This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 10.54 05:47:00.50 +40:10:49.0
170.50586 6.05881 galactic Aur Second-epoch detections are separated by 2.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J086.7611+40.1933 | 05:47:02.94 +40:11:00.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 1947AnDea...5....1L DO 11548
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:47:00.50 +40:10:49.0: 12.17 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:47:00.50 +40:10:49.0: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.7611+40.1933,2461152.6182,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.7611+40.1933 20260422.1182 10.54CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J082.2006+35.7751,2461152.6182,10.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.2006+35.7751 20260422.1182 10.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 12.73 05:18:14.53 +40:21:39.6
167.36688 1.55102 galactic Aur Second-epoch detections are separated by 5.9" and 5.6 pix
The object was found in VSX18" Gaia DR3 188836861467316864
Type: RS
# Max. Min./Amp. JD0 Period
14.860 G 14.920 G 1.655140000000 G
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:18:14.53 +40:21:39.6: 13.50 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:18:14.53 +40:21:39.6: 13.53 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 188836861467316864,2461152.6182,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 188836861467316864 20260422.1182 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 12.48 05:47:05.27 +40:56:38.7
169.85262 6.46127 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 | ATO J086.7744+40.9372 | 05:47:06.44 +40:56:57.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:47:05.27 +40:56:38.7: 14.96 +/- 0.12 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:47:05.27 +40:56:38.7: 14.75 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.84 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.7744+40.9372,2461152.6182,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.7744+40.9372 20260422.1182 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 12.61 05:38:19.93 +42:16:25.7
167.85580 5.75127 galactic Aur Second-epoch detections are separated by 5.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J084.5910+42.2678 | 05:38:21.23 +42:16:46.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:38:19.93 +42:16:25.7: 14.67 +/- 0.11 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:38:19.93 +42:16:25.7: 14.84 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.08
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.5910+42.2678,2461152.6182,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.5910+42.2678 20260422.1182 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 12.63 05:24:09.32 +34:46:44.2
172.62246 -0.66555 galactic Aur Second-epoch detections are separated by 5.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J081.0335+34.7749 | 05:24:08.04 +34:46:29.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:24:09.32 +34:46:44.2: 13.33 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:24:09.32 +34:46:44.2: 14.18 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.0335+34.7749,2461152.6182,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.0335+34.7749 20260422.1182 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 12.11 05:30:29.53 +38:07:44.3
170.54764 2.25711 galactic Aur Second-epoch detections are separated by 8.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 190380477006723712 | 05:30:30.49 +38:07:52.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:30:29.53 +38:07:44.3: 12.99 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:30:29.53 +38:07:44.3: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 190380477006723712,2461152.6182,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 190380477006723712 20260422.1182 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 11.94 05:59:51.48 +41:47:36.1
170.30141 8.96385 galactic Aur Second-epoch detections are separated by 4.6" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 192153439507622144 | 05:59:52.60 +41:47:40.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:59:51.48 +41:47:36.1: 12.87 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:59:51.48 +41:47:36.1: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192153439507622144,2461152.6182,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192153439507622144 20260422.1182 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 12.18 05:25:44.63 +41:56:03.0
166.87051 3.60598 galactic Aur Second-epoch detections are separated by 8.3" 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 | ATO J081.4404+41.9393 | 05:25:44.83 +41:56:22.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:25:44.63 +41:56:03.0: 13.17 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:25:44.63 +41:56:03.0: 13.10 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.4404+41.9393,2461152.6182,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.4404+41.9393 20260422.1182 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 12.15 05:25:43.50 +41:03:07.1
167.60194 3.11088 galactic Aur Second-epoch detections are separated by 2.7" 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 J081.4134+41.0499 | 05:25:42.01 +41:03:06.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:25:43.50 +41:03:07.1: 13.50 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:25:43.50 +41:03:07.1: 13.48 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.49 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.4134+41.0499,2461152.6182,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.4134+41.0499 20260422.1182 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 11.86 05:57:35.26 +41:36:49.0
170.25463 8.50588 galactic Aur Second-epoch detections are separated by 2.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 192136186620601856 | 05:57:37.17 +41:36:55.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:57:35.26 +41:36:49.0: 13.67 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:57:35.26 +41:36:49.0: 13.87 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192136186620601856,2461152.6182,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192136186620601856 20260422.1182 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 11.91 05:59:13.06 +41:57:06.9
170.10272 8.93511 galactic Aur Second-epoch detections are separated by 0.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.8034+41.9534 | 05:59:14.16 +41:57:14.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:59:13.06 +41:57:06.9: 13.10 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:59:13.06 +41:57:06.9: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.8034+41.9534,2461152.6182,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.8034+41.9534 20260422.1182 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 11.74 06:02:51.88 +41:05:46.4
171.19369 9.12812 galactic Aur Second-epoch detections are separated by 2.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J090.7112+41.0964 | 06:02:53.25 +41:05:49.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 06:02:51.88 +41:05:46.4: 12.75 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 06:02:51.88 +41:05:46.4: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.7112+41.0964,2461152.6182,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.7112+41.0964 20260422.1182 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 11.51 05:52:17.11 +34:45:03.7
175.73494 4.20170 galactic Aur Second-epoch detections are separated by 2.5" and 6.3 pix
The object was found in VSX16" NSVS 6998598
Type: SR
# Max. Min./Amp. JD0 Period
13.415 g Y 0.731 g 2458291.47310 359.618147900000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:52:17.11 +34:45:03.7: 12.40 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:52:17.11 +34:45:03.7: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 6998598,2461152.6182,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 6998598 20260422.1182 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 11.46 05:56:27.27 +40:13:14.2
171.37869 7.64118 galactic Aur Second-epoch detections are separated by 3.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3458564372642520576 | 05:56:28.68 +40:13:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 1947AnDea...5....1L DO 11713
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:56:27.27 +40:13:14.2: 12.90 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:56:27.27 +40:13:14.2: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3458564372642520576,2461152.6182,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3458564372642520576 20260422.1182 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 11.38 05:58:34.10 +41:28:43.3
170.46370 8.60142 galactic Aur Second-epoch detections are separated by 6.6" and 5.1 pix
The object was found in VSX12" Gaia DR3 192142341312248576
Type: DSCT|GDOR
# Max. Min./Amp. JD0 Period
12.960 G 12.990 G A
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:58:34.10 +41:28:43.3: 12.76 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:58:34.10 +41:28:43.3: 12.72 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192142341312248576,2461152.6182,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192142341312248576 20260422.1182 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 11.71 05:56:39.34 +38:24:36.4
172.98838 6.78723 galactic Aur Second-epoch detections are separated by 6.9" 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 | Gaia DR3 3457804541387882496 | 05:56:42.59 +38:24:39.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:56:39.34 +38:24:36.4: 14.77 +/- 0.11 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:56:39.34 +38:24:36.4: 14.78 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3457804541387882496,2461152.6182,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3457804541387882496 20260422.1182 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 11.93 05:58:37.21 +35:27:09.4
175.77309 5.67465 galactic Aur Second-epoch detections are separated by 4.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.6673+35.4463 | 05:58:38.01 +35:26:49.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:58:37.21 +35:27:09.4: 14.32 +/- 0.07 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:58:37.21 +35:27:09.4: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.07 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.6673+35.4463,2461152.6182,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.6673+35.4463 20260422.1182 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.1182 2461152.6182 11.94 05:53:33.77 +35:52:27.6
174.89303 4.99260 galactic Aur Second-epoch detections are separated by 6.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3455169871010622976 | 05:53:32.90 +35:51:53.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:53:33.77 +35:52:27.6: 15.33 +/- 0.18 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:53:33.77 +35:52:27.6: 15.27 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.30 +/- 0.12
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3455169871010622976,2461152.6182,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3455169871010622976 20260422.1182 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J084.3742+41.0080,2461152.6182,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3742+41.0080 20260422.1182 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3449541947727446656,2461152.6182,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3449541947727446656 20260422.1182 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3458183456285001728,2461152.6182,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3458183456285001728 20260422.1182 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.1364+38.1181,2461152.6182,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.1364+38.1181 20260422.1182 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3449360670045396864,2461152.6182,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3449360670045396864 20260422.1182 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3454433198220980096,2461152.6182,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3454433198220980096 20260422.1182 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 184230938537964672,2461152.6182,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 184230938537964672 20260422.1182 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 191894740741083264,2461152.6182,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 191894740741083264 20260422.1182 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461152.6182,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260422.1182 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 191060971626352000,2461152.6182,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 191060971626352000 20260422.1182 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 182708050507066624,2461152.6182,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 182708050507066624 20260422.1182 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J085.9044+41.7647,2461152.6182,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.9044+41.7647 20260422.1182 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BH Aur,2461152.6182,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BH Aur 20260422.1182 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3458201838746776576,2461152.6182,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3458201838746776576 20260422.1182 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194807587560369024,2461152.6182,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194807587560369024 20260422.1182 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 191542141104156160,2461152.6182,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 191542141104156160 20260422.1182 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194316483820829440,2461152.6182,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194316483820829440 20260422.1182 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 184384908821614208,2461152.6182,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 184384908821614208 20260422.1182 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 182865826129990272,2461152.6182,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 182865826129990272 20260422.1182 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3458367628781128704,2461152.6182,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3458367628781128704 20260422.1182 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 189560344412811008,2461152.6182,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 189560344412811008 20260422.1182 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461083.61922233 12.02.2026 02:51:30.809 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
First image: 2461083.61922233 12.02.2026 02:51:30.809 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Last image: 2461152.61849161 22.04.2026 02:50:27.675 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 25
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
