This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI
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 09 06.2965 2461289.7965 11.05 05:31:34.44 +37:53:11.4
170.86749 2.30247 galactic Aur Second-epoch detections are separated by 0.4" and 5.7 pix
The object was found in VSX 0" ASASSN-V J053134.42+375311.7
Type: SR
# Max. Min./Amp. JD0 Period
12.590 V 13.050 V 2457823.80000 73.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:31:34.44 +37:53:11.4: 11.99 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:31:34.44 +37:53:11.4: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 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
ASASSN-V J053134.42+375311.7,2461289.7965,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053134.42+375311.7 20260906.2965 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.43 05:09:58.01 +36:14:44.0
169.75548 -2.17270 galactic Aur Second-epoch detections are separated by 0.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.980 Anacostia -1 -0 1 12.7 0 0
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:09:58.01 +36:14:44.0: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:09:58.01 +36:14:44.0: 15.71 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461289.7965,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260906.2965 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.91 05:25:50.95 +39:25:03.8
168.97222 2.21770 galactic Aur Second-epoch detections are separated by 0.9" 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 | ATO J081.4619+39.4179 | 05:25:50.95 +39:25:03.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K7 (LAMOST DR5) J-Ks=1.501+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:25:50.95 +39:25:03.8: 13.89 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:25:50.95 +39:25:03.8: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.4619+39.4179,2461289.7965,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.4619+39.4179 20260906.2965 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 13.02 05:24:17.43 +37:16:09.8
170.57984 0.75957 galactic Aur Second-epoch detections are separated by 5.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J081.0750+37.2631 | 05:24:17.43 +37:16:09.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:24:17.43 +37:16:09.8: 13.92 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:24:17.43 +37:16:09.8: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 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 J081.0750+37.2631,2461289.7965,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.0750+37.2631 20260906.2965 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.89 05:35:27.86 +37:11:40.0
171.86825 2.57439 galactic Aur Second-epoch detections are separated by 2.1" and 5.8 pix
The object was found in VSX 1" ZTF J053527.77+371140.1
Type: SR
# Max. Min./Amp. JD0 Period
15.549 g Y 0.194 g 2458432.83990 59.210346100000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:35:27.86 +37:11:40.0: 14.06 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:35:27.86 +37:11:40.0: 13.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.95 +/- 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
ZTF J053527.77+371140.1,2461289.7965,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J053527.77+371140.1 20260906.2965 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 13.10 05:05:49.67 +36:22:10.9
169.15672 -2.76673 galactic Aur Second-epoch detections are separated by 2.7" and 5.2 pix
The object was found in VSX 0" ZTF J050549.65+362210.4
Type: SR
# Max. Min./Amp. JD0 Period
13.380 r Y 0.171 r 2458526.73150 40.609851400000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:05:49.67 +36:22:10.9: 14.07 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:05:49.67 +36:22:10.9: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 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
ZTF J050549.65+362210.4,2461289.7965,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J050549.65+362210.4 20260906.2965 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 11.80 05:22:17.16 +36:57:51.8
170.60564 0.25754 galactic Aur Second-epoch detections are separated by 1.6" 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 | VSSP J052217.88+365753.2 | 05:22:17.04 +36:57:52.6 (Gaia DR3) | E (VSX @ VizieR) | 0.343303000000 (VSX @ VizieR) | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5) J-Ks=1.410+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:22:17.16 +36:57:51.8: 12.76 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:22:17.16 +36:57:51.8: 12.71 +/- 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
VSSP J052217.88+365753.2,2461289.7965,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VSSP J052217.88+365753.2 20260906.2965 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.09 05:31:34.75 +37:21:56.9
171.30424 2.01848 galactic Aur Second-epoch detections are separated by 0.9" and 5.5 pix
The object was found in VSX 5" ASASSN-V J053134.85+372201.7
Type: SRS
# Max. Min./Amp. JD0 Period
14.650 g Y 0.140 g 2459121.95600 26.938000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:31:34.75 +37:21:56.9: 13.19 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:31:34.75 +37:21:56.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053134.85+372201.7,2461289.7965,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053134.85+372201.7 20260906.2965 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.43 05:29:04.39 +38:16:12.1
170.27617 2.10209 galactic Aur Second-epoch detections are separated by 0.9" and 5.5 pix
The object was found in VSX 1" Gaia DR3 190567217889022720
Type: L
# Max. Min./Amp. JD0 Period
11.880 G 12.000 G M
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:29:04.39 +38:16:12.1: 13.34 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:29:04.39 +38:16:12.1: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 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 190567217889022720,2461289.7965,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 190567217889022720 20260906.2965 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.50 05:22:50.86 +37:36:37.8
170.13657 0.71572 galactic Aur Second-epoch detections are separated by 0.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J080.7119+37.6105 | 05:22:50.86 +37:36:37.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M0 (LAMOST DR5) J-Ks=1.348+/-0.024 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:22:50.86 +37:36:37.8: 13.39 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:22:50.86 +37:36:37.8: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 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 J080.7119+37.6105,2461289.7965,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.7119+37.6105 20260906.2965 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.71 05:21:39.05 +37:47:05.9
169.85856 0.61974 galactic Aur Second-epoch detections are separated by 0.8" and 5.6 pix
The object was found in VSX 1" ZTF J052139.09+374705.5
Type: SR
# Max. Min./Amp. JD0 Period
15.069 g Y 0.253 g 2458193.56010 215.644782800000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:21:39.05 +37:47:05.9: 13.67 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:21:39.05 +37:47:05.9: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.65 +/- 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
ZTF J052139.09+374705.5,2461289.7965,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J052139.09+374705.5 20260906.2965 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.78 05:31:51.67 +37:21:15.4
171.34456 2.05909 galactic Aur Second-epoch detections are separated by 0.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:31:51.67 +37:21:15.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.468+/-0.024 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:31:51.67 +37:21:15.4: 13.65 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:31:51.67 +37:21:15.4: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 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
target,2461289.7965,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2965 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.85 05:36:05.09 +38:07:01.9
171.15555 3.17429 galactic Aur Second-epoch detections are separated by 2.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J084.0211+38.1172 | 05:36:05.09 +38:07:01.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: M0 (LAMOST DR5) J-Ks=1.484+/-0.028 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:36:05.09 +38:07:01.9: 13.81 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:36:05.09 +38:07:01.9: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.0211+38.1172,2461289.7965,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.0211+38.1172 20260906.2965 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.71 05:45:26.24 +38:32:10.8
171.76660 4.95428 galactic Aur Second-epoch detections are separated by 1.7" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J086.3588+38.5367 | 05:45:26.24 +38:32:10.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.340+/-0.039 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:45:26.24 +38:32:10.8: 13.72 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:45:26.24 +38:32:10.8: 13.78 +/- 0.04 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
ATO J086.3588+38.5367,2461289.7965,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.3588+38.5367 20260906.2965 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.80 05:27:07.60 +37:21:25.1
170.82304 1.27586 galactic Aur Second-epoch detections are separated by 2.5" and 5.9 pix
The object was found in VSX 1" ZTF J052707.54+372125.9
Type: SR
# Max. Min./Amp. JD0 Period
14.996 g Y 0.114 g 2458380.25090 24.961798600000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:27:07.60 +37:21:25.1: 13.71 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:27:07.60 +37:21:25.1: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 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
ZTF J052707.54+372125.9,2461289.7965,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J052707.54+372125.9 20260906.2965 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.65 05:47:51.28 +38:34:38.8
171.97479 5.38093 galactic Aur Second-epoch detections are separated by 0.8" and 5.5 pix
The object was found in VSX 1" ASASSN-V J054751.27+383440.1
Type: L
# Max. Min./Amp. JD0 Period
13.680 V 14.150 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:47:51.28 +38:34:38.8: 13.68 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:47:51.28 +38:34:38.8: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 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
ASASSN-V J054751.27+383440.1,2461289.7965,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J054751.27+383440.1 20260906.2965 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.61 05:17:13.30 +35:18:57.7
171.37149 -1.52457 galactic Aur Second-epoch detections are separated by 1.3" and 5.9 pix
The object was found in VSX 0" ASASSN-V J051713.28+351857.6
Type: L
# Max. Min./Amp. JD0 Period
14.130 V 14.280 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:17:13.30 +35:18:57.7: 13.61 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:17:13.30 +35:18:57.7: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 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
ASASSN-V J051713.28+351857.6,2461289.7965,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051713.28+351857.6 20260906.2965 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 09 06.2965 2461289.7965 12.64 05:23:09.47 +37:30:30.7
170.25544 0.70872 galactic Aur Second-epoch detections are separated by 1.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:23:09.47 +37:30:30.7 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5) J-Ks=1.233+/-0.024 (M)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:23:09.47 +37:30:30.7: 13.55 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:23:09.47 +37:30:30.7: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.58 +/- 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
target,2461289.7965,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2965 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.63 05:36:14.11 +37:56:39.8
171.31747 3.10650 galactic Aur Second-epoch detections are separated by 1.8" and 5.5 pix
The object was found in VSX 1" ASASSN-V J053614.04+375640.8
Type: SRS
# Max. Min./Amp. JD0 Period
13.780 V 13.970 V 2457039.85200 26.656000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:36:14.11 +37:56:39.8: 13.54 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:36:14.11 +37:56:39.8: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 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
ASASSN-V J053614.04+375640.8,2461289.7965,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053614.04+375640.8 20260906.2965 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 09 06.2965 2461289.7965 13.33 04:56:35.81 +35:11:01.6
168.94818 -4.97310 galactic Aur Second-epoch detections are separated by 1.2" and 5.5 pix
The object was found in VSX 2" ASASSN-V J045635.70+351059.5
Type: SRS:
# Max. Min./Amp. JD0 Period
16.570 g Y 0.380 g 2458772.96200 10.620000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:56:35.81 +35:11:01.6: 14.56 +/- 0.10 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:56:35.81 +35:11:01.6: 14.40 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045635.70+351059.5,2461289.7965,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045635.70+351059.5 20260906.2965 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.55 05:20:26.13 +38:08:02.6
169.43517 0.62185 galactic Aur Second-epoch detections are separated by 1.2" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J080.1088+38.1342 | 05:20:26.12 +38:08:03.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M4 (LAMOST DR5) J-Ks=1.465+/-0.039 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:26.13 +38:08:02.6: 13.45 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:26.13 +38:08:02.6: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.1088+38.1342,2461289.7965,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.1088+38.1342 20260906.2965 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.47 05:32:09.90 +37:20:04.0
171.39419 2.09883 galactic Aur Second-epoch detections are separated by 0.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J083.0410+37.3344 | 05:32:09.85 +37:20:03.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: M1 (LAMOST DR5) J-Ks=1.644+/-0.024 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:32:09.90 +37:20:04.0: 13.43 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:32:09.90 +37:20:04.0: 13.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.45 +/- 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 J083.0410+37.3344,2461289.7965,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.0410+37.3344 20260906.2965 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.32 05:20:28.20 +39:26:18.2
168.36811 1.37223 galactic Aur Second-epoch detections are separated by 0.2" and 5.6 pix
The object was found in VSX 1" NEV46
Type: SRS
# Max. Min./Amp. JD0 Period
13.680 V 14.130 V 2457668.08000 29.390000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:28.20 +39:26:18.2: 13.33 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:28.20 +39:26:18.2: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 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
NEV46,2461289.7965,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NEV46 20260906.2965 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.20 05:40:16.66 +38:35:46.9
171.18737 4.12519 galactic Aur Second-epoch detections are separated by 1.1" and 5.5 pix
The object was found in VSX 1" ASASSN-V J054016.74+383547.8
Type: SR
