_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245296_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:57:55.00 +34:54:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.09, MAG_FAINT_SEARCH_LIMIT=10.07)GAIADR2_OUTPUT=# 0.446 3451958193249640576 089.47921054818 +34.91102041126 9.5460 8.4796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245297_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245297_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245298_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245298_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245299_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245299_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:44:53.08 +33:31:43.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245301_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245301_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245303_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245303_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:01:28.10 +36:11:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.10, MAG_FAINT_SEARCH_LIMIT=10.08)GAIADR2_OUTPUT=# 1.635 3456549758103757184 090.36762300997 +36.19560069925 9.3292 8.1259 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245306_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245306_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245307_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245307_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:49:18.97 +34:12:38.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245310_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245310_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:04:28.45 +36:08:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.14, MAG_FAINT_SEARCH_LIMIT=10.12)GAIADR2_OUTPUT=# 1.840 3453628355708157312 091.11876937263 +36.14528240562 9.9387 9.4161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245311_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245311_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245314_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245314_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245315_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245315_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245316_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245316_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245317_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245317_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245318_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245318_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:57:13.67 +32:54:50.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245319_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245319_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245323_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245323_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:56:13.76 +33:52:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.32, MAG_FAINT_SEARCH_LIMIT=10.30)GAIADR2_OUTPUT=# 1.102 3451750561646691328 089.05755698992 +33.87681231018 9.4761 8.2444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245324_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245324_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:56:30.57 +35:08:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.31, MAG_FAINT_SEARCH_LIMIT=10.29)GAIADR2_OUTPUT=# 0.916 3454982198120474752 089.12767126860 +35.14450572638 9.4094 8.1192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245325_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245325_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:04:52.91 +36:53:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.21, MAG_FAINT_SEARCH_LIMIT=10.19)GAIADR2_OUTPUT=# 1.046 3453688244731760512 091.22024437953 +36.89604040449 9.7448 8.8029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245328_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245328_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:02:00.59 +33:16:33.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245329_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245329_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245333_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245333_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245334_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245334_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245335_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 245335_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 245336_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245336_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245338_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245338_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245341_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245341_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245343_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245343_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245344_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245344_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:55:13.40 +34:02:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.38, MAG_FAINT_SEARCH_LIMIT=10.36)GAIADR2_OUTPUT=# 1.127 3451803819240862976 088.80593388935 +34.04817041214 10.1667 8.8497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245345_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245345_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245347_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245347_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245348_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245348_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:59:42.94 +35:21:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.43, MAG_FAINT_SEARCH_LIMIT=10.41)GAIADR2_OUTPUT=# 1.273 3451995576644650496 089.92894426812 +35.36465849490 10.1116 9.0417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245349_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245349_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245351_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245351_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245352_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245352_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245353_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245353_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245355_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245355_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245356_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245356_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245357_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245357_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:04:06.12 +34:41:01.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245358_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245358_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245359_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245359_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245361_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245361_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245364_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245364_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245366_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245366_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245367_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245367_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:56:45.24 +34:34:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.55, MAG_FAINT_SEARCH_LIMIT=10.53)GAIADR2_OUTPUT=# 1.044 3451854220678925824 089.18870031016 +34.58112259986 10.1586 8.9619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245371_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245371_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245373_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245373_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245374_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245374_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:00:18.23 +35:58:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.48, MAG_FAINT_SEARCH_LIMIT=10.46)GAIADR2_OUTPUT=# 0.480 3456520036930176512 090.07605132997 +35.96722110015 10.1919 9.4251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245375_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245375_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:01:51.24 +36:13:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.49, MAG_FAINT_SEARCH_LIMIT=10.47)GAIADR2_OUTPUT=# 2.252 3456550926334839168 090.46349585908 +36.21915227241 10.1113 9.0946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245377_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 245377_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 245379_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245379_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:44:11.67 +33:05:59.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 245380_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245380_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245382_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 245382_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 245383_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245383_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245384_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245384_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245389_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 245389_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 245390_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245390_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:02:42.85 +35:32:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.40, MAG_FAINT_SEARCH_LIMIT=10.38)GAIADR2_OUTPUT=# 2.951 3453449749489784576 090.67848173781 +35.54404035555 10.2520 9.7609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245391_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245391_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:57:23.02 +35:16:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.59, MAG_FAINT_SEARCH_LIMIT=10.57)GAIADR2_OUTPUT=# 0.320 3454978143671243392 089.34602344641 +35.27557238776 10.1546 9.2894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245392_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245392_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:01:07.33 +36:03:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.49, MAG_FAINT_SEARCH_LIMIT=10.47)GAIADR2_OUTPUT=# 1.413 3456524641135058048 090.28070847294 +36.06190920595 10.1850 9.4487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245394_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245394_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:58:16.03 +35:24:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.56, MAG_FAINT_SEARCH_LIMIT=10.54)GAIADR2_OUTPUT=# 1.035 3454977765714029568 089.56682568525 +35.40261958290 10.2540 9.4760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245395_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 245395_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245396_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245396_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245397_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 245397_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245401_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245401_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:57:52.66 +35:13:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.56, MAG_FAINT_SEARCH_LIMIT=10.54)GAIADR2_OUTPUT=# 1.210 3454973917423405440 089.46936778888 +35.22308300426 10.2451 9.4595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245402_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245402_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245403_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245403_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245404_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245404_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245405_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 245405_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245406_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245406_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245409_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245409_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245411_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245411_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:51:52.05 +33:08:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.88, MAG_FAINT_SEARCH_LIMIT=10.86)GAIADR2_OUTPUT=# 1.325 3451284712315164032 087.96708381648 +33.14770379398 10.5139 9.7344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245412_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245412_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:56:03.07 +34:34:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.75, MAG_FAINT_SEARCH_LIMIT=10.73)GAIADR2_OUTPUT=# 0.046 