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: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 22441
Objects passed selection criteria: 22286
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 15538
Average stars matched: 15045 (96.8271 %)
Memory usage VmPeak: 128372 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 21 21:57:33 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461083.61922233 12.02.2026 02:51:30.809 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
First image: 2461083.61922233 12.02.2026 02:51:30.809 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Last image: 2461152.61849161 22.04.2026 02:50:27.675 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 300
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 50 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 175506
Objects passed selection criteria: 174923
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 116529
Average stars matched: 111542 (95.7208 %)
Memory usage VmPeak: 2010072 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 21 22:04:50 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_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-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461152.61784931
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
Saving wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits to local_wcs_cache/
'wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits' -> 'local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits'
wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits exists and is non-empty
Saving wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits to local_wcs_cache/
'wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits'
wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits'
wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits (1st reference image)
verification OK: wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Image size: 943.3'x627.4' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:33.978 +37:59:21.26 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/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-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
Image size: 938.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:27:28.425 +38:01:31.18 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:33.978 +37:59:21.26
Second-epoch image center 05:27:28.425 +38:01:31.18
Angular distance between the image centers 0.0404 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
Image size: 938.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:27:30.665 +38:01:03.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:33.978 +37:59:21.26
Second-epoch image center 05:27:30.665 +38:01:03.77
Angular distance between the image centers 0.0305 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 05:27:28.425 +38:01:31.18
Second-epoch second image center 05:27:30.665 +38:01:03.77
Angular distance between the image centers 0.01059 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.jxoHQJXPfc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits &> /tmp/tmp.rJbkU45mbI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits &> /tmp/tmp.XV1QQDztmx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits &> /tmp/tmp.fhHVL5Hpso
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
Found non-empty wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
The reference image (wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits) and catalog (wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat) found
'wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat' -> 'wcsmag.cat'
Read 30329 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3560 to 92.7536 deg, Dec +32.1688 to +43.3136 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 71.3560 to 92.7536 deg, Dec 32.1688 to 43.3136 deg
Loaded 16011 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): 5748 out of 6465 total matches.
Matched with Tycho-2 6465 out of 30329 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.940226
a=0.000000 b=1.000000 c=22.940226
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 30329 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3560 to 92.7536 deg, Dec +32.1688 to +43.3136 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 71.3560 to 92.7536 deg, Dec 32.1688 to 43.3136 deg
Loaded 16011 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): 5748 out of 6465 total matches.
Matched with Tycho-2 6465 out of 30329 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits (aperture=5.8)
Read 30261 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.4177 to 92.7541 deg, Dec +32.1709 to +43.3193 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 71.4177 to 92.7541 deg, Dec 32.1709 to 43.3193 deg
Loaded 16007 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): 10343 out of 11765 total matches.
Matched with Tycho-2 11765 out of 30261 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 18 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
2.1 pix Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
4.5 pix fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
4.5 pix fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
2.1 pix wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
2.1 pix wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Limiting magnitude estimates:
15.4 mag. Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
15.4 mag. Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
13.5 mag. fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
13.5 mag. fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 11.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jxoHQJXPfc (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3460, passed=30329
Got 30329 stars (including 26832 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 30329 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.3'
Seting catalog search parameters based on the expected field of view 943.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013101 (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 0.010481 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 896 matched stars entering correct_measured_positions(), 863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.84"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 896 matched stars entering correct_measured_positions(), 26894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.17"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 26910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.14"
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 27622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.18"
Excluding outliers - 912 stars left (next iteration limit 985)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rJbkU45mbI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_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-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_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-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_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-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3436, passed=30261
Got 30261 stars (including 26784 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 30261 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 28158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 28159 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 28158 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits -region wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.XV1QQDztmx (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=750, passed=9161
Got 9161 stars (including 8407 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat
util/solve_plate_with_UCAC5 got 9161 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 8629 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.01"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 8630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.01"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 8631 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 943 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits -region wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fhHVL5Hpso (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=780, passed=9128
Got 9128 stars (including 8346 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 9128 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 8666 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 8665 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 8667 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Excluding outliers - 943 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits -region wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits'
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits'
Preparing the HTML report for the field Aur-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out21583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51884.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51800_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 51800_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 06:01:58.90 +39:54:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.78, MAG_FAINT_SEARCH_LIMIT=11.76)GAIADR2_OUTPUT=# 4.390 3458367628780409728 090.49393352540 +39.91581068723 10.3093 9.5850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51830_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 51830_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:26:54.69 +36:54:13.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51884_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 51884_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12093_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 12093_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:51:28.36 +39:08:52.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16925_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 16925_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:51:01.75 +37:18:20.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21583_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 21583_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10199_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 10199_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 06:01:06.76 +39:40:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17570_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 17570_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:24:39.18 +37:23:09.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 22263_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 22263_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:26:54.27 +35:27:30.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 09825_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 09825_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:36:52.11 +40:10:53.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10370_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 10370_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:19:09.86 +40:05:35.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14920_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 14920_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:13:26.09 +38:29:01.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24585_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 24585_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:27:38.80 +34:28:40.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12169_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 12169_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:49:09.51 +39:10:49.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26763_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 26763_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:20:01.06 +33:57:34.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25148_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 25148_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:52:39.60 +33:55:08.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06231_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 06231_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:06:31.42 +41:13:56.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16581_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 16581_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:59:42.93 +37:12:43.5 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 14s
Prepared the HTML report for the field Aur-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:28:49.77 +35:47:17.2
05:47:00.50 +40:10:49.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_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-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Creating symlink local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits exists and is non-empty
wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits exists and is non-empty
wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits (1st reference image)
verification OK: wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Image size: 943.3'x627.4' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:33.978 +37:59:21.26 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/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-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
Image size: 938.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:27:28.425 +38:01:31.18 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:33.978 +37:59:21.26
Second-epoch image center 05:27:28.425 +38:01:31.18
Angular distance between the image centers 0.0404 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
Image size: 938.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:27:30.665 +38:01:03.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:33.978 +37:59:21.26
Second-epoch image center 05:27:30.665 +38:01:03.77
Angular distance between the image centers 0.0305 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 05:27:28.425 +38:01:31.18
Second-epoch second image center 05:27:30.665 +38:01:03.77
Angular distance between the image centers 0.01059 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.gujIXZkgs9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits &> /tmp/tmp.3wKrZRkUgt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits &> /tmp/tmp.dkCmpKQctl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits &> /tmp/tmp.Itbg35QHI5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
Found non-empty wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
The reference image (wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits) and catalog (wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat) found
'wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat' -> 'wcsmag.cat'
Read 230190 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3492 to 92.7576 deg, Dec +32.1361 to +43.3174 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 71.3492 to 92.7576 deg, Dec 32.1361 to 43.3174 deg
Loaded 16068 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): 4267 out of 6645 total matches.