# Max. Min./Amp. JD0 Period
14.600 g Y 0.370 g 2459099.05000 70.010000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:40:16.66 +38:35:46.9: 13.22 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:40:16.66 +38:35:46.9: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J054016.74+383547.8,2461289.7965,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J054016.74+383547.8 20260906.2965 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.11 05:20:46.20 +36:06:46.5
171.13263 -0.47731 galactic Aur Second-epoch detections are separated by 1.5" and 5.9 pix
The object was found in VSX 1" ZTF J052046.17+360647.7
Type: SR
# Max. Min./Amp. JD0 Period
14.409 g Y 0.217 g 2458206.65240 86.893218700000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:46.20 +36:06:46.5: 13.00 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:46.20 +36:06:46.5: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 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
ZTF J052046.17+360647.7,2461289.7965,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J052046.17+360647.7 20260906.2965 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 09 06.2965 2461289.7965 12.04 05:24:00.67 +37:05:19.0
170.69788 0.61177 galactic Aur Second-epoch detections are separated by 1.0" and 5.5 pix
The object was found in VSX 1" ASASSN-V J052400.72+370519.2
Type: SR
# Max. Min./Amp. JD0 Period
13.190 V 13.590 V 2458385.73690 81.318819100000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:24:00.67 +37:05:19.0: 12.99 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:24:00.67 +37:05:19.0: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052400.72+370519.2,2461289.7965,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052400.72+370519.2 20260906.2965 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 13.23 05:32:41.29 +38:27:36.4
170.50588 2.79893 galactic Aur Second-epoch detections are separated by 3.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J083.1716+38.4602 | 05:32:41.29 +38:27:36.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=1.519+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:32:41.29 +38:27:36.4: 14.36 +/- 0.07 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:32:41.29 +38:27:36.4: 14.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.1716+38.4602,2461289.7965,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.1716+38.4602 20260906.2965 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.04 05:37:15.19 +39:47:47.7
169.85549 4.26468 galactic Aur Second-epoch detections are separated by 0.9" and 5.7 pix
The object was found in VSX 1" ASASSN-V J053715.12+394747.5
Type: SR
# Max. Min./Amp. JD0 Period
12.950 V 13.370 V 2457095.80000 344.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:37:15.19 +39:47:47.7: 12.98 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:37:15.19 +39:47:47.7: 13.00 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053715.12+394747.5,2461289.7965,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053715.12+394747.5 20260906.2965 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 13.24 05:19:54.15 +36:28:35.7
170.73430 -0.41293 galactic Aur Second-epoch detections are separated by 2.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:19:54.15 +36:28:35.7 (user input) | T | P | (position from user input) SpType: K5 (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:19:54.15 +36:28:35.7: 14.17 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:19:54.15 +36:28:35.7: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.17 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7965,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2965 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 11.96 05:27:42.97 +38:15:22.3
170.14011 1.87263 galactic Aur Second-epoch detections are separated by 0.9" and 5.6 pix
The object was found in VSX 0" ZTF J052742.99+381522.5
Type: SR
# Max. Min./Amp. JD0 Period
12.058 r Y 0.423 r 2458336.86460 66.714520900000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:27:42.97 +38:15:22.3: 12.78 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:27:42.97 +38:15:22.3: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 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
ZTF J052742.99+381522.5,2461289.7965,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J052742.99+381522.5 20260906.2965 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 13.15 05:31:53.33 +37:35:55.4
171.14270 2.19727 galactic Aur Second-epoch detections are separated by 1.0" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:31:53.33 +37:35:55.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.473+/-0.024 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:31:53.33 +37:35:55.4: 14.24 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:31:53.33 +37:35:55.4: 14.28 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7965,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2965 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 13.17 05:21:25.37 +37:42:32.9
169.89529 0.53954 galactic Aur Second-epoch detections are separated by 0.2" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:21:25.37 +37:42:32.9 (user input) | T | P | (position from user input) SpType: M0 (LAMOST DR5) J-Ks=1.430+/-0.026 (Very red! L if it's a dwarf)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:21:25.37 +37:42:32.9: 14.23 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:21:25.37 +37:42:32.9: 14.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7965,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2965 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 13.06 05:25:40.54 +38:52:38.0
169.40179 1.88759 galactic Aur Second-epoch detections are separated by 1.5" 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 | target | 05:25:40.54 +38:52:38.0 (user input) | T | P | (position from user input) SpType: M2 (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:25:40.54 +38:52:38.0: 14.05 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:25:40.54 +38:52:38.0: 14.16 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461289.7965,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260906.2965 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.90 05:01:27.55 +33:10:54.4
171.15409 -5.41222 galactic Aur Second-epoch detections are separated by 2.1" and 5.4 pix
The object was found in VSX 1" ASASSN-V J050127.44+331054.4
Type: L
# Max. Min./Amp. JD0 Period
14.310 V 14.650 V
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:01:27.55 +33:10:54.4: 14.01 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:01:27.55 +33:10:54.4: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 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
ASASSN-V J050127.44+331054.4,2461289.7965,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050127.44+331054.4 20260906.2965 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.91 05:38:07.86 +36:52:05.5
172.42960 2.84874 galactic Aur Second-epoch detections are separated by 4.2" and 5.2 pix
The object was found in VSX 2" ASASSN-V J053807.98+365206.6
Type: SR
# Max. Min./Amp. JD0 Period
15.640 g Y 0.330 g 2458592.62200 257.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:38:07.86 +36:52:05.5: 13.98 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:38:07.86 +36:52:05.5: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 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
ASASSN-V J053807.98+365206.6,2461289.7965,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053807.98+365206.6 20260906.2965 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.74 05:30:38.78 +37:43:02.9
170.90850 2.05656 galactic Aur Second-epoch detections are separated by 1.6" 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 | ATO J082.6616+37.7183 | 05:30:38.78 +37:43:02.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F6 (LAMOST DR5)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:30:38.78 +37:43:02.9: 13.57 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:30:38.78 +37:43:02.9: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.6616+37.7183,2461289.7965,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.6616+37.7183 20260906.2965 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 06.2965 2461289.7965 12.96 05:18:46.64 +39:20:46.1
168.25638 1.05133 galactic Aur Second-epoch detections are separated by 1.0" and 5.7 pix
The object was found in VSX12" Gaia DR3 187973199380132608
Type: ROT
# Max. Min./Amp. JD0 Period
15.870 G 15.900 G K
The object was not found in astcheck.
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:18:46.64 +39:20:46.1: 13.91 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:18:46.64 +39:20:46.1: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 187973199380132608,2461289.7965,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 187973199380132608 20260906.2965 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461289.79678641 06.09.2026 07:07:12.346 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 14
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 24192
Objects passed selection criteria: 24054
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: 17318.8
Average stars matched: 16514.8 (95.3576 %)
Memory usage VmPeak: 251428 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 6 02:09:18 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: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461058.61200600 18.01.2026 02:41:07.318 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461289.79678641 06.09.2026 07:07:12.346 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 201
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 55 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 180744
Objects passed selection criteria: 180218
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: 129584
Average stars matched: 121157 (93.4969 %)
Memory usage VmPeak: 649024 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 6 02:10:54 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.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: 2461289.79621143
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits exists and is non-empty
wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:16.998 +37:59:58.58 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
Image size: 943.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:17.780 +37:57:25.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:16.998 +37:59:58.58
Second-epoch image center 05:27:17.780 +37:57:25.33
Angular distance between the image centers 0.0426 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
Image size: 943.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:17.381 +37:57:58.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:16.998 +37:59:58.58
Second-epoch image center 05:27:17.381 +37:57:58.42
Angular distance between the image centers 0.0334 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 05:27:17.780 +37:57:25.33
Second-epoch second image center 05:27:17.381 +37:57:58.42
Angular distance between the image centers 0.00928 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.XqZaXQDxjV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.tIUaOHSFV5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits &> /tmp/tmp.OZmqfegHSy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits &> /tmp/tmp.HNbMidgvI1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
The reference image (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat) found
'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat' -> 'wcsmag.cat'
Read 27843 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8756 to 92.1259 deg, Dec +31.9880 to +43.3913 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.8756 to 92.1259 deg, Dec 31.9880 to 43.3913 deg
Loaded 16034 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): 11109 out of 12457 total matches.
Matched with Tycho-2 12457 out of 27843 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.927300
a=0.000000 b=1.000000 c=22.927300
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 27843 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8756 to 92.1259 deg, Dec +31.9880 to +43.3913 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.8756 to 92.1259 deg, Dec 31.9880 to 43.3913 deg
Loaded 16034 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): 11109 out of 12457 total matches.
Matched with Tycho-2 12457 out of 27843 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (aperture=6.2)
Read 27116 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3491 to 92.6948 deg, Dec +32.1392 to +43.3190 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 71.3491 to 92.6948 deg, Dec 32.1392 to 43.3190 deg
Loaded 16026 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): 11083 out of 12589 total matches.
Matched with Tycho-2 12589 out of 27116 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
2.1 pix Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
3.1 pix fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
3.1 pix fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
Limiting magnitude estimates:
15.2 mag. Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
15.2 mag. Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
13.1 mag. fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
13.1 mag. fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
All-image limiting magnitude estimate: 13.1 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.XqZaXQDxjV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2982, bad_region=0, passed=27843
Got 27843 stars (including 24835 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
util/solve_plate_with_UCAC5 got 27843 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 4823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 27843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 27843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 27843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4821 stars left (next iteration limit 5305)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits N_match=4821 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.462 sigma_q2_arcsec=0.372 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.289 n_q1=919 n_q2=1327 n_q3=1362 n_q4=1213 worst_quadrant_to_overall_ratio=1.287
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.tIUaOHSFV5 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3147, bad_region=0, passed=27116
Got 27116 stars (including 23937 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
util/solve_plate_with_UCAC5 got 27116 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 4824 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 27116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4822 matched stars entering correct_measured_positions(), 27116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4822 matched stars entering correct_measured_positions(), 27116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4822 stars left (next iteration limit 5305)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits N_match=4822 sigma_overall_arcsec=0.496 sigma_q1_arcsec=0.624 sigma_q2_arcsec=0.487 sigma_q3_arcsec=0.457 sigma_q4_arcsec=0.442 n_q1=1116 n_q2=1448 n_q3=1299 n_q4=959 worst_quadrant_to_overall_ratio=1.258
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.OZmqfegHSy (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_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.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_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=261, bad_region=0, passed=7317
Got 7317 stars (including 7054 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat
util/solve_plate_with_UCAC5 got 7317 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.2'
Seting catalog search parameters based on the expected field of view 943.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013100 (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 0.010480 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.3)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 4820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 7314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.3)
Done reading UCAC5 zone files...