3451856419704480256 089.01279328631 +34.57598718222 10.4250 9.7388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245414_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245414_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:57:17.50 +34:52:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.83, MAG_FAINT_SEARCH_LIMIT=10.81)GAIADR2_OUTPUT=# 0.823 3451867109878703104 089.32267724375 +34.86814445718 10.6622 10.0734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245416_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245416_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245417_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245417_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245420_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245420_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245422_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245422_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245423_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245423_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:55:00.08 +34:30:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.85, MAG_FAINT_SEARCH_LIMIT=10.83)GAIADR2_OUTPUT=# 0.556 3454834004569019136 088.75026626568 +34.50907806305 10.7026 9.9429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245424_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245424_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245427_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245427_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:53:57.54 +34:35:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.82, MAG_FAINT_SEARCH_LIMIT=10.80)GAIADR2_OUTPUT=# 1.826 3454844999685164416 088.48986454071 +34.59800152224 10.5132 9.7709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245428_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245428_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245430_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245430_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245432_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245432_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:03:58.13 +36:36:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.42, MAG_FAINT_SEARCH_LIMIT=10.40)GAIADR2_OUTPUT=# 1.394 3453659206456089344 090.99181384228 +36.60394384958 10.1507 9.3824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245438_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245438_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:56:24.21 +35:00:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.82, MAG_FAINT_SEARCH_LIMIT=10.80)GAIADR2_OUTPUT=# 0.613 3454874823937763584 089.10097062625 +35.01012656709 10.6667 9.9155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245443_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245443_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245445_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245445_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:59:55.37 +34:54:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.79, MAG_FAINT_SEARCH_LIMIT=10.77)GAIADR2_OUTPUT=# 2.656 3451903290683724928 089.98019952220 +34.90244718065 10.6665 10.2188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245448_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245448_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245450_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245450_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245451_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245451_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:59:45.86 +34:51:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.71, MAG_FAINT_SEARCH_LIMIT=10.69)GAIADR2_OUTPUT=# 1.003 3451902775287660928 089.94123665886 +34.85991518403 10.3839 9.6423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245457_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245457_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:51:52.03 +34:09:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.83, MAG_FAINT_SEARCH_LIMIT=10.81)GAIADR2_OUTPUT=# 1.825 3454458899305179264 087.96740438838 +34.15479970659 9.7982 8.4320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245459_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245459_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:03:00.34 +36:34:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.65, MAG_FAINT_SEARCH_LIMIT=10.63)GAIADR2_OUTPUT=# 0.591 3456656750032958208 090.75124489128 +36.57336701456 10.5390 9.7831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245460_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245460_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245461_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245461_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:00:41.03 +35:24:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.71, MAG_FAINT_SEARCH_LIMIT=10.69)GAIADR2_OUTPUT=# 1.196 3451989838566946560 090.17084496336 +35.40431976374 10.5624 10.2019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245462_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245462_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 245463_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 245463_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:48:27.03 +33:23:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.96, MAG_FAINT_SEARCH_LIMIT=10.94)GAIADR2_OUTPUT=# 1.228 3454293590304386944 087.11303212096 +33.38491748133 10.3723 9.3121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 119817_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 119817_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 215460_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 215460_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 223536_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 223536_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 05543_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 05543_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 49544_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 49544_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 237333_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 237333_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 11248_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 11248_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 10963_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 10963_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 232881_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 232881_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 26461_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 26461_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 230622_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 230622_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 228522_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 228522_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 06:03:22.66 +36:25:03.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 226471_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 226471_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:50:37.56 +33:48:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.25, MAG_FAINT_SEARCH_LIMIT=10.23)GAIADR2_OUTPUT=# 1.465 3454420824418247168 087.65663685203 +33.80747049202 8.8572 7.4739 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 226224_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 226224_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 224801_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 224801_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:48:58.30 +33:16:12.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 05430_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 05430_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 221050_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 221050_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 220667_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 220667_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 219399_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 219399_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 34382_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 34382_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 218310_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 218310_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 218073_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 218073_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 05499_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 05499_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:57:25.23 +33:08:00.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 217393_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 217393_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 52949_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 52949_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 43115_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 43115_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 54756_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 54756_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 50407_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 50407_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 08197_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 08197_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 40254_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 40254_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 24401_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 24401_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 51928_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 51928_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 09609_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 09609_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 52315_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 52315_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 37028_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 37028_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 03828_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 03828_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 159150_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 159150_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
Rejecting candidate due to large distance (44.8") between the two second-epoch detections
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Considering the candidate 05824_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 05824_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 12009_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 12009_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
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Considering the candidate 47827_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
Preparing report for the candidate 47827_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
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Considering the candidate 35080_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 35080_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:27:38.86 +34:28:32.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 26464_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 26464_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:20:00.95 +33:57:29.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 22925_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 22925_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:19:00.05 +33:44:53.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 17489_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 17489_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:18:10.73 +33:22:14.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 186160_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 186160_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:06:30.97 +41:14:02.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 114368_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 114368_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:51:29.36 +39:08:54.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 19751_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 19751_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:56:59.88 +33:09:59.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 85136_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 85136_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:52:38.03 +36:42:11.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101713_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 101713_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 04:59:15.54 +37:53:22.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 152323_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 152323_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
**** FOUND 05:02:28.77 +41:04:32.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 101136_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355
The candidate 101136_fd_Aur-03-Q1b1x1_2026-08-06_03-48-43_20.00sec_-0.00C_LIGHTs_0355 did not pass the final checks