Matched with Tycho-2 6645 out of 230190 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.800367
a=0.000000 b=1.000000 c=22.800367
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 230190 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3492 to 92.7576 deg, Dec +32.1361 to +43.3174 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 71.3492 to 92.7576 deg, Dec 32.1361 to 43.3174 deg
Loaded 16068 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): 4267 out of 6645 total matches.
Matched with Tycho-2 6645 out of 230190 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits (aperture=4.4)
Read 230022 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3956 to 92.7710 deg, Dec +32.1459 to +43.3193 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 71.3956 to 92.7710 deg, Dec 32.1459 to 43.3193 deg
Loaded 16054 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): 7582 out of 11992 total matches.
Matched with Tycho-2 11992 out of 230022 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 200 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
1.9 pix Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
3.0 pix fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
3.0 pix fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
1.9 pix wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
1.9 pix wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Limiting magnitude estimates:
15.6 mag. Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
15.5 mag. Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
13.7 mag. fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
13.7 mag. fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.0 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gujIXZkgs9 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=35441, passed=230149
Got 230149 stars (including 194360 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 230149 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.3'
Seting catalog search parameters based on the expected field of view 943.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013101 (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 0.010481 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.04"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 215460 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.04"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 215468 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.03"
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 218781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.02"
Excluding outliers - 919 stars left (next iteration limit 990)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3wKrZRkUgt (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_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-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_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-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_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-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=62, blended=35436, passed=229960
Got 229960 stars (including 194138 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 229960 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 221502 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 221500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 221503 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits -region wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dkCmpKQctl (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=149, blended=8440, passed=60236
Got 60236 stars (including 51729 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat
util/solve_plate_with_UCAC5 got 60236 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 59146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 59145 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 59144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits -region wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Itbg35QHI5 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=140, blended=8498, passed=60354
Got 60354 stars (including 51777 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 60354 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 59277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.01"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 59277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.01"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 59278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits -region wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-49-32_20.00sec_-5.00C_LIGHT_0037.fits
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-21_CI_Aur-03-Q2b1x1_215137_TTUQ2b1x1_1529126_dCyVTTUT/wcs_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038.fits
Preparing the HTML report for the field Aur-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out257891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out257999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out258130.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out258283.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out100225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out182446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out223643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out224540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out258774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74349.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 159s
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: 29s
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Considering the candidate 257891_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257891_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:13:59.08 +38:24:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 4.937 188203409625747840 078.49511046042 +38.40987132558 13.5170 13.1248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257895_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257895_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:11:28.24 +42:03:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.654 201217366692713728 077.86819245675 +42.05397999273 13.1574 12.6455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257899_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257899_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:23:51.09 +38:49:30.4: 13.16 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:23:51.09 +38:49:30.4: 12.95 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
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Considering the candidate 257906_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257906_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:12:13.27 +34:19:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.991 182221516613780736 078.05512240264 +34.32927051440 13.4159 12.7274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 257911_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257911_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:08:49.41 +41:07:36.0: 14.64 +/- 0.11 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:08:49.41 +41:07:36.0: 13.51 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
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Considering the candidate 257917_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257917_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:39:17.91 +39:48:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.018 191003212906017408 084.82283253420 +39.81135643093 12.8981 12.4999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.018#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257920_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257920_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:13:22.11 +40:23:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 257921_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257921_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:07:43.55 +40:45:37.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)
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Considering the candidate 257928_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257928_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:26:27.36 +38:43:10.0: 13.04 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:26:27.36 +38:43:10.0: 13.21 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.01
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Considering the candidate 257930_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257930_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:22:37.38 +38:36:05.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:22:37.38 +38:36:05.0: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.01
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Considering the candidate 257936_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257936_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:22:37.56 +38:35:47.6: 12.61 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:22:37.56 +38:35:47.6: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
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Considering the candidate 257937_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257937_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:49:00.81 +36:16:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.626 3455980275503174528 087.25212921266 +36.27684016429 12.8801 12.3349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257939_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257939_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:38:14.37 +40:07:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 5.779 191069625981614208 084.55856431616 +40.12207934990 12.7229 12.1998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257941_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257941_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:08:26.87 +34:10:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.010 184833883223833216 077.11193029761 +34.16944269606 13.2291 12.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257949_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257949_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:52:42.82 +36:09:36.5: 12.83 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:52:42.82 +36:09:36.5: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
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Considering the candidate 257950_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257950_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 257958_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257958_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:22:59.47 +39:02:39.2: 12.84 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:22:59.47 +39:02:39.2: 12.64 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
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Considering the candidate 257977_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257977_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:32:30.03 +39:44:47.3: 12.67 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:32:30.03 +39:44:47.3: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
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Considering the candidate 257980_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257980_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:31:02.37 +36:52:23.8: 12.67 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:31:02.37 +36:52:23.8: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
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Considering the candidate 257982_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257982_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:28:47.33 +38:31:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 4.087 190591132266678016 082.19815844286 +38.52905269402 12.2143 11.7801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 257991_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257991_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:44:52.71 +41:57:42.3: 13.37 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:44:52.71 +41:57:42.3: 13.25 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