Matched 4883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 7314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 7314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4817 stars left (next iteration limit 5298)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4817 robust_rms=5.808 arcsec worst_quadrant_rms=6.341 arcsec
SIP_REFIT: SIP order 3 trial: matched=4817 robust_rms=0.500 arcsec worst_quadrant_rms=0.693 arcsec
SIP_REFIT: SIP order 5 trial: matched=4817 robust_rms=0.420 arcsec worst_quadrant_rms=0.544 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4817 robust_rms_before=1.026 arcsec robust_rms_before_corrected=0.462 arcsec robust_rms_after=0.420 arcsec worst_quadrant_rms_before=0.552 worst_quadrant_rms_after=0.544
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.552 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits N_match=4817 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.450 sigma_q2_arcsec=0.535 sigma_q3_arcsec=0.410 sigma_q4_arcsec=0.432 n_q1=1343 n_q2=1245 n_q3=1003 n_q4=1226 worst_quadrant_to_overall_ratio=1.166
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits -region wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.HNbMidgvI1 (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_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.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_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=266, bad_region=1, passed=7388
Got 7388 stars (including 7116 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat
util/solve_plate_with_UCAC5 got 7388 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.2'
Seting catalog search parameters based on the expected field of view 943.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013100 (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 0.010480 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.3)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 4824 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 7388 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.3)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 7388 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 7388 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4819 stars left (next iteration limit 5303)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4819 robust_rms=5.512 arcsec worst_quadrant_rms=6.263 arcsec
SIP_REFIT: SIP order 3 trial: matched=4819 robust_rms=0.492 arcsec worst_quadrant_rms=0.651 arcsec
SIP_REFIT: SIP order 5 trial: matched=4819 robust_rms=0.413 arcsec worst_quadrant_rms=0.518 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4819 robust_rms_before=1.013 arcsec robust_rms_before_corrected=0.448 arcsec robust_rms_after=0.413 arcsec worst_quadrant_rms_before=0.537 worst_quadrant_rms_after=0.518
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.537 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits N_match=4819 sigma_overall_arcsec=0.442 sigma_q1_arcsec=0.431 sigma_q2_arcsec=0.525 sigma_q3_arcsec=0.365 sigma_q4_arcsec=0.437 n_q1=1344 n_q2=1257 n_q3=987 n_q4=1231 worst_quadrant_to_overall_ratio=1.189
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits -region wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
Saving the final (post-refit) wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits to local_wcs_cache/
'wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
Saving the final (post-refit) wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits'
Saving the final (post-refit) wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits sigma_overall=0.359 worst_q_ratio=1.287
ref2=Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits sigma_overall=0.496 worst_q_ratio=1.258
new1=fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits sigma_overall=0.459 worst_q_ratio=1.166
new2=fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits sigma_overall=0.442 worst_q_ratio=1.189
reference average sigma_overall=0.4275 worst_q_ratio=1.2725
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049_astrometric_residuals.png (4821 matched stars from wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054_astrometric_residuals.png (4822 matched stars from wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173_astrometric_residuals.png (4817 matched stars from wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174_astrometric_residuals.png (4819 matched stars from wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits'
Saving fully-calibrated image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits'
Preparing the HTML report for the field Aur-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:28:05.06 +35:19:25.1: 11.11 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:31:34.44 +37:53:11.4: 11.99 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:28:05.06 +35:19:25.1: 11.14 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.12 +/- 0.01
Forced photometry filter REJECTED candidate at 05:28:05.06 +35:19:25.1: ref_mag=11.12 +/- 0.01 new_mean_mag=10.6994 delta=0.42 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:31:34.44 +37:53:11.4: 12.05 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter KEPT candidate at 05:31:34.44 +37:53:11.4: ref_mag=12.02 +/- 0.01 new_mean_mag=11.0505 delta=0.97 (need > 0.90)
Adding exclusion_list_local.txt__out12379.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 33140_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 33140_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:07:56.98 +37:48:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33169_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 33169_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:26:54.57 +36:54:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20686_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 20686_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 06:01:46.71 +41:06:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07734_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 07734_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:06:30.41 +35:23:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15871_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 15871_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:47:32.76 +39:27:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21472_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 21472_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:46:54.85 +41:24:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20505_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 20505_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:55:45.47 +41:06:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14476_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 14476_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:41:55.85 +38:56:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31076_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 31076_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:59:47.57 +35:03:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30081_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 30081_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12379_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 12379_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06908_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 06908_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:18:18.99 +35:15:00.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11579_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 11579_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:40:07.80 +37:38:11.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14940_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 14940_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:28:59.97 +39:02:52.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Aur-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:31:34.44 +37:53:11.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
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-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits exists and is non-empty
wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits exists and is non-empty
wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:16.998 +37:59:58.58 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits (1st new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
Image size: 943.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:17.780 +37:57:25.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:27:16.998 +37:59:58.58
Second-epoch image center 05:27:17.780 +37:57:25.33
Angular distance between the image centers 0.0426 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits (2nd new image)
verification OK: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
Image size: 943.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:27:17.381 +37:57:58.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:27:16.998 +37:59:58.58
Second-epoch image center 05:27:17.381 +37:57:58.42
Angular distance between the image centers 0.0334 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 05:27:17.780 +37:57:25.33
Second-epoch second image center 05:27:17.381 +37:57:58.42
Angular distance between the image centers 0.00928 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.EgsNAuCVyt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits &> /tmp/tmp.tlc6ZpE7PV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits &> /tmp/tmp.WLw0pPHsmi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits &> /tmp/tmp.iST0gSLXYo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Found non-empty wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
The reference image (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat) found
'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat' -> 'wcsmag.cat'
Read 202315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8143 to 92.1485 deg, Dec +31.9880 to +43.3918 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.8143 to 92.1485 deg, Dec 31.9880 to 43.3918 deg
Loaded 16061 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8339 out of 12799 total matches.
Matched with Tycho-2 12799 out of 202315 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.787200
a=0.000000 b=1.000000 c=22.787200
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 202315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 70.8143 to 92.1485 deg, Dec +31.9880 to +43.3918 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 70.8143 to 92.1485 deg, Dec 31.9880 to 43.3918 deg
Loaded 16061 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8339 out of 12799 total matches.
Matched with Tycho-2 12799 out of 202315 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (aperture=4.7)
Read 212259 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.3331 to 92.7203 deg, Dec +32.1392 to +43.3198 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 71.3331 to 92.7203 deg, Dec 32.1392 to 43.3198 deg
Loaded 16048 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8212 out of 12990 total matches.
Matched with Tycho-2 12990 out of 212259 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Forced-photometry filter: calibrated wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -> calib.txt_param_ref_wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 198 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
1.9 pix Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
2.9 pix fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
2.9 pix fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
Limiting magnitude estimates:
15.4 mag. Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
15.4 mag. Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
13.6 mag. fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
13.5 mag. fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.EgsNAuCVyt (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=30655, bad_region=1, passed=202260
Got 202260 stars (including 171302 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat
util/solve_plate_with_UCAC5 got 202260 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 4824 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 202260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 4876 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 202260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 202260 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4823 stars left (next iteration limit 5306)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits N_match=4823 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.468 sigma_q2_arcsec=0.351 sigma_q3_arcsec=0.350 sigma_q4_arcsec=0.308 n_q1=927 n_q2=1360 n_q3=1306 n_q4=1230 worst_quadrant_to_overall_ratio=1.304
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.tlc6ZpE7PV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat corresponding to the image wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=32150, bad_region=8, passed=212204
Got 212204 stars (including 179717 good ones) from the SExtractor catalog wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat
util/solve_plate_with_UCAC5 got 212204 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 4822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 212204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 4872 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 212204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 212204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4819 stars left (next iteration limit 5303)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits N_match=4819 sigma_overall_arcsec=0.482 sigma_q1_arcsec=0.573 sigma_q2_arcsec=0.484 sigma_q3_arcsec=0.442 sigma_q4_arcsec=0.412 n_q1=1096 n_q2=1410 n_q3=1324 n_q4=989 worst_quadrant_to_overall_ratio=1.189
The image catalog is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits -region wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.WLw0pPHsmi (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_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.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_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2735, bad_region=7, passed=53233
Got 53233 stars (including 50439 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat
util/solve_plate_with_UCAC5 got 53233 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.2'
Seting catalog search parameters based on the expected field of view 943.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013100 (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 0.010480 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.3)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 4821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 53216 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.3)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 53216 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 53216 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4819 stars left (next iteration limit 5302)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4819 robust_rms=5.907 arcsec worst_quadrant_rms=6.391 arcsec
SIP_REFIT: SIP order 3 trial: matched=4819 robust_rms=0.502 arcsec worst_quadrant_rms=0.656 arcsec
SIP_REFIT: SIP order 5 trial: matched=4819 robust_rms=0.420 arcsec worst_quadrant_rms=0.536 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4819 robust_rms_before=1.024 arcsec robust_rms_before_corrected=0.444 arcsec robust_rms_after=0.420 arcsec worst_quadrant_rms_before=0.557 worst_quadrant_rms_after=0.536
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.557 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits N_match=4819 sigma_overall_arcsec=0.447 sigma_q1_arcsec=0.447 sigma_q2_arcsec=0.518 sigma_q3_arcsec=0.385 sigma_q4_arcsec=0.423 n_q1=1349 n_q2=1180 n_q3=1040 n_q4=1250 worst_quadrant_to_overall_ratio=1.160