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Considering the candidate 257999_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 257999_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:28:06.17 +39:14:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.608 193692996305312128 082.02627815341 +39.24850718555 12.4008 11.9884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258000_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258000_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:26:49.95 +38:36:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.515 190648070650303360 081.70700879736 +38.61418893750 12.7848 12.3624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258001_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258001_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:17:02.18 +41:07:13.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 258002_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258002_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:26:33.92 +38:13:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 5.572 184625667507500032 081.64211893420 +38.22871953875 12.2878 11.4703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258004_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258004_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:12:55.46 +40:35:29.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 258009_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258009_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:25:07.98 +37:23:23.2: 12.86 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:25:07.98 +37:23:23.2: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.01
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Considering the candidate 258010_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258010_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:28:00.65 +38:44:57.5: 12.61 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:28:00.65 +38:44:57.5: 12.65 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
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Considering the candidate 258013_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258013_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:27:51.72 +38:40:23.8: 12.86 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:27:51.72 +38:40:23.8: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.01
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Considering the candidate 258014_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258014_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:24:17.82 +38:44:39.6: 12.93 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:24:17.82 +38:44:39.6: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
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Considering the candidate 258017_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258017_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258022_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258022_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:07:26.05 +41:46:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258024_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258024_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:32:12.84 +39:07:22.4: 12.43 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:32:12.84 +39:07:22.4: 12.63 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
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Considering the candidate 258026_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258026_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:53:48.40 +35:10:12.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)
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Considering the candidate 258029_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258029_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:04:48.32 +41:47:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258032_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258032_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:30:31.15 +40:16:40.0: 12.68 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:30:31.15 +40:16:40.0: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
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Considering the candidate 258041_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258041_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:25:28.13 +40:35:21.5: 12.76 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:25:28.13 +40:35:21.5: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
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Considering the candidate 258049_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258049_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:10:11.88 +40:03:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 4.782 188946061011548160 077.54872184005 +40.05224295435 13.3188 12.5774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258050_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258050_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:28:54.80 +36:46:29.6: 12.80 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:28:54.80 +36:46:29.6: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
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Considering the candidate 258054_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258054_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:19:39.45 +37:30:30.2: 13.35 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:19:39.45 +37:30:30.2: 13.20 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
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Considering the candidate 258063_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258063_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:21:41.89 +38:20:55.9: 12.57 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:21:41.89 +38:20:55.9: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
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Considering the candidate 258064_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258064_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:23:42.24 +38:22:01.1: 12.38 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:23:42.24 +38:22:01.1: 12.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
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Considering the candidate 258066_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258066_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:24:53.31 +39:47:34.8: 12.65 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:24:53.31 +39:47:34.8: 13.04 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
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Considering the candidate 258068_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258068_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:30:25.87 +40:55:57.8: 12.82 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:30:25.87 +40:55:57.8: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
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Considering the candidate 258070_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258070_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:33:17.32 +38:21:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 5.192 190488607104413440 083.32346237700 +38.35542101951 12.2441 11.9578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258073_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258073_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:26:56.87 +38:24:18.0: 12.61 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:26:56.87 +38:24:18.0: 12.85 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
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Considering the candidate 258081_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258081_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258088_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258088_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:14:21.27 +40:11:32.8: 13.10 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:14:21.27 +40:11:32.8: 12.98 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
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Considering the candidate 258094_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258094_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:22:25.10 +37:05:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.489 184449672630737664 080.60460621435 +37.08832999489 12.5017 12.0422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258097_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258097_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:25:02.17 +38:48:40.3: 13.33 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:25:02.17 +38:48:40.3: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.01
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Considering the candidate 258103_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258103_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:42:50.87 +35:49:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258106_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258106_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:23:08.86 +39:25:37.7: 12.41 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:23:08.86 +39:25:37.7: 12.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
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Considering the candidate 258109_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258109_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:26:49.49 +38:48:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.801 190654663422351232 081.70701245237 +38.80646134712 11.9387 11.1284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258111_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258111_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258112_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258112_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:15:07.90 +36:33:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 5.888 187006758720756224 078.78099446735 +36.55503965455 11.6887 10.4946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258117_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258117_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:35:09.78 +40:32:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 4.571 191237271444113664 083.79240866224 +40.53343086522 12.4597 12.1774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258121_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258121_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:53:52.60 +35:46:36.6: 12.87 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:53:52.60 +35:46:36.6: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.01
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Considering the candidate 258122_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258122_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:22:26.04 +38:29:48.8: 12.62 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:22:26.04 +38:29:48.8: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
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Considering the candidate 258130_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258130_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:23:14.93 +38:36:17.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 258139_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258139_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258154_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258154_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:25:20.39 +39:08:39.2: 12.50 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:25:20.39 +39:08:39.2: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
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Considering the candidate 258158_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258158_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:34:27.21 +38:34:09.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)
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Considering the candidate 258163_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258163_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:30:50.03 +34:12:13.4: 12.83 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:30:50.03 +34:12:13.4: 12.67 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.01
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Considering the candidate 258169_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258169_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:25:08.68 +39:12:47.5: 12.38 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:25:08.68 +39:12:47.5: 12.76 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
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Considering the candidate 258171_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258171_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:35:47.74 +34:12:01.4: 12.57 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:35:47.74 +34:12:01.4: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
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Considering the candidate 258182_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258182_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 258186_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258186_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:20:27.16 +36:53:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.836 184077350506006400 080.11221199978 +36.89563899356 12.6151 12.2843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258187_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258187_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:25:46.71 +37:54:22.9: 12.16 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:25:46.71 +37:54:22.9: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
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Considering the candidate 258190_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258190_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 258193_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258193_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:26:41.22 +38:11:51.6: 12.50 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:26:41.22 +38:11:51.6: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.42 +/- 0.01
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Considering the candidate 258196_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258196_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:24:29.24 +39:01:51.7: 12.21 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:24:29.24 +39:01:51.7: 12.33 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
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Considering the candidate 258197_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258197_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:39:45.62 +33:55:43.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)
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Considering the candidate 258198_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258198_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:31:34.21 +37:53:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 4.791 190358692932790656 082.89342684571 +37.88657732547 10.2398 8.8429 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258200_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258200_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:24:57.74 +38:27:11.6: 12.34 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:24:57.74 +38:27:11.6: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.34 +/- 0.01
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Considering the candidate 258202_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258202_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:47:39.22 +34:13:25.2: 12.19 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:47:39.22 +34:13:25.2: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
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Considering the candidate 258205_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258205_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:06:05.26 +41:39:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258226_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258226_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 258229_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258229_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:24:00.85 +38:47:47.7: 11.96 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:24:00.85 +38:47:47.7: 12.30 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.09 +/- 0.01
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Considering the candidate 258237_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258237_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258240_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258240_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:24:26.22 +37:45:30.2: 12.24 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:24:26.22 +37:45:30.2: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.13 +/- 0.01
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Considering the candidate 258248_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258248_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:10:27.16 +36:04:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258249_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258249_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:56:47.84 +42:00:12.7: 12.70 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:56:47.84 +42:00:12.7: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
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Considering the candidate 258258_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258258_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:25:33.80 +38:22:13.1: 12.41 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:25:33.80 +38:22:13.1: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.01
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Considering the candidate 258262_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258262_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:54:03.60 +37:23:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 4.314 3457644871684530944 088.51645533746 +37.39471257231 11.8061 10.8375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258272_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258272_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:25:15.14 +38:18:50.7: 12.30 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:25:15.14 +38:18:50.7: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.22 +/- 0.01
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Considering the candidate 258278_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258278_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:24:41.26 +38:18:23.3: 12.02 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:24:41.26 +38:18:23.3: 12.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
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Considering the candidate 258280_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258280_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:22:21.09 +38:54:05.4: 12.13 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:22:21.09 +38:54:05.4: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
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Considering the candidate 258281_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258281_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258283_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258283_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:26:59.62 +38:59:43.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)
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Considering the candidate 258285_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258285_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258286_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258286_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:23:50.55 +38:38:51.7: 12.08 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:23:50.55 +38:38:51.7: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.12 +/- 0.01
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Considering the candidate 258287_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258287_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:49:17.33 +41:47:24.4: 13.00 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:49:17.33 +41:47:24.4: 12.82 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
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Considering the candidate 258292_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258292_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:52:55.82 +40:16:44.7: 12.61 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:52:55.82 +40:16:44.7: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.01
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Considering the candidate 258299_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258299_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 258300_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258300_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:12:25.15 +38:07:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258302_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258302_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:14:58.44 +35:05:28.1: 13.11 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:14:58.44 +35:05:28.1: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
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Considering the candidate 258304_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258304_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258308_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258308_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:10:09.16 +36:56:18.7: 12.58 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:10:09.16 +36:56:18.7: 12.59 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
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Considering the candidate 258312_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258312_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:43:00.88 +40:00:46.9: 12.91 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:43:00.88 +40:00:46.9: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
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Considering the candidate 258315_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258315_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258320_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258320_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:56:04.70 +34:06:14.3: 13.85 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:56:04.70 +34:06:14.3: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.23 +/- 0.01
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Considering the candidate 258328_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258328_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:25:54.24 +37:05:57.9: 12.41 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:25:54.24 +37:05:57.9: 12.37 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.39 +/- 0.01
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Considering the candidate 258332_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258332_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:52:01.46 +42:11:46.4: 12.57 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:52:01.46 +42:11:46.4: 12.55 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