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits -region wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.iST0gSLXYo (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_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.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_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
Checking if the catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat corresponding to the image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
WCS catalog name: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=2741, bad_region=12, passed=53393
Got 53393 stars (including 50584 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat
util/solve_plate_with_UCAC5 got 53393 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.2'
Seting catalog search parameters based on the expected field of view 943.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013100 (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 0.010480 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 4818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4817 matched stars entering correct_measured_positions(), 53387 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.3)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 53387 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 53387 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 4815 stars left (next iteration limit 5298)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4815 robust_rms=5.670 arcsec worst_quadrant_rms=6.277 arcsec
SIP_REFIT: SIP order 3 trial: matched=4815 robust_rms=0.498 arcsec worst_quadrant_rms=0.634 arcsec
SIP_REFIT: SIP order 5 trial: matched=4815 robust_rms=0.418 arcsec worst_quadrant_rms=0.519 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4815 robust_rms_before=1.011 arcsec robust_rms_before_corrected=0.454 arcsec robust_rms_after=0.418 arcsec worst_quadrant_rms_before=0.513 worst_quadrant_rms_after=0.519
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.513 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits N_match=4815 sigma_overall_arcsec=0.453 sigma_q1_arcsec=0.450 sigma_q2_arcsec=0.520 sigma_q3_arcsec=0.382 sigma_q4_arcsec=0.432 n_q1=1358 n_q2=1188 n_q3=1017 n_q4=1252 worst_quadrant_to_overall_ratio=1.147
The image catalog is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits -region wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.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_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-06-22_20.00sec_0.00C_LIGHTs_0173.fits
Saving fully-calibrated image wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.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_2026-09-06_CI_Aur-03-Q1b1x1_020800_TTUQ1b1x1_2565468_AnNMbhNI/wcs_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174.fits
Preparing the HTML report for the field Aur-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:22:55.52 +39:26:07.9: 11.76 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:42:17.21 +40:03:40.7: 13.34 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:37:52.24 +42:14:44.6: 12.55 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:34:08.43 +39:56:55.9: 12.42 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:42:17.21 +40:03:40.7: 13.33 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:22:55.52 +39:26:07.9: 11.76 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:34:08.43 +39:56:55.9: 12.47 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.02
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:37:52.24 +42:14:44.6: 12.65 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 05:42:17.21 +40:03:40.7: ref_mag=13.33 +/- 0.02 new_mean_mag=12.9185 delta=0.42 (need > 0.90)
Forced photometry reference-image weighted average: 11.76 +/- 0.01
Forced photometry filter REJECTED candidate at 05:22:55.52 +39:26:07.9: ref_mag=11.76 +/- 0.01 new_mean_mag=11.5889 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 05:37:52.24 +42:14:44.6: ref_mag=12.60 +/- 0.01 new_mean_mag=12.3704 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:34:08.43 +39:56:55.9: ref_mag=12.45 +/- 0.01 new_mean_mag=12.3737 delta=0.07 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:09:58.01 +36:14:44.0: 15.64 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:14:49.44 +39:31:03.4: 12.66 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:09:58.01 +36:14:44.0: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:22:18.94 +36:11:54.9: 13.15 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:14:49.44 +39:31:03.4: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.69 +/- 0.02
Forced photometry filter REJECTED candidate at 05:14:49.44 +39:31:03.4: ref_mag=12.69 +/- 0.02 new_mean_mag=12.2456 delta=0.45 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:00:38.47 +36:37:54.8: 13.30 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:45:51.11 +37:37:55.8: 12.68 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:19:22.87 +40:08:56.3: 13.09 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:22:18.94 +36:11:54.9: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter REJECTED candidate at 05:22:18.94 +36:11:54.9: ref_mag=13.14 +/- 0.02 new_mean_mag=12.6661 delta=0.47 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:30:14.73 +40:29:51.7: 12.86 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:45:51.11 +37:37:55.8: 12.65 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:00:38.47 +36:37:54.8: 13.30 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:19:22.87 +40:08:56.3: 13.08 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry reference-image weighted average: 13.30 +/- 0.03
Forced photometry filter REJECTED candidate at 05:45:51.11 +37:37:55.8: ref_mag=12.66 +/- 0.01 new_mean_mag=12.3703 delta=0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:00:38.47 +36:37:54.8: ref_mag=13.30 +/- 0.03 new_mean_mag=12.9122 delta=0.39 (need > 0.90)
Forced photometry reference-image weighted average: 13.09 +/- 0.03
Forced photometry filter REJECTED candidate at 05:19:22.87 +40:08:56.3: ref_mag=13.09 +/- 0.03 new_mean_mag=12.8182 delta=0.27 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:49:37.96 +38:41:13.6: 12.89 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:08:09.80 +36:07:12.7: 13.56 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:30:14.73 +40:29:51.7: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter REJECTED candidate at 05:30:14.73 +40:29:51.7: ref_mag=12.90 +/- 0.02 new_mean_mag=12.6403 delta=0.26 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:49:37.96 +38:41:13.6: 12.98 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:08:09.80 +36:07:12.7: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter REJECTED candidate at 05:49:37.96 +38:41:13.6: ref_mag=12.93 +/- 0.02 new_mean_mag=12.5919 delta=0.34 (need > 0.90)
Forced photometry reference-image weighted average: 13.51 +/- 0.03
Forced photometry filter REJECTED candidate at 05:08:09.80 +36:07:12.7: ref_mag=13.51 +/- 0.03 new_mean_mag=13.0747 delta=0.44 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:01:24.24 +37:13:28.8: 13.73 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:52:31.12 +40:09:39.1: 13.08 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:52:31.12 +40:09:39.1: 13.01 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:01:24.24 +37:13:28.8: 13.64 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry reference-image weighted average: 13.68 +/- 0.04
Forced photometry filter REJECTED candidate at 05:01:24.24 +37:13:28.8: ref_mag=13.68 +/- 0.04 new_mean_mag=13.1312 delta=0.55 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:52:31.12 +40:09:39.1: ref_mag=13.04 +/- 0.02 new_mean_mag=12.6399 delta=0.40 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:10:28.62 +37:19:33.4: 13.55 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:10:28.62 +37:19:33.4: 13.50 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.03
Forced photometry filter REJECTED candidate at 05:10:28.62 +37:19:33.4: ref_mag=13.52 +/- 0.03 new_mean_mag=13.2957 delta=0.23 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:25:50.95 +39:25:03.8: 13.89 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:24:17.43 +37:16:09.8: 13.92 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:24:57.90 +35:54:44.5: 13.96 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:35:27.86 +37:11:40.0: 14.06 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:25:50.95 +39:25:03.8: 13.92 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Forced photometry filter KEPT candidate at 05:25:50.95 +39:25:03.8: ref_mag=13.91 +/- 0.03 new_mean_mag=12.9147 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:24:17.43 +37:16:09.8: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Forced photometry filter KEPT candidate at 05:24:17.43 +37:16:09.8: ref_mag=13.88 +/- 0.04 new_mean_mag=12.9777 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:05:49.67 +36:22:10.9: 14.07 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:24:57.90 +35:54:44.5: 13.93 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:35:27.86 +37:11:40.0: 13.88 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.03
Forced photometry filter REJECTED candidate at 05:24:57.90 +35:54:44.5: ref_mag=13.95 +/- 0.03 new_mean_mag=13.0740 delta=0.87 (need > 0.90)
Forced photometry reference-image weighted average: 13.95 +/- 0.03
Forced photometry filter KEPT candidate at 05:35:27.86 +37:11:40.0: ref_mag=13.95 +/- 0.03 new_mean_mag=12.8915 delta=1.06 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:05:49.67 +36:22:10.9: 14.04 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.04
Forced photometry filter KEPT candidate at 05:05:49.67 +36:22:10.9: ref_mag=14.06 +/- 0.04 new_mean_mag=13.0913 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:22:17.16 +36:57:51.8: 12.76 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:22:17.16 +36:57:51.8: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter KEPT candidate at 05:22:17.16 +36:57:51.8: ref_mag=12.73 +/- 0.01 new_mean_mag=11.8055 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:31:34.75 +37:21:56.9: 13.19 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:29:04.39 +38:16:12.1: 13.34 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:22:50.86 +37:36:37.8: 13.39 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:31:34.75 +37:21:56.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter KEPT candidate at 05:31:34.75 +37:21:56.9: ref_mag=13.20 +/- 0.02 new_mean_mag=12.0841 delta=1.12 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:29:04.39 +38:16:12.1: 13.42 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry filter KEPT candidate at 05:29:04.39 +38:16:12.1: ref_mag=13.38 +/- 0.02 new_mean_mag=12.3975 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:22:50.86 +37:36:37.8: 13.40 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.40 +/- 0.02
Forced photometry filter KEPT candidate at 05:22:50.86 +37:36:37.8: ref_mag=13.40 +/- 0.02 new_mean_mag=12.4935 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:21:39.05 +37:47:05.9: 13.67 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:21:39.05 +37:47:05.9: 13.63 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.02
Forced photometry filter KEPT candidate at 05:21:39.05 +37:47:05.9: ref_mag=13.65 +/- 0.02 new_mean_mag=12.6992 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:31:51.67 +37:21:15.4: 13.65 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:28:49.95 +38:06:50.8: 13.71 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:31:51.67 +37:21:15.4: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.68 +/- 0.03
Forced photometry filter KEPT candidate at 05:31:51.67 +37:21:15.4: ref_mag=13.68 +/- 0.03 new_mean_mag=12.7678 delta=0.91 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:28:49.95 +38:06:50.8: 13.75 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter REJECTED candidate at 05:28:49.95 +38:06:50.8: ref_mag=13.73 +/- 0.03 new_mean_mag=12.8498 delta=0.88 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:36:05.09 +38:07:01.9: 13.81 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:47:17.05 +39:17:22.3: 13.54 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:36:05.09 +38:07:01.9: 13.82 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:47:17.05 +39:17:22.3: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry reference-image weighted average: 13.55 +/- 0.03
Forced photometry filter KEPT candidate at 05:36:05.09 +38:07:01.9: ref_mag=13.81 +/- 0.03 new_mean_mag=12.8431 delta=0.97 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:47:17.05 +39:17:22.3: ref_mag=13.55 +/- 0.03 new_mean_mag=12.8230 delta=0.72 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:27:11.45 +40:00:30.5: 13.32 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:27:11.45 +40:00:30.5: 13.36 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.34 +/- 0.02
Forced photometry filter REJECTED candidate at 05:27:11.45 +40:00:30.5: ref_mag=13.34 +/- 0.02 new_mean_mag=12.8379 delta=0.50 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:45:26.24 +38:32:10.8: 13.72 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:45:26.24 +38:32:10.8: 13.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter KEPT candidate at 05:45:26.24 +38:32:10.8: ref_mag=13.75 +/- 0.03 new_mean_mag=12.6797 delta=1.07 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:27:07.60 +37:21:25.1: 13.71 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:27:07.60 +37:21:25.1: 13.86 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.78 +/- 0.03
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:47:51.28 +38:34:38.8: 13.68 +/- 0.04 detection
Forced photometry filter KEPT candidate at 05:27:07.60 +37:21:25.1: ref_mag=13.78 +/- 0.03 new_mean_mag=12.8022 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:17:13.30 +35:18:57.7: 13.61 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:47:51.28 +38:34:38.8: 13.64 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter KEPT candidate at 05:47:51.28 +38:34:38.8: ref_mag=13.66 +/- 0.03 new_mean_mag=12.6417 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:17:13.30 +35:18:57.7: 13.60 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Forced photometry filter KEPT candidate at 05:17:13.30 +35:18:57.7: ref_mag=13.61 +/- 0.03 new_mean_mag=12.6037 delta=1.01 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:23:09.47 +37:30:30.7: 13.55 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:23:09.47 +37:30:30.7: 13.62 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.02
Forced photometry filter KEPT candidate at 05:23:09.47 +37:30:30.7: ref_mag=13.58 +/- 0.02 new_mean_mag=12.6588 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:36:14.11 +37:56:39.8: 13.54 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:36:14.11 +37:56:39.8: 13.71 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.03
Forced photometry filter KEPT candidate at 05:36:14.11 +37:56:39.8: ref_mag=13.61 +/- 0.03 new_mean_mag=12.6119 delta=1.00 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:56:35.81 +35:11:01.6: 14.56 +/- 0.10 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:56:35.81 +35:11:01.6: 14.40 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.06
Forced photometry filter KEPT candidate at 04:56:35.81 +35:11:01.6: ref_mag=14.47 +/- 0.06 new_mean_mag=13.3209 delta=1.15 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:26.13 +38:08:02.6: 13.45 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:26.13 +38:08:02.6: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter KEPT candidate at 05:20:26.13 +38:08:02.6: ref_mag=13.50 +/- 0.03 new_mean_mag=12.5240 delta=0.98 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 04:55:24.49 +35:22:43.0: 13.45 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:17:21.65 +38:51:05.6: 13.10 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:32:09.90 +37:20:04.0: 13.43 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 04:55:24.49 +35:22:43.0: 13.27 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter REJECTED candidate at 04:55:24.49 +35:22:43.0: ref_mag=13.35 +/- 0.03 new_mean_mag=12.4550 delta=0.89 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:32:09.90 +37:20:04.0: 13.46 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:17:21.65 +38:51:05.6: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter KEPT candidate at 05:32:09.90 +37:20:04.0: ref_mag=13.45 +/- 0.02 new_mean_mag=12.4636 delta=0.98 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:17:21.65 +38:51:05.6: ref_mag=13.11 +/- 0.02 new_mean_mag=12.4743 delta=0.63 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:25:57.63 +38:42:34.0: 13.07 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:25:57.63 +38:42:34.0: 13.13 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter REJECTED candidate at 05:25:57.63 +38:42:34.0: ref_mag=13.10 +/- 0.02 new_mean_mag=12.5205 delta=0.58 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:37:26.67 +39:42:58.1: 13.06 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:28.20 +39:26:18.2: 13.33 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:37:26.67 +39:42:58.1: 13.16 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry filter REJECTED candidate at 05:37:26.67 +39:42:58.1: ref_mag=13.11 +/- 0.02 new_mean_mag=12.3326 delta=0.78 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:28.20 +39:26:18.2: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 05:20:28.20 +39:26:18.2: ref_mag=13.30 +/- 0.02 new_mean_mag=12.3258 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:40:16.66 +38:35:46.9: 13.22 +/- 0.03 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:40:16.66 +38:35:46.9: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 05:40:16.66 +38:35:46.9: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2014 delta=1.02 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:20:46.20 +36:06:46.5: 13.00 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:24:00.67 +37:05:19.0: 12.99 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:20:46.20 +36:06:46.5: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 05:20:46.20 +36:06:46.5: ref_mag=13.03 +/- 0.02 new_mean_mag=12.1066 delta=0.93 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:24:00.67 +37:05:19.0: 13.06 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 05:24:00.67 +37:05:19.0: ref_mag=13.02 +/- 0.02 new_mean_mag=12.0349 delta=0.99 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:32:41.29 +38:27:36.4: 14.36 +/- 0.07 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:37:15.19 +39:47:47.7: 12.98 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:19:54.15 +36:28:35.7: 14.17 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:32:41.29 +38:27:36.4: 14.39 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.05
Forced photometry filter KEPT candidate at 05:32:41.29 +38:27:36.4: ref_mag=14.37 +/- 0.05 new_mean_mag=13.1841 delta=1.19 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:22:53.06 +36:24:23.8: 12.64 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:37:15.19 +39:47:47.7: 13.00 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:19:54.15 +36:28:35.7: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 05:37:15.19 +39:47:47.7: ref_mag=12.99 +/- 0.02 new_mean_mag=12.0398 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 14.17 +/- 0.04
Forced photometry filter KEPT candidate at 05:19:54.15 +36:28:35.7: ref_mag=14.17 +/- 0.04 new_mean_mag=13.2484 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:22:53.06 +36:24:23.8: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter REJECTED candidate at 05:22:53.06 +36:24:23.8: ref_mag=12.65 +/- 0.01 new_mean_mag=12.0960 delta=0.56 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:27:42.97 +38:15:22.3: 12.78 +/- 0.02 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:27:42.97 +38:15:22.3: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter KEPT candidate at 05:27:42.97 +38:15:22.3: ref_mag=12.90 +/- 0.01 new_mean_mag=11.9527 delta=0.95 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:31:53.33 +37:35:55.4: 14.24 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:21:25.37 +37:42:32.9: 14.23 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:31:53.33 +37:35:55.4: 14.28 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.26 +/- 0.04
Forced photometry filter KEPT candidate at 05:31:53.33 +37:35:55.4: ref_mag=14.26 +/- 0.04 new_mean_mag=13.1515 delta=1.11 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:21:25.37 +37:42:32.9: 14.06 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.04
Forced photometry filter KEPT candidate at 05:21:25.37 +37:42:32.9: ref_mag=14.13 +/- 0.04 new_mean_mag=13.1655 delta=0.97 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:28:13.34 +41:11:29.1: 11.81 +/- 0.01 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:28:13.34 +41:11:29.1: 11.88 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.84 +/- 0.01
Forced photometry filter REJECTED candidate at 05:28:13.34 +41:11:29.1: ref_mag=11.84 +/- 0.01 new_mean_mag=11.2757 delta=0.57 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:25:40.54 +38:52:38.0: 14.05 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:25:40.54 +38:52:38.0: 14.16 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Forced photometry filter KEPT candidate at 05:25:40.54 +38:52:38.0: ref_mag=14.10 +/- 0.04 new_mean_mag=13.0536 delta=1.05 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:01:27.55 +33:10:54.4: 14.01 +/- 0.06 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:38:07.86 +36:52:05.5: 13.98 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:01:27.55 +33:10:54.4: 13.68 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.04
Forced photometry filter KEPT candidate at 05:01:27.55 +33:10:54.4: ref_mag=13.81 +/- 0.04 new_mean_mag=12.9046 delta=0.90 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:43:39.54 +39:56:46.3: 13.44 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:38:07.86 +36:52:05.5: 14.02 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.00 +/- 0.04
Forced photometry filter KEPT candidate at 05:38:07.86 +36:52:05.5: ref_mag=14.00 +/- 0.04 new_mean_mag=12.9134 delta=1.08 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:43:39.54 +39:56:46.3: 13.41 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter REJECTED candidate at 05:43:39.54 +39:56:46.3: ref_mag=13.43 +/- 0.02 new_mean_mag=12.6859 delta=0.74 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:19:10.25 +36:44:18.5: 13.70 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:30:38.78 +37:43:02.9: 13.57 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:19:10.25 +36:44:18.5: 13.82 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.03
Forced photometry filter REJECTED candidate at 05:19:10.25 +36:44:18.5: ref_mag=13.75 +/- 0.03 new_mean_mag=12.9801 delta=0.77 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:30:38.78 +37:43:02.9: 13.68 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter KEPT candidate at 05:30:38.78 +37:43:02.9: ref_mag=13.62 +/- 0.03 new_mean_mag=12.7039 delta=0.92 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:19:51.17 +35:43:51.4: 13.47 +/- 0.04 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:19:51.17 +35:43:51.4: 13.46 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry filter REJECTED candidate at 05:19:51.17 +35:43:51.4: ref_mag=13.47 +/- 0.03 new_mean_mag=12.9940 delta=0.48 (need > 0.90)
Forced photometry on wcs_Aur-03-Q1b1x1_2026-01-17_20-41-07_20.00sec_-15.00C_LIGHT_0049.fits at 05:18:46.64 +39:20:46.1: 13.91 +/- 0.05 detection
Forced photometry on wcs_Aur-03-Q1b1x1_2026-02-21_20-50-53_20.00sec_-15.00C_LIGHT_0054.fits at 05:18:46.64 +39:20:46.1: 13.85 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Forced photometry filter KEPT candidate at 05:18:46.64 +39:20:46.1: ref_mag=13.88 +/- 0.04 new_mean_mag=12.9416 delta=0.94 (need > 0.90)
Adding exclusion_list_local.txt__out100147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89198.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99384.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 31s
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: 19s
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Considering the candidate 245221_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245221_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 245230_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245230_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:18:44.02 +41:49:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245235_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245235_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:28:10.80 +39:10:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245250_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245250_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:17:06.13 +39:11:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245251_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245251_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 245254_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245254_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 245255_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245255_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:17:57.97 +35:10:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245256_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245256_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:36:28.41 +34:07:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245257_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245257_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:17:19.77 +39:28:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245261_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245261_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 245323_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245323_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:19:15.63 +40:07:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245328_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245328_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:24:43.04 +37:25:06.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245337_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245337_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:56:57.87 +33:05:59.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 245366_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245366_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:50:57.81 +37:20:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245401_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245401_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:24:47.31 +37:21:50.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245407_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245407_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:13:19.94 +38:30:50.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245413_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245413_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:49:06.74 +39:13:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245419_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245419_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:10:27.42 +37:19:04.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245440_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245440_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:06:25.52 +34:49:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245486_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245486_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:24:49.89 +37:22:48.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245503_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 245503_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 245505_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245505_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:19:01.59 +41:06:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245524_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245524_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:52:57.70 +42:34:50.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245526_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245526_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 245534_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245534_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:56:07.83 +35:10:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245535_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245535_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:30:54.21 +39:49:17.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245557_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245557_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:20:06.12 +39:18:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245559_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245559_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:06:33.99 +35:29:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245562_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245562_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:45:47.07 +40:29:14.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245565_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245565_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 06:01:11.70 +41:56:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245581_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245581_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:29:49.40 +35:22:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245587_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245587_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:50:52.24 +37:18:45.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245597_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245597_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245599_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245599_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:26:40.73 +34:23:15.