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Considering the candidate 258333_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258333_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258336_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258336_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:56:38.49 +40:34:36.3: 12.22 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:56:38.49 +40:34:36.3: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
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Considering the candidate 258339_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258339_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:18:35.21 +38:05:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 4.863 187558992732467328 079.64516301950 +38.08411559662 11.5158 11.3753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258345_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258345_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258352_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258352_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:24:14.16 +38:12:17.5: 11.90 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:24:14.16 +38:12:17.5: 11.75 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.00
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Considering the candidate 258356_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258356_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:13:13.81 +34:11:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 3.524 182169697830963200 078.30831619648 +34.19754571078 11.6762 10.8958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258358_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258358_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:44:20.68 +36:32:52.2: 12.22 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:44:20.68 +36:32:52.2: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.01
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Considering the candidate 258363_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258363_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258366_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258366_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:24:46.74 +38:24:05.0: 11.98 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:24:46.74 +38:24:05.0: 11.62 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.75 +/- 0.00
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Considering the candidate 258367_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258367_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:23:52.05 +38:44:54.3: 11.92 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:23:52.05 +38:44:54.3: 11.57 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.69 +/- 0.00
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Considering the candidate 258370_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258370_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258371_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258371_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 258374_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258374_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258375_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258375_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 258378_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258378_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:24:15.54 +38:26:16.3: 10.21 +/- 0.00 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:24:15.54 +38:26:16.3: 10.40 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.30 +/- 0.00
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Considering the candidate 258691_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258691_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258747_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258747_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258752_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258752_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:06:25.42 +34:49:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258765_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258765_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:06:43.44 +41:15:42.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 258774_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 258774_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 258995_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 258995_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 259077_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 259077_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:14:45.37 +39:31:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259200_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 259200_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:06:20.14 +41:15:43.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 162109_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 162109_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:23:51.28 +36:23:54.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 242255_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 242255_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:32:22.82 +39:38:04.1: 13.42 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:32:22.82 +39:38:04.1: 13.34 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.37 +/- 0.02
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Considering the candidate 49412_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 49412_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:19:23.30 +41:14:51.6: 13.09 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:19:23.30 +41:14:51.6: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
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Considering the candidate 52915_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 52915_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 184495_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 184495_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 72476_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 72476_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 113533_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 113533_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 226738_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 226738_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 185012_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 185012_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 155302_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 155302_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 150552_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 150552_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:26:54.64 +36:54:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40971_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 40971_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 182446_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 182446_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 74349_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 74349_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 57186_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 57186_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:54:38.98 +40:33:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224540_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 224540_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 31605_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 31605_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 50779_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 50779_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:19:31.10 +41:12:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223643_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 223643_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 100225_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 100225_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 63212_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 63212_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 225631_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 225631_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:07:03.52 +34:02:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71851_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 71851_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 50648_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 50648_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 154218_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 154218_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 45963_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 45963_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:18:01.36 +41:23:16.5: 13.06 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:18:01.36 +41:23:16.5: 13.03 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.05 +/- 0.02
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Considering the candidate 193869_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 193869_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 85410_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 85410_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:37:26.41 +39:43:07.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)
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Considering the candidate 169453_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 169453_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits at 05:27:54.98 +35:51:37.1: 13.85 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits at 05:27:54.98 +35:51:37.1: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.01
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Considering the candidate 69555_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 69555_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 136791_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
Preparing report for the candidate 136791_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