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245621_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245621_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:20:49.31 +37:27:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245622_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245622_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:39:56.38 +37:58:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245628_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245628_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:24:38.54 +39:45:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245631_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245631_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:18:56.59 +41:04:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245633_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245633_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245647_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245647_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245652_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245652_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:59:46.12 +38:13:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245670_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245670_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245671_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245671_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:06:28.75 +35:34:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245680_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245680_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:44:55.94 +38:31:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245681_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245681_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:41:00.67 +39:37:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245690_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245690_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245691_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245691_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:15:04.69 +35:21:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245692_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245692_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245697_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245697_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:25:44.40 +38:02:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245704_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245704_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245707_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245707_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:18:32.17 +40:27:40.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245708_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245708_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:54:12.21 +35:47:04.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245720_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245720_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:20:43.60 +37:24:53.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245730_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245730_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 245755_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245755_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:18:58.79 +35:53:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245757_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245757_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:18:40.11 +39:21:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245761_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245761_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 245765_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245765_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:35:43.60 +38:03:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245775_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245775_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:18:44.81 +36:47:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245787_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245787_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:14:44.98 +39:31:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245791_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245791_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:08:43.60 +37:38:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245817_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245817_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:19:27.59 +34:00:23.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245818_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245818_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:51:41.85 +42:03:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245819_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245819_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 245828_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245828_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:32:23.72 +40:57:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245834_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 245834_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:19:17.30 +39:33:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79639_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 79639_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:59:43.11 +37:12:41.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 113198_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 113198_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:28:59.96 +39:02:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119084_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 119084_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 79215_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 79215_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 55832_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 55832_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 75744_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 75744_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 117999_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 117999_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:47:32.76 +39:27:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68876_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 68876_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 29050_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 29050_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:38:03.88 +34:25:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73667_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 73667_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:03:20.33 +36:34:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103006_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 103006_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:21:01.16 +38:28:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79222_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 79222_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:31:11.35 +37:20:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159818_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 159818_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
Rejecting candidate due to large distance (32.9") between the two second-epoch detections
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Considering the candidate 69235_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 69235_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:21:28.46 +36:40:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74231_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 74231_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 112577_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 112577_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:43:21.35 +39:12:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110147_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 110147_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:30:18.69 +38:59:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143808_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 143808_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:20:58.15 +40:30:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44756_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 44756_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:26:35.49 +35:15:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79537_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 79537_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 96341_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 96341_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 85853_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 85853_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 103231_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 103231_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:19:46.04 +38:30:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46614_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 46614_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:16:59.41 +35:14:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102689_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 102689_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:32:02.42 +38:38:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89198_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 89198_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 79204_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 79204_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 93498_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 93498_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 87684_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 87684_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:20:05.63 +37:40:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50001_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 50001_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:25:27.32 +35:35:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33314_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 33314_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:24:12.50 +34:32:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50292_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 50292_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:25:29.57 +35:35:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113884_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 113884_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 42031_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 42031_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:02:26.35 +34:39:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92347_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 92347_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 239975_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 239975_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
Rejecting candidate due to large distance (33.1") between the two second-epoch detections
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Considering the candidate 130823_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 130823_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 54418_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 54418_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:52:52.70 +35:09:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99384_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 99384_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 33421_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 33421_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 06:02:50.24 +34:41:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80265_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 80265_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 100147_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 100147_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 47784_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 47784_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 60353_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 60353_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:38:25.59 +36:19:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39993_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 39993_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:36:12.61 +35:03:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114580_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 114580_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:37:14.74 +39:16:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93298_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 93298_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:32:58.98 +38:08:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83880_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 83880_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 82064_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 82064_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:22:09.36 +37:23:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80809_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 80809_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:44:20.73 +37:30:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89224_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 89224_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 133126_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 133126_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:24:55.82 +40:04:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42169_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 42169_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:00:49.71 +34:37:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224060_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 224060_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:09:08.30 +37:40:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52956_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 52956_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 95920_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 95920_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 134014_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 134014_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
Rejecting candidate due to large distance (33.4") between the two second-epoch detections
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Considering the candidate 222900_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 222900_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:49:33.31 +34:07:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56972_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 56972_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 78812_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 78812_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 110527_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 110527_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 81296_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 81296_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:30:27.05 +37:27:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86440_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 86440_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:30:32.75 +37:44:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115354_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 115354_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:30:24.00 +39:15:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105370_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 105370_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 111451_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 111451_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:51:12.96 +39:09:35.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 102240_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 102240_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:45:01.88 +38:39:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61328_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 61328_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:52:11.77 +36:24:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55055_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 55055_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:30:54.96 +35:56:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70444_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 70444_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:30:56.43 +36:52:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121142_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 121142_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 217102_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 217102_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:55:45.51 +41:06:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217034_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 217034_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 117810_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 117810_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:21:01.83 +39:16:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123486_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 123486_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:36:37.56 +39:42:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32333_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 32333_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:59:52.76 +33:59:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101056_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 101056_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 30548_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 30548_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:28:49.13 +34:25:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39924_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 39924_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:17:30.61 +34:49:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108410_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 108410_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:40:58.86 +38:58:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60069_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 60069_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 95220_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 95220_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:07:56.99 +37:48:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72927_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 72927_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:26:54.58 +36:54:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49989_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 49989_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:59:47.60 +35:03:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76164_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 76164_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 99069_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 99069_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 124971_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 124971_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 65978_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 65978_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 64088_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 64088_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 89057_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 89057_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:42:57.53 +37:58:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97836_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 97836_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:24:59.92 +38:16:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96604_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 96604_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 194777_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 194777_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:41:19.88 +41:19:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104499_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 104499_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:20:36.58 +38:35:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197929_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 197929_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 06:01:46.76 +41:06:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83607_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 83607_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 46899_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 46899_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:18:18.98 +35:14:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76522_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 76522_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:17:46.85 +36:59:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87833_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 87833_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
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Considering the candidate 53361_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 53361_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:06:30.42 +35:23:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49281_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 49281_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:38:22.12 +35:37:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41258_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 41258_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:18:57.01 +34:57:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192838_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 192838_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:46:54.84 +41:24:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195314_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 195314_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
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Considering the candidate 152185_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 152185_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
Rejecting candidate due to large distance (33.4") between the two second-epoch detections
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Considering the candidate 89575_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 89575_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:31:34.42 +37:53:11.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 85254_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 85254_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:40:07.73 +37:38:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86818_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 86818_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:08:17.28 +37:24:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108684_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 108684_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92668_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 92668_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:20:07.47 +37:57:30.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56197_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 56197_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:25:08.45 +35:56:59.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111430_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 111430_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:41:55.85 +38:56:00.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44233_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 44233_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:20:55.58 +35:05:22.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127526_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 127526_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:49:41.85 +39:54:39.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17125_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 17125_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69851_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 69851_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:24:50.89 +36:46:09.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69401_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 69401_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127290_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 127290_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55043_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 55043_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:20:58.50 +35:48:41.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126082_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 126082_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:34:41.75 +39:50:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70949_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 70949_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49874_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 49874_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:26:53.90 +35:34:48.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85907_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 85907_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85851_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 85851_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:33:34.40 +37:43:24.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53845_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 53845_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85632_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 85632_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:33:03.17 +37:43:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67315_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 67315_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:27:17.85 +36:39:06.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96748_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 96748_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:20:45.10 +38:10:49.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86283_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 86283_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:35:11.11 +37:45:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40767_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 40767_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 04:54:11.84 +34:22:00.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119633_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
Preparing report for the candidate 119633_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 114368_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174
The candidate 114368_fd_Aur-03-Q1b1x1_2026-09-06_02-07-12_20.00sec_-0.00C_LIGHTs_0174 did not pass the final checks
**** FOUND 05:51:29.01 +39:08:51.3 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 53s
Prepared the HTML report for the field Aur-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:31:34.44 +37:53:11.4
05:47:51.28 +38:34:38.8
05:40:16.66 +38:35:46.9
05:25:40.54 +38:52:38.0
05:25:50.95 +39:25:03.8
05:18:46.64 +39:20:46.1
05:20:28.20 +39:26:18.2
05:37:15.19 +39:47:47.7
05:01:27.55 +33:10:54.4
05:09:58.01 +36:14:44.0
05:17:13.30 +35:18:57.7
04:56:35.81 +35:11:01.6
05:20:46.20 +36:06:46.5
05:19:54.15 +36:28:35.7
05:05:49.67 +36:22:10.9
05:38:07.86 +36:52:05.5
05:22:17.16 +36:57:51.8
05:35:27.86 +37:11:40.0
05:24:00.67 +37:05:19.0
05:32:09.90 +37:20:04.0
05:31:51.67 +37:21:15.4
05:24:17.43 +37:16:09.8
05:31:34.75 +37:21:56.9
05:27:07.60 +37:21:25.1
05:31:53.33 +37:35:55.4
05:23:09.47 +37:30:30.7
05:22:50.86 +37:36:37.8
05:30:38.78 +37:43:02.9
05:21:25.37 +37:42:32.9
05:21:39.05 +37:47:05.9
05:36:14.11 +37:56:39.8
05:36:05.09 +38:07:01.9
05:20:26.13 +38:08:02.6
05:29:04.39 +38:16:12.1
05:27:42.97 +38:15:22.3
05:32:41.29 +38:27:36.4
05:45:26.24 +38:32:10.8
########### Completed Aur-03-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:31:34.44 +37:53:11.4
05:09:58.01 +36:14:44.0
05:25:50.95 +39:25:03.8
05:24:17.43 +37:16:09.8
05:35:27.86 +37:11:40.0
05:05:49.67 +36:22:10.9
05:22:17.16 +36:57:51.8
05:31:34.75 +37:21:56.9
05:29:04.39 +38:16:12.1
05:22:50.86 +37:36:37.8
05:21:39.05 +37:47:05.9
05:31:51.67 +37:21:15.4
05:36:05.09 +38:07:01.9
05:45:26.24 +38:32:10.8
05:27:07.60 +37:21:25.1
05:47:51.28 +38:34:38.8
05:17:13.30 +35:18:57.7
05:23:09.47 +37:30:30.7
05:36:14.11 +37:56:39.8
04:56:35.81 +35:11:01.6
05:20:26.13 +38:08:02.6
05:32:09.90 +37:20:04.0
05:20:28.20 +39:26:18.2
05:40:16.66 +38:35:46.9
05:20:46.20 +36:06:46.5
05:24:00.67 +37:05:19.0
05:32:41.29 +38:27:36.4
05:37:15.19 +39:47:47.7
05:19:54.15 +36:28:35.7
05:27:42.97 +38:15:22.3
05:31:53.33 +37:35:55.4
05:21:25.37 +37:42:32.9
05:25:40.54 +38:52:38.0
05:01:27.55 +33:10:54.4
05:38:07.86 +36:52:05.5
05:30:38.78 +37:43:02.9
05:18:46.64 +39:20:46.1
###################################################################################
05:31:34.44 +37:53:11.4 -- not an asteroid (will add it to exclusion list)
05:09:58.01 +36:14:44.0 -- asteroid (will NOT add it to exclusion list)
05:25:50.95 +39:25:03.8 -- not an asteroid (will add it to exclusion list)
05:24:17.43 +37:16:09.8 -- not an asteroid (will add it to exclusion list)
05:35:27.86 +37:11:40.0 -- not an asteroid (will add it to exclusion list)
05:05:49.67 +36:22:10.9 -- not an asteroid (will add it to exclusion list)
05:22:17.16 +36:57:51.8 -- not an asteroid (will add it to exclusion list)
05:31:34.75 +37:21:56.9 -- not an asteroid (will add it to exclusion list)
05:29:04.39 +38:16:12.1 -- not an asteroid (will add it to exclusion list)
05:22:50.86 +37:36:37.8 -- not an asteroid (will add it to exclusion list)
05:21:39.05 +37:47:05.9 -- not an asteroid (will add it to exclusion list)
05:31:51.67 +37:21:15.4 -- not an asteroid (will add it to exclusion list)
05:36:05.09 +38:07:01.9 -- not an asteroid (will add it to exclusion list)
05:45:26.24 +38:32:10.8 -- not an asteroid (will add it to exclusion list)
05:27:07.60 +37:21:25.1 -- not an asteroid (will add it to exclusion list)
05:47:51.28 +38:34:38.8 -- not an asteroid (will add it to exclusion list)
05:17:13.30 +35:18:57.7 -- not an asteroid (will add it to exclusion list)
05:23:09.47 +37:30:30.7 -- not an asteroid (will add it to exclusion list)
05:36:14.11 +37:56:39.8 -- not an asteroid (will add it to exclusion list)
04:56:35.81 +35:11:01.6 -- not an asteroid (will add it to exclusion list)
05:20:26.13 +38:08:02.6 -- not an asteroid (will add it to exclusion list)
05:32:09.90 +37:20:04.0 -- not an asteroid (will add it to exclusion list)
05:20:28.20 +39:26:18.2 -- not an asteroid (will add it to exclusion list)
05:40:16.66 +38:35:46.9 -- not an asteroid (will add it to exclusion list)
05:20:46.20 +36:06:46.5 -- not an asteroid (will add it to exclusion list)
05:24:00.67 +37:05:19.0 -- not an asteroid (will add it to exclusion list)
05:32:41.29 +38:27:36.4 -- not an asteroid (will add it to exclusion list)
05:37:15.19 +39:47:47.7 -- not an asteroid (will add it to exclusion list)
05:19:54.15 +36:28:35.7 -- not an asteroid (will add it to exclusion list)
05:27:42.97 +38:15:22.3 -- not an asteroid (will add it to exclusion list)
05:31:53.33 +37:35:55.4 -- not an asteroid (will add it to exclusion list)
05:21:25.37 +37:42:32.9 -- not an asteroid (will add it to exclusion list)
05:25:40.54 +38:52:38.0 -- not an asteroid (will add it to exclusion list)
05:01:27.55 +33:10:54.4 -- not an asteroid (will add it to exclusion list)
05:38:07.86 +36:52:05.5 -- not an asteroid (will add it to exclusion list)
05:30:38.78 +37:43:02.9 -- not an asteroid (will add it to exclusion list)