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Considering the candidate 122520_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 122520_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:31:26.67 +38:19:08.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141622_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 141622_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:20:43.20 +37:26:20.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144361_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 144361_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:24:39.22 +37:23:09.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180042_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 180042_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:29:42.65 +35:22:31.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86808_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 86808_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:30:45.06 +39:49:29.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166651_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 166651_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:24:44.82 +36:12:03.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143614_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 143614_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:13:17.38 +37:20:11.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191506_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 191506_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:25:12.89 +34:51:23.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77226_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 77226_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:36:52.14 +40:10:53.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188647_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 188647_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:28:26.46 +34:41:54.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179923_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 179923_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:26:54.28 +35:27:31.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82851_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 82851_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:19:09.92 +40:05:34.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53946_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 53946_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:34:16.73 +41:07:20.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121199_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 121199_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:13:26.11 +38:29:01.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190904_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 190904_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:33:38.11 +34:43:34.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 229126_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 229126_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:25:30.02 +34:11:13.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47067_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 47067_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:39:08.35 +41:21:24.2 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58043_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 58043_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:18:55.48 +41:05:40.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73472_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 73472_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:18:40.56 +40:27:50.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57298_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 57298_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:22:50.38 +41:01:39.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26081_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 26081_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:29:01.13 +42:16:08.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46875_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 46875_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:30:49.02 +41:27:36.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56391_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 56391_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:20:14.77 +41:05:04.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184240_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 184240_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:27:38.87 +34:28:39.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183527_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 183527_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:26:48.81 +34:23:34.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146575_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 146575_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:10:19.21 +37:18:08.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220898_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 220898_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:28:00.98 +33:45:46.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29452_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 29452_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:33:28.65 +42:06:28.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 225002_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 225002_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:19:23.93 +33:59:10.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34014_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 34014_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:38:43.76 +41:50:15.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194420_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 194420_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 06:00:24.49 +34:30:28.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38398_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 38398_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:21:48.53 +41:48:08.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98275_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 98275_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:49:09.53 +39:10:49.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 223926_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 223926_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:20:01.09 +33:57:34.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84974_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 84974_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:52:39.54 +39:34:28.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140783_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 140783_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:51:01.79 +37:18:20.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181008_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 181008_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:16:18.35 +34:18:50.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98445_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 98445_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:51:28.44 +39:08:52.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220776_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 220776_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:18:19.07 +33:46:06.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218749_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 218749_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:19:00.22 +33:44:58.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56929_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 56929_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:06:31.15 +41:13:59.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180333_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 180333_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:52:39.63 +33:55:08.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139019_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038
The candidate 139019_fd_Aur-03-Q2b1x1_2026-04-21_21-50-27_20.00sec_-4.90C_LIGHT_0038 did not pass the final checks
**** FOUND 05:59:42.96 +37:12:43.6 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 191s
Prepared the HTML report for the field Aur-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:28:49.77 +35:47:17.2
05:47:00.50 +40:10:49.0
05:59:56.71 +38:42:51.9
06:00:32.99 +38:06:38.9
05:33:43.91 +37:29:18.2
05:22:34.49 +36:41:39.8
05:28:28.14 +36:35:48.5
05:39:00.55 +34:12:09.8
05:35:51.17 +34:21:10.1
05:51:24.79 +34:03:45.2
05:28:42.44 +34:57:52.2
05:12:04.19 +33:57:46.8
05:23:05.96 +33:58:32.8
05:39:22.23 +33:56:16.3
05:18:14.53 +40:21:39.6
05:47:05.27 +40:56:38.7
05:38:19.93 +42:16:25.7
05:24:09.32 +34:46:44.2
05:30:29.53 +38:07:44.3
05:59:51.48 +41:47:36.1
05:25:44.63 +41:56:03.0
05:25:43.50 +41:03:07.1
05:57:35.26 +41:36:49.0
05:59:13.06 +41:57:06.9
06:02:51.88 +41:05:46.4
05:52:17.11 +34:45:03.7
05:56:27.27 +40:13:14.2
05:58:34.10 +41:28:43.3
05:56:39.34 +38:24:36.4
05:58:37.21 +35:27:09.4
05:53:33.77 +35:52:27.6
05:43:36.28 +41:46:04.5
05:49:49.79 +41:17:45.0
05:30:19.88 +41:09:17.2
05:37:30.14 +41:00:37.8
05:20:36.69 +40:42:37.6
06:01:56.82 +39:54:57.8
05:48:49.01 +40:05:29.2
05:55:04.38 +39:56:50.3
05:39:40.00 +40:09:11.1
########### Completed Aur-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:47:00.50 +40:10:49.0
05:28:49.77 +35:47:17.2
05:18:14.53 +40:21:39.6
05:47:05.27 +40:56:38.7
05:38:19.93 +42:16:25.7
05:24:09.32 +34:46:44.2
05:30:29.53 +38:07:44.3
05:59:51.48 +41:47:36.1
05:25:44.63 +41:56:03.0
05:25:43.50 +41:03:07.1
05:57:35.26 +41:36:49.0
05:59:13.06 +41:57:06.9
06:02:51.88 +41:05:46.4
05:52:17.11 +34:45:03.7
05:56:27.27 +40:13:14.2
05:58:34.10 +41:28:43.3
05:56:39.34 +38:24:36.4
05:58:37.21 +35:27:09.4
05:53:33.77 +35:52:27.6
05:37:30.14 +41:00:37.8
05:35:51.17 +34:21:10.1
05:55:04.38 +39:56:50.3
06:00:32.99 +38:06:38.9
05:39:22.23 +33:56:16.3
05:51:24.79 +34:03:45.2
05:28:28.14 +36:35:48.5
05:49:49.79 +41:17:45.0
05:39:00.55 +34:12:09.8
05:39:40.00 +40:09:11.1
05:23:05.96 +33:58:32.8
05:43:36.28 +41:46:04.5
05:12:04.19 +33:57:46.8
05:59:56.71 +38:42:51.9
05:20:36.69 +40:42:37.6
05:48:49.01 +40:05:29.2
05:30:19.88 +41:09:17.2
05:22:34.49 +36:41:39.8
05:28:42.44 +34:57:52.2
06:01:56.82 +39:54:57.8
05:33:43.91 +37:29:18.2
###################################################################################
05:47:00.50 +40:10:49.0 -- not an asteroid (will add it to exclusion list)
05:28:49.77 +35:47:17.2 -- not an asteroid (will add it to exclusion list)
05:18:14.53 +40:21:39.6 -- not an asteroid (will add it to exclusion list)
05:47:05.27 +40:56:38.7 -- not an asteroid (will add it to exclusion list)
05:38:19.93 +42:16:25.7 -- not an asteroid (will add it to exclusion list)
05:24:09.32 +34:46:44.2 -- not an asteroid (will add it to exclusion list)
05:30:29.53 +38:07:44.3 -- not an asteroid (will add it to exclusion list)
05:59:51.48 +41:47:36.1 -- not an asteroid (will add it to exclusion list)
05:25:44.63 +41:56:03.0 -- not an asteroid (will add it to exclusion list)
05:25:43.50 +41:03:07.1 -- not an asteroid (will add it to exclusion list)
05:57:35.26 +41:36:49.0 -- not an asteroid (will add it to exclusion list)
05:59:13.06 +41:57:06.9 -- not an asteroid (will add it to exclusion list)
06:02:51.88 +41:05:46.4 -- not an asteroid (will add it to exclusion list)
05:52:17.11 +34:45:03.7 -- not an asteroid (will add it to exclusion list)
05:56:27.27 +40:13:14.2 -- not an asteroid (will add it to exclusion list)
05:58:34.10 +41:28:43.3 -- not an asteroid (will add it to exclusion list)
05:56:39.34 +38:24:36.4 -- not an asteroid (will add it to exclusion list)
05:58:37.21 +35:27:09.4 -- not an asteroid (will add it to exclusion list)
05:53:33.77 +35:52:27.6 -- not an asteroid (will add it to exclusion list)
05:37:30.14 +41:00:37.8 -- not an asteroid (will add it to exclusion list)
05:35:51.17 +34:21:10.1 -- not an asteroid (will add it to exclusion list)
05:55:04.38 +39:56:50.3 -- not an asteroid (will add it to exclusion list)
06:00:32.99 +38:06:38.9 -- not an asteroid (will add it to exclusion list)
05:39:22.23 +33:56:16.3 -- not an asteroid (will add it to exclusion list)
05:51:24.79 +34:03:45.2 -- not an asteroid (will add it to exclusion list)
05:28:28.14 +36:35:48.5 -- not an asteroid (will add it to exclusion list)
05:49:49.79 +41:17:45.0 -- not an asteroid (will add it to exclusion list)
05:39:00.55 +34:12:09.8 -- not an asteroid (will add it to exclusion list)
05:39:40.00 +40:09:11.1 -- not an asteroid (will add it to exclusion list)
05:23:05.96 +33:58:32.8 -- not an asteroid (will add it to exclusion list)
05:43:36.28 +41:46:04.5 -- not an asteroid (will add it to exclusion list)
05:12:04.19 +33:57:46.8 -- not an asteroid (will add it to exclusion list)
05:59:56.71 +38:42:51.9 -- not an asteroid (will add it to exclusion list)
05:20:36.69 +40:42:37.6 -- not an asteroid (will add it to exclusion list)
05:48:49.01 +40:05:29.2 -- not an asteroid (will add it to exclusion list)
05:30:19.88 +41:09:17.2 -- not an asteroid (will add it to exclusion list)
05:22:34.49 +36:41:39.8 -- not an asteroid (will add it to exclusion list)
05:28:42.44 +34:57:52.2 -- not an asteroid (will add it to exclusion list)
06:01:56.82 +39:54:57.8 -- not an asteroid (will add it to exclusion list)
05:33:43.91 +37:29:18.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:12:04.19 +33:57:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:14.53 +40:21:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:36.69 +40:42:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:34.49 +36:41:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:05.96 +33:58:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:09.32 +34:46:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:43.50 +41:03:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:44.63 +41:56:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:28.14 +36:35:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:42.44 +34:57:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:49.77 +35:47:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:19.88 +41:09:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:29.53 +38:07:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:43.91 +37:29:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:51.17 +34:21:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:30.14 +41:00:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:19.93 +42:16:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:00.55 +34:12:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:22.23 +33:56:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:40.00 +40:09:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:36.28 +41:46:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:00.50 +40:10:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:05.27 +40:56:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:49.01 +40:05:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:49.79 +41:17:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:24.79 +34:03:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:17.11 +34:45:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:33.77 +35:52:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:04.38 +39:56:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:27.27 +40:13:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:39.34 +38:24:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:35.26 +41:36:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:34.10 +41:28:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:37.21 +35:27:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:13.06 +41:57:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:51.48 +41:47:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:56.71 +38:42:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:32.99 +38:06:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:56.82 +39:54:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:51.88 +41:05:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
05:12:04.19 +33:57:46.8 -- a known variable star
05:18:14.53 +40:21:39.6 -- a known variable star
05:20:36.69 +40:42:37.6 -- not a known variable star
05:22:34.49 +36:41:39.8 -- a known variable star
05:23:05.96 +33:58:32.8 -- a known variable star
05:24:09.32 +34:46:44.2 -- not a known variable star
05:25:43.50 +41:03:07.1 -- not a known variable star
05:25:44.63 +41:56:03.0 -- not a known variable star
05:28:28.14 +36:35:48.5 -- a known variable star
05:28:42.44 +34:57:52.2 -- a known variable star
05:28:49.77 +35:47:17.2 -- not a known variable star
05:30:19.88 +41:09:17.2 -- not a known variable star
05:30:29.53 +38:07:44.3 -- not a known variable star
05:33:43.91 +37:29:18.2 -- not a known variable star
05:35:51.17 +34:21:10.1 -- a known variable star
05:37:30.14 +41:00:37.8 -- not a known variable star
05:38:19.93 +42:16:25.7 -- not a known variable star
05:39:00.55 +34:12:09.8 -- not a known variable star
05:39:22.23 +33:56:16.3 -- a known variable star
05:39:40.00 +40:09:11.1 -- not a known variable star
05:43:36.28 +41:46:04.5 -- not a known variable star
05:47:00.50 +40:10:49.0 -- not a known variable star
05:47:05.27 +40:56:38.7 -- not a known variable star
05:48:49.01 +40:05:29.2 -- not a known variable star
05:49:49.79 +41:17:45.0 -- not a known variable star
05:51:24.79 +34:03:45.2 -- not a known variable star
05:52:17.11 +34:45:03.7 -- a known variable star
05:53:33.77 +35:52:27.6 -- not a known variable star
05:55:04.38 +39:56:50.3 -- not a known variable star
05:56:27.27 +40:13:14.2 -- not a known variable star
05:56:39.34 +38:24:36.4 -- not a known variable star
05:57:35.26 +41:36:49.0 -- not a known variable star
05:58:34.10 +41:28:43.3 -- a known variable star
05:58:37.21 +35:27:09.4 -- not a known variable star
05:59:13.06 +41:57:06.9 -- not a known variable star
05:59:51.48 +41:47:36.1 -- not a known variable star
05:59:56.71 +38:42:51.9 -- a known variable star
06:00:32.99 +38:06:38.9 -- not a known variable star
06:01:56.82 +39:54:57.8 -- not a known variable star
06:02:51.88 +41:05:46.4 -- not a known variable star
Found 29 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
40 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
05:12:04.19 +33:57:46.8
05:18:14.53 +40:21:39.6
05:20:36.69 +40:42:37.6
05:22:34.49 +36:41:39.8
05:23:05.96 +33:58:32.8
05:24:09.32 +34:46:44.2
05:25:43.50 +41:03:07.1
05:25:44.63 +41:56:03.0
05:28:28.14 +36:35:48.5
05:28:42.44 +34:57:52.2
05:28:49.77 +35:47:17.2
05:30:19.88 +41:09:17.2
05:30:29.53 +38:07:44.3
05:33:43.91 +37:29:18.2
05:35:51.17 +34:21:10.1
05:37:30.14 +41:00:37.8
05:38:19.93 +42:16:25.7
05:39:00.55 +34:12:09.8
05:39:22.23 +33:56:16.3
05:39:40.00 +40:09:11.1
05:43:36.28 +41:46:04.5
05:47:00.50 +40:10:49.0
05:47:05.27 +40:56:38.7
05:48:49.01 +40:05:29.2
05:49:49.79 +41:17:45.0
05:51:24.79 +34:03:45.2
05:52:17.11 +34:45:03.7
05:53:33.77 +35:52:27.6
05:55:04.38 +39:56:50.3
05:56:27.27 +40:13:14.2
05:56:39.34 +38:24:36.4
05:57:35.26 +41:36:49.0
05:58:34.10 +41:28:43.3
05:58:37.21 +35:27:09.4
05:59:13.06 +41:57:06.9
05:59:51.48 +41:47:36.1
05:59:56.71 +38:42:51.9
06:00:32.99 +38:06:38.9
06:01:56.82 +39:54:57.8
06:02:51.88 +41:05:46.4
06:01:58.90 +39:54:58.5
05:13:59.08 +38:24:31.6
05:11:28.24 +42:03:15.2
05:12:13.27 +34:19:47.3
05:39:17.91 +39:48:40.1
05:07:43.55 +40:45:37.5
05:49:00.81 +36:16:36.9
05:38:14.37 +40:07:24.0
05:08:26.87 +34:10:11.0
05:28:47.33 +38:31:41.5
05:28:06.17 +39:14:50.3
05:26:49.95 +38:36:49.5
05:17:02.18 +41:07:13.6
05:26:33.92 +38:13:48.5
05:12:55.46 +40:35:29.4
05:53:48.40 +35:10:12.6
05:10:11.88 +40:03:03.8
05:33:17.32 +38:21:23.2
05:22:25.10 +37:05:14.5
05:26:49.49 +38:48:21.6
05:15:07.90 +36:33:16.2
05:35:09.78 +40:32:00.9
05:34:27.21 +38:34:09.7
05:20:27.16 +36:53:45.0
05:39:45.62 +33:55:43.2
05:31:34.21 +37:53:07.6
05:54:03.60 +37:23:42.1
05:18:35.21 +38:05:00.7
05:13:13.81 +34:11:48.5
05:37:26.41 +39:43:07.6
05:23:14.93 +38:36:17.1
05:26:59.62 +38:59:43.2
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461152.61784931 -observatory V36
00:41:24.10 +01:39:46.1 Mercury (-0.2mag)
03:38:54.11 +19:59:59.3 Venus (-3.9mag)
00:35:11.56 +02:45:59.5 Mars (1.2mag)
07:15:36.35 +22:41:13.4 Jupiter (-2.1mag)
00:31:52.68 +01:05:42.5 Saturn (0.9mag)
03:49:00.99 +19:51:40.8 Uranus (5.8mag)
00:11:37.50 -00:10:26.6 Neptune (7.8mag)
20:33:59.10 -22:53:01.1 Pluto (14.5mag)
06:22:05.02 +27:33:55.2 Moon (-9.7mag)
-rw-r--r-- 1 apache apache 362 Apr 21 21:57 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461152.61784931:
07:15:40.59 +22:41:02.0 Io (5.8mag)
07:15:24.54 +22:41:39.5 Europa (5.9mag)
07:15:54.14 +22:40:38.0 Ganymede (5.4mag)
07:15:15.95 +22:41:48.9 Callisto (6.6mag)
07:18:39.37 +22:26:09.5 Himalia (15.4mag)
07:15:37.35 +22:41:08.9 Thebe (16.3mag)
07:18:57.91 +22:56:27.9 Elara (17.3mag)
07:14:54.14 +23:18:01.7 Pasiphae (17.4mag)
07:23:47.45 +22:39:48.0 Carme (18.6mag)
00:31:46.89 +01:05:41.6 Titan (8.8mag)
00:31:58.46 +01:05:44.0 Rhea (10.1mag)
00:31:24.79 +01:04:53.9 Iapetus (11.5mag)
00:31:41.91 +01:05:59.1 Hyperion (14.8mag)
00:33:24.53 +01:13:49.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 21 21:57 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461152.61784931:
16:02:57.67 -20:11:40.8 JWST
17:04:42.81 +43:57:51.7 Chandra
07:53:20.36 -35:16:16.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 21 21:57 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461152.61784931 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
05:29:56.06 +30:49:47.6 18.0mag P/2009 WX51 (Catalina)
18:54:05.71 -29:09:09.2 13.8mag P/2010 H2 (Vales)
05:11:17.25 -69:23:00.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:52.10 +31:28:53.6 17.3mag C/2017 K2 (PANSTARRS)
17:29:38.43 +11:15:37.6 17.6mag C/2021 G2 (ATLAS)
23:11:42.89 +29:28:54.3 17.1mag C/2022 E2 (ATLAS)
04:36:26.31 +26:11:57.9 16.1mag C/2022 N2 (PANSTARRS)
09:04:58.77 +32:01:52.8 16.3mag C/2022 QE78 (ATLAS)
08:32:12.03 +00:28:24.7 17.4mag C/2022 R6 (PANSTARRS)
18:52:03.99 +19:02:06.4 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:38:33.54 -11:25:52.8 17.5mag P/2023 B1 (PANSTARRS)
09:05:06.02 -10:55:50.8 17.7mag C/2023 F3 (ATLAS)
21:59:55.81 +63:16:50.1 17.6mag C/2023 H5 (Lemmon)
19:13:17.11 -03:51:16.7 14.1mag C/2023 R1 (PANSTARRS)
21:12:53.70 +86:46:15.2 17.8mag C/2023 X2 (Lemmon)
06:21:14.93 +63:30:00.2 17.2mag C/2024 A1 (ATLAS)
05:25:58.51 +20:09:54.0 11.4mag C/2024 E1 (Wierzchos)
16:15:08.52 +07:23:05.1 17.3mag C/2024 G6 (ATLAS)
20:22:15.80 +16:58:04.6 14.5mag C/2024 J3 (ATLAS)
03:31:56.83 -21:28:36.3 16.3mag C/2024 T5 (ATLAS)
05:22:01.23 +43:49:08.8 17.7mag C/2025 J1 (Borisov)
13:13:57.98 +48:47:48.8 15.5mag C/2025 L1 (ATLAS)
03:35:13.59 -27:12:12.1 17.9mag C/2025 Q3 (ATLAS)
01:03:41.92 +14:18:19.2 7.8mag C/2025 R3 (PANSTARRS)
12:51:31.03 +03:22:07.5 17.4mag C/2025 Y1 (ATLAS)
04:09:52.10 +02:07:52.0 14.8mag C/2026 A1 (MAPS)
00:16:29.03 +38:16:30.9 14.8mag C/2026 B2 (Sun-Gao)
18:54:48.61 -09:23:07.6 11.5mag 10P/Tempel
14:51:57.70 +02:30:59.9 14.5mag 24P/Schaumasse
11:01:20.85 -01:20:30.9 15.7mag 29P/Schwassmann-Wachmann
10:37:44.64 -03:39:06.6 17.0mag 43P/Wolf-Harrington
01:58:10.18 +18:31:09.0 17.3mag 47P/Ashbrook-Jackson
07:22:19.81 +35:40:35.0 17.0mag 63P/Wild
23:36:44.13 -10:43:50.4 15.7mag 65P/Gunn
04:19:54.16 +23:16:54.5 15.9mag 76P/West-Kohoutek-Ikemura
01:19:11.75 +09:25:09.0 14.3mag 78P/Gehrels
23:21:10.20 -07:34:55.6 14.7mag 88P/Howell
02:27:58.09 +22:13:35.3 15.1mag 93P/Lovas
05:06:37.04 +32:35:33.5 16.1mag 123P/West-Hartley
08:36:00.63 +35:32:44.7 16.2mag 124P/Mrkos
02:42:44.67 +15:02:27.6 16.4mag 128P/Shoemaker-Holt
02:59:35.24 +15:12:57.7 17.5mag 131P/Mueller
01:58:46.30 +15:12:02.1 10.5mag 141P/Machholz
02:06:42.65 +07:08:23.2 10.5mag 141P-A/Machholz
00:49:25.87 +02:53:39.7 12.1mag 141P-D/Machholz
02:37:20.15 +08:52:36.2 17.9mag 141P-I/Machholz
01:19:31.72 +01:33:49.2 15.0mag 162P/SidingSpring
14:40:41.47 +00:29:40.9 17.8mag 210P/Christensen
21:55:49.96 -09:59:24.7 17.8mag 218P/LINEAR
17:17:23.70 -13:11:09.5 16.1mag 235P/LINEAR
05:47:51.00 +35:06:50.8 16.8mag 240P/NEAT
07:41:44.36 -04:32:05.4 17.8mag 242P/Spahr
22:32:13.20 -19:17:21.6 17.7mag 260P/McNaught
02:10:53.16 +21:59:17.0 17.9mag 295P/LINEAR
15:40:02.68 +07:22:15.1 17.5mag 391P/Kowalski
07:36:46.13 +21:22:23.8 17.7mag 450P/LONEOS
05:44:56.97 +44:40:31.8 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 21 21:57 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
-rw-r--r-- 1 apache apache 5.8K Apr 21 21:57 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 21 21:57 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
12:06:16.602 -06:52:59.29 AT 2026jpa 2026-04-13.89 19.276
06:42:32.732 -34:30:04.15 AT 2026joz 2026-04-14.77 18.707
13:06:33.339 -08:24:24.46 AT 2026joy 2026-04-14.02 19.307
21:07:11.613 -12:36:56.09 AT 2026jox 2026-04-14.14 18.849
05:34:42.408 -28:21:31.62 AT 2026jow 2026-04-14.74 18.902
12:30:54.108 -14:11:53.07 AT 2026jov 2026-04-14.03 19.309
05:52:53.155 -34:43:22.49 AT 2026jou 2026-04-14.75 19.398
05:40:18.921 -24:52:33.50 AT 2026jot 2026-04-14.77 18.65
15:53:02.304 +04:30:53.21 AT 2026jos 2026-04-14.09 19.566
11:19:37.053 +36:36:59.54 AT 2026jor 2026-04-11.94 20.14
08:17:15.784 +16:04:01.41 AT 2026joq 2026-04-11.86 19.95
15:52:58.319 -17:01:02.93 AT 2026jop 2026-04-09.53 19.69
09:28:29.338 +17:46:10.46 AT 2026joo 2026-04-11.90 19.1
14:08:31.151 +20:01:29.32 AT 2026jon 2026-04-08.02 19.9
08:15:22.510 -21:29:08.39 AT 2026jom 2026-04-12.37 19.76
12:13:11.990 +05:30:27.70 AT 2026jol 2026-04-08.25 16.6
09:57:55.902 +03:33:01.27 AT 2026jok 2026-03-06.10 21.72
15:47:58.800 -16:07:43.45 AT 2026joj 2026-04-10.44 20.1583
09:57:44.859 +01:08:42.73 AT 2026joi 2026-04-06.02 22.85
14:40:55.647 +05:24:36.73 SN 2026joh 2026-04-14.03 17.708
-rw-r--r-- 1 apache apache 30K Apr 21 21:57 tns_transients_list.txt