05:18:46.64 +39:20:46.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:56:35.81 +35:11:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:27.55 +33:10:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:49.67 +36:22:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:13.30 +35:18:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:46.64 +39:20:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:54.15 +36:28:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:26.13 +38:08:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:28.20 +39:26:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:46.20 +36:06:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:25.37 +37:42:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:39.05 +37:47:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:17.16 +36:57:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:50.86 +37:36:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:09.47 +37:30:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:00.67 +37:05:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:17.43 +37:16:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:40.54 +38:52:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:50.95 +39:25:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:07.60 +37:21:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:42.97 +38:15:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:04.39 +38:16:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:38.78 +37:43:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:34.44 +37:53:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:34.75 +37:21:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:51.67 +37:21:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:53.33 +37:35:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:09.90 +37:20:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:41.29 +38:27:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:27.86 +37:11:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:05.09 +38:07:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:14.11 +37:56:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:15.19 +39:47:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:07.86 +36:52:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:16.66 +38:35:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:26.24 +38:32:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:51.28 +38:34:38.8 -- 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)
04:56:35.81 +35:11:01.6 -- a known variable star
05:01:27.55 +33:10:54.4 -- a known variable star
05:05:49.67 +36:22:10.9 -- a known variable star
05:17:13.30 +35:18:57.7 -- a known variable star
05:18:46.64 +39:20:46.1 -- a known variable star
05:19:54.15 +36:28:35.7 -- not a known variable star
05:20:26.13 +38:08:02.6 -- not a known variable star
05:20:28.20 +39:26:18.2 -- a known variable star
05:20:46.20 +36:06:46.5 -- a known variable star
05:21:25.37 +37:42:32.9 -- not a known variable star
05:21:39.05 +37:47:05.9 -- a known variable star
05:22:17.16 +36:57:51.8 -- not a known variable star
05:22:50.86 +37:36:37.8 -- not a known variable star
05:23:09.47 +37:30:30.7 -- not a known variable star
05:24:00.67 +37:05:19.0 -- a known variable star
05:24:17.43 +37:16:09.8 -- not a known variable star
05:25:40.54 +38:52:38.0 -- not a known variable star
05:25:50.95 +39:25:03.8 -- not a known variable star
05:27:07.60 +37:21:25.1 -- a known variable star
05:27:42.97 +38:15:22.3 -- a known variable star
05:29:04.39 +38:16:12.1 -- a known variable star
05:30:38.78 +37:43:02.9 -- not a known variable star
05:31:34.44 +37:53:11.4 -- a known variable star
05:31:34.75 +37:21:56.9 -- a known variable star
05:31:51.67 +37:21:15.4 -- not a known variable star
05:31:53.33 +37:35:55.4 -- not a known variable star
05:32:09.90 +37:20:04.0 -- not a known variable star
05:32:41.29 +38:27:36.4 -- not a known variable star
05:35:27.86 +37:11:40.0 -- a known variable star
05:36:05.09 +38:07:01.9 -- not a known variable star
05:36:14.11 +37:56:39.8 -- a known variable star
05:37:15.19 +39:47:47.7 -- a known variable star
05:38:07.86 +36:52:05.5 -- a known variable star
05:40:16.66 +38:35:46.9 -- a known variable star
05:45:26.24 +38:32:10.8 -- not a known variable star
05:47:51.28 +38:34:38.8 -- a known variable star
Found 16 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
36 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
04:56:35.81 +35:11:01.6
05:01:27.55 +33:10:54.4
05:05:49.67 +36:22:10.9
05:17:13.30 +35:18:57.7
05:18:46.64 +39:20:46.1
05:19:54.15 +36:28:35.7
05:20:26.13 +38:08:02.6
05:20:28.20 +39:26:18.2
05:20:46.20 +36:06:46.5
05:21:25.37 +37:42:32.9
05:21:39.05 +37:47:05.9
05:22:17.16 +36:57:51.8
05:22:50.86 +37:36:37.8
05:23:09.47 +37:30:30.7
05:24:00.67 +37:05:19.0
05:24:17.43 +37:16:09.8
05:25:40.54 +38:52:38.0
05:25:50.95 +39:25:03.8
05:27:07.60 +37:21:25.1
05:27:42.97 +38:15:22.3
05:29:04.39 +38:16:12.1
05:30:38.78 +37:43:02.9
05:31:34.44 +37:53:11.4
05:31:34.75 +37:21:56.9
05:31:51.67 +37:21:15.4
05:31:53.33 +37:35:55.4
05:32:09.90 +37:20:04.0
05:32:41.29 +38:27:36.4
05:35:27.86 +37:11:40.0
05:36:05.09 +38:07:01.9
05:36:14.11 +37:56:39.8
05:37:15.19 +39:47:47.7
05:38:07.86 +36:52:05.5
05:40:16.66 +38:35:46.9
05:45:26.24 +38:32:10.8
05:47:51.28 +38:34:38.8
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The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461289.79621143 -observatory V36
11:32:32.76 +04:14:37.5 Mercury (-0.9mag)
13:33:31.44 -14:08:12.3 Venus (-4.7mag)
07:11:17.09 +23:02:37.6 Mars (1.2mag)
09:08:13.49 +17:01:01.8 Jupiter (-1.8mag)
00:51:57.68 +02:40:15.2 Saturn (0.5mag)
04:13:40.44 +21:01:57.2 Uranus (5.7mag)
00:13:50.45 -00:02:35.5 Neptune (7.7mag)
20:25:39.77 -23:39:23.1 Pluto (14.5mag)
06:46:09.13 +26:29:36.3 Moon (-9.7mag)
-rw-r--r-- 1 apache apache 362 Sep 6 02:09 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461289.79621143:
09:08:10.35 +17:01:18.6 Io (6.2mag)
09:08:23.85 +17:00:11.7 Europa (6.3mag)
09:08:30.32 +16:59:38.9 Ganymede (5.7mag)
09:07:47.02 +17:03:11.2 Callisto (6.9mag)
09:05:57.80 +17:17:06.7 Himalia (15.7mag)
09:08:11.36 +17:01:12.4 Thebe (16.6mag)
09:05:35.60 +17:11:08.8 Elara (17.7mag)
09:12:08.49 +16:28:54.6 Pasiphae (17.9mag)
09:09:22.89 +17:18:32.0 Carme (19.0mag)
00:51:58.68 +02:40:35.9 Titan (8.3mag)
00:51:53.84 +02:40:20.9 Rhea (9.6mag)
00:52:15.47 +02:42:50.5 Iapetus (11.0mag)
00:52:09.41 +02:39:36.1 Hyperion (14.3mag)
00:50:45.50 +02:30:05.1 Phoebe (16.4mag)
-rw-r--r-- 1 apache apache 568 Sep 6 02:09 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461289.79621143:
21:56:26.58 -00:01:40.8 JWST
15:07:36.07 +52:14:41.2 Chandra
05:55:25.29 +31:57:59.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Sep 6 02:09 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461289.79621143 -observatory V36
03:39:48.99 +19:17:35.8 17.4mag P/1996 R2 (Lagerkvist)
18:02:34.18 -34:13:46.7 14.3mag P/2010 H2 (Vales)
07:18:42.62 -70:14:47.6 17.3mag C/2014 UN271 (Bernardinelli-Bernstein)
06:15:34.50 +33:40:28.1 17.7mag C/2017 K2 (PANSTARRS)
04:49:56.87 +45:19:41.2 15.7mag P/2021 N1 (ZTF)
04:49:56.87 +45:19:41.2 15.7mag P/2021 N1 (ZTF)
04:49:56.87 +45:19:41.2 15.7mag P/2021 N1 (ZTF)
04:49:56.87 +45:19:41.2 15.7mag P/2021 N1 (ZTF)
22:14:17.19 +28:47:28.3 17.4mag C/2022 E2 (ATLAS)
07:09:25.48 +25:59:51.7 16.9mag C/2022 N2 (PANSTARRS)
10:48:34.49 +27:15:44.5 17.1mag C/2022 QE78 (ATLAS)
09:48:01.98 +05:14:18.3 18.0mag C/2022 R6 (PANSTARRS)
15:29:49.03 -15:33:40.8 14.8mag C/2023 R1 (PANSTARRS)
08:37:30.61 +32:49:52.6 15.8mag C/2024 E1 (Wierzchos)
15:06:28.40 +15:20:04.7 17.9mag C/2024 G6 (ATLAS)
18:34:15.27 +43:12:41.9 13.7mag C/2024 J3 (ATLAS)
20:27:32.85 +49:21:09.8 17.4mag C/2024 R4 (PANSTARRS)
05:35:04.08 -13:00:48.4 15.1mag C/2024 T5 (ATLAS)
07:11:16.69 +18:44:34.4 17.8mag C/2025 J1 (Borisov)
11:16:22.53 +18:50:48.7 16.8mag C/2025 V2 (Rankin)
13:18:48.34 +00:11:48.4 16.8mag C/2025 Y1 (ATLAS)
16:38:49.24 +74:11:47.5 16.1mag C/2026 A2 (Bok)
03:06:16.13 +46:09:53.5 17.4mag C/2026 B2 (Sun-Gao)
12:12:20.81 +11:12:03.2 17.5mag A/2026 E1
22:25:10.33 -34:57:56.9 13.4mag 10P/Tempel
01:17:55.24 +36:49:21.7 18.0mag 11P/Tempel-Swift-LINEAR
11:47:30.15 -05:23:35.9 16.3mag 29P/Schwassmann-Wachmann
12:06:33.29 -04:46:39.6 17.6mag 63P/Wild
00:45:12.73 -07:00:20.0 15.4mag 65P/Gunn
06:37:23.21 +19:19:38.2 17.1mag 78P/Gehrels
03:17:12.08 +14:59:04.6 16.7mag 88P/Howell
05:34:54.63 +28:14:51.9 17.5mag 112P/Urata-Niijima
07:28:49.29 +25:04:09.8 17.9mag 114P/Wiseman-Skiff
10:25:39.36 +21:04:44.7 14.8mag 123P/West-Hartley
12:44:24.16 -20:59:19.9 17.4mag 124P/Mrkos
06:16:11.87 +20:40:10.7 15.9mag 128P/Shoemaker-Holt
02:35:55.02 -17:43:20.3 15.3mag 161P/Hartley-IRAS
09:39:34.41 +14:23:58.7 12.0mag 169P/NEAT
03:23:34.49 +08:33:19.2 14.5mag 220P/McNaught
04:45:21.66 +36:00:17.5 15.2mag 260P/McNaught
08:29:10.98 +35:48:20.6 17.3mag 295P/LINEAR
15:24:35.53 -00:08:11.5 17.9mag 391P/Kowalski
09:26:55.19 +16:54:05.7 17.9mag 450P/LONEOS
-rw-r--r-- 1 apache apache 2.1K Sep 6 02:09 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
19:45:06.20 +18:22:48.80 V488 2026-08-30.13 9.37
18:25:12.74 -22:25:28.60 V8055 2026-08-30.22 10.89
17:17:45.96 +64:31:40.10 ASASSN-26ez 2026-08-25.13 10.87
19:02:47.09 +58:08:21.00 AT2026zwo 2026-08-24.16 15.78
04:20:07.58 -42:26:59.90 AT2026zjy 2026-08-23.03 15.91
03:08:18.02 +11:54:46.50 SN2026ymb 2026-08-23.4 16.44
20:22:32.48 -50:45:14.30 SN2026yid 2026-08-22.82 15.13
04:24:28.39 -56:20:21.60 ASASSN-26ey 2026-08-20.02 15.55
16:46:37.81 -63:14:59.80 ASASSN-26ex 2026-08-18.78 3.63
21:28:47.85 +20:31:03.60 SN 2026sfn 2026-08-16.3 17.09
23:01:28.67 -61:00:39.00 SN 2026yib 2026-08-14.85 17.36
00:22:23.20 -32:16:02.70 SN 2026whu 2026-08-14.96 16.5
19:56:21.71 -37:24:19.90 ASASSN-26ew 2026-08-13.82 14.73
13:53:14.21 +00:26:52.00 SN 2026wkv 2026-08-10.12 15.83
05:21:07.61 +23:38:20.10 TCP J05210763+2338194 2026-08-10.59 9.34
01:28:20.49 +40:13:27.10 SN2026wpd 2026-08-9.34 16.37
23:47:50.89 +49:28:51.30 SN2026wjs 2026-08-9.24 17.09
16:03:20.92 +17:43:23.70 AT2026xau 2026-08-9.3 17.71
01:10:22.05 -09:34:08.50 SN2026weo 2026-08-7.46 15.76
00:56:54.35 -35:55:29.40 AT2026wdy 2026-08-5.05 16.08
22:08:07.63 -53:03:58.90 AT2026wek 2026-08-3.82 17.17
14:51:51.34 +66:13:24.60 ASASSN-26ev 2026-08-2.15 14.02
12:06:50.79 -36:16:06.20 SN2026wgm 2026-08-1.73 15.61
16:56:36.90 -59:29:26.00 ASASSN-26er 2026-07-25.82 15.09
01:21:27.83 -10:37:05.00 SN2026vbh 2026-07-25.61 15.97
21:17:31.59 +22:25:50.90 ASASSN-26eq 2026-07-24.37 15.13
18:53:36.89 +16:56:43.60 ASASSN-26ep 2026-07-23.47 -4.06
12:18:47.98 -30:48:47.50 ASASSN-26et 2026-07-22.76 13.98
13:00:47.82 +15:42:17.60 SN2026uwk 2026-07-21.75 16.38
18:52:31.11 -32:28:00.90 ASASSN-26en 2026-07-21.77 14.63
14:42:58.01 -62:32:59.10 ASASSN-26es 2026-07-20.79 15.36
20:12:45.57 -32:53:13.00 ASASSN-26em 2026-07-20.94 16.83
18:54:24.33 -46:11:51.70 ASASSN-26eu 2026-07-20.93 14.86
03:18:56.99 -80:55:10.40 AT2026ugi 2026-07-20.03 17.12
18:43:58.40 +24:22:41.80 ASASSN-26eo 2026-07-19.36 16.16
04:50:01.03 -02:22:33.80 ASASSN-26ej 2026-07-16.17 17.02
18:34:55.28 -31:41:00.90 ASASSN-26ek 2026-07-16.24 15.73
17:07:43.61 -44:21:53.50 ASASSN-26el 2026-07-15.86 16.01
14:45:08.35 +24:13:12.30 ASASSN-26ei 2026-07-16.17 16.46
10:00:46.44 -32:36:31.10 AT 2023mhb 2026-07-14.73 16.67
14:39:37.45 -11:22:36.20 AT 2026unl 2026-07-15.27 17.11
10:49:42.57 -11:25:55.80 ASASSN-26eh 2026-07-14.72 16.58
19:33:53.06 -07:15:00.80 ASASSN-22le 2026-07-14.15 15.5
02:45:40.52 -27:55:30.30 ASASSN-26ef 2026-07-12.35 15.86
23:26:43.80 +04:42:39.70 SN 2026qtn 2026-07-12.22 16.47
02:19:17.26 +28:57:15.40 ASASSN-26ec 2026-07-11.53 2.78
18:31:15.56 -05:34:31.50 AT2026stb 2026-07-11.28 -1.29
13:36:08.24 +23:29:05.00 AT2026pjf 2026-07-10.18 -0.72
17:33:39.82 +04:22:36.70 SN2026pir 2026-07-9.86 -0.66
11:21:41.26 -50:33:36.30 ASASSN-26ed 2026-07-8.8 -1.3
23:41:42.11 +26:29:49.10 AT2026qil 2026-07-9.3 16.15
20:21:30.50 -32:03:40.10 ASASSN-26ee 2026-07-7.22 15.53
19:37:44.09 -05:35:42.80 AT2026ryu 2026-07-7.17 14.88
11:06:55.46 -04:07:04.50 AT2026qqg 2026-07-5.01 16.82
19:07:23.69 -74:13:37.30 AT2026qly 2026-07-5.02 17.31
17:57:43.80 +27:18:40.10 ASASSN-26ea 2026-07-5.07 16.67
19:59:01.43 -32:07:34.30 ASASSN-26eb 2026-07-4.97 15.52
18:46:50.35 -57:44:13.20 SN 2026qqp 2026-07-5.03 -0.92
19:17:31.69 -39:55:29.90 ASASSN-26dz 2026-07-5.14 15.91
19:14:31.37 +12:03:52.90 AT 2026rdg 2026-07-3.43 11.81
04:05:50.09 -70:24:34.40 AT 2026qpr 2026-06-30.4 15.96
13:45:37.49 -05:59:35.80 SN 2026pub 2026-06-30.09 16.01
16:41:15.63 +39:17:14.70 SN 2026pel 2026-06-26.38 16.07
10:14:40.19 -35:38:21.30 ASASSN-26dy 2026-06-25.99 15.63
14:47:21.56 -40:15:51.30 ASASSN-26dv 2026-06-23.03 14.62
13:38:49.79 -77:21:06.70 ASASSN-26dw 2026-06-23.04 16.09
00:59:27.90 +33:08:13.20 SN 2026mke 2026-06-22.39 17.13
11:10:44.73 -30:20:45.50 SN 2026nmv 2026-06-22.06 16.56
21:36:15.68 -21:19:12.50 AT2026oxh 2026-06-22.15 17.14
17:31:38.38 -56:05:51.90 ASASSN-26dx 2026-06-22.02 14.72
14:10:13.44 -38:46:46.10 AT2026pvk 2026-06-22.06 16.53
20:56:47.23 -18:31:05.20 AT2026plb 2026-06-21.31 16.4
15:44:29.68 +21:00:59.30 SN2026ore 2026-06-21.29 17.57
23:50:05.98 -14:01:41.30 AT2026oxl 2026-06-21.52 17.64
17:36:54.73 -18:10:04.20 AT2026ouj 2026-06-20.92 15.15
00:34:04.08 -30:22:09.20 AT2026ntk 2026-06-18.09 17.34
20:49:13.39 +25:17:59.20 ASASSN-26du 2026-06-15.39 15.93
23:09:30.84 +32:40:42.00 SN2026oxc 2026-06-14.35 16.83
02:02:26.78 +32:04:21.30 AT2026ovz 2026-06-14.59 15.39
21:26:28.11 -72:31:19.50 AT2026nwc 2026-06-11 17.05
17:54:57.33 +26:32:34.20 SN 2026odc 2026-06-11.23 17.62
13:55:59.94 +17:30:37.20 SN 2026nyq 2026-06-11.1 16.24
00:50:45.14 -71:38:36.90 ASASSN-26dt 2026-06-11.13 10.22
14:42:19.73 +19:11:35.60 SN2026nyp 2026-06-10.3 16.32
12:23:23.92 +12:56:43.50 SN2026mta 2026-06-8.29 16.69
12:30:18.51 +47:12:33.20 SN2026oao 2026-06-9.32 17.02
10:51:05.21 -42:28:56.60 AT2026nvf 2026-06-8.12 16.75
13:50:22.48 -07:35:00.00 SN2026npn 2026-06-8.02 17.58
00:56:07.17 +43:01:43.20 ASASSN-26dq 2026-06-7.43 13.58
01:07:49.46 +41:59:43.70 SN 2026obc 2026-06-7.43 15.15
21:11:25.22 +14:14:31.90 ASASSN-26dr 2026-06-7.24 16.24
06:21:27.06 -65:16:42.00 ASASSN-26ds 2026-06-2.97 15.02
20:07:38.15 -21:07:05.40 SN2026mho 2026-05-25.18 -1.12
11:29:42.55 +79:01:03.10 AT2026min 2026-05-24.21 16.63
11:44:33.11 -68:48:32.90 ASASSN-26no 2026-05-24.03 8.35
19:00:42.82 -48:31:01.60 ASASSN-26dp 2026-05-22.31 -3.28
14:23:56.59 -58:37:47.40 ASASSN-26dn 2026-05-20.01 14.59
11:24:54.06 +47:57:01.60 AT2026nma 2026-05-20.29 15.46
21:27:08.58 +33:24:38.10 AT2026lli 2026-05-19.34 15.86
00:31:01.41 -13:38:51.70 AT2026nad 2026-05-19.39 15.34
-rw-r--r-- 1 apache apache 5.7K Sep 6 02:09 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:44:56.43 +41:57:41.6 PNV J00445643+4157416 2026-07-13.8026 17.98Cmag
00:42:55.36 +41:17:27.0 PNV J00425536+4117270 2026-07-20.1813 17.7mag
20:35:43.64 +61:31:32.9 TCP J20354364+6131329 2026-07-20.5443 14.4mag
21:17:31.48 +22:25:51.0 TCP J21173148+2225510 2026-07-23.5577 14.8mag
00:41:24.04 +40:49:02.8 PNV J00412404+4049028 2026-07-25.0157 18.7mag
00:43:04.26 +41:02:28.6 PNV J00430426+4102286 2026-07-26.1512 20mag
14:51:51.40 +66:13:24.0 TCP J14515140+6613240 2026-07-29.2561 13.5mag
00:43:06.15 +41:22:08.2 PNV J00430615+4122082 2026-07-30.0085 19.4mag
00:41:33.23 +41:10:12.2 PNV J00413323+4110122 2026-08-02.8913 17.1mag
05:21:07.63 +23:38:19.4 TCP J05210763+2338194 2026-08-06.4109 11.2mag
22:57:17.96 +47:07:41.8 TCP J22571796+4707418 2026-08-09.3289 14.3mag
09:13:38.17 +76:28:18.1 PSN J09133817+7628181 2026-08-09.8037 15.4mag
00:43:17.29 +41:26:48.6 PNV J00431729+4126486 2026-08-14.0920 16.8mag
00:42:52.82 +41:10:58.6 PNV J00425282+4110586 2026-08-17.7723 19.9mag
00:42:52.83 +41:10:59.6 PNV J00425283+4110596 2026-08-18.6119 19.3mag
18:25:12.76 -22:25:29.3 TCP J18251276-2225293 2026-08-19.1062 9.4mag
18:03:09.04 +12:18:14.0 TCP J18030904+1218140 2026-08-19.5199 14.9mag
19:45:06.48 +18:22:42.2 PNV J19450648+1822422 2026-08-25.1278 9.0mag
00:42:54.65 +41:22:59.3 PNV J00425465+4122593 2026-08-25.4712 18.9mag
00:42:50.38 +41:18:58.76 PNV J00425038+4118587 2026-09-04.1512 18.2mag
-rw-r--r-- 1 apache apache 190K Sep 6 02:09 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
01:07:41.150 -00:00:30.93 AT 2026yng 2026-08-06.84 21.99
01:00:19.600 +05:13:13.68 AT 2026ynf 2026-08-06.84 21.4
00:02:10.680 +04:29:05.91 AT 2026yne 2026-08-06.83 22.4
00:13:33.330 +04:19:21.34 AT 2026ynd 2026-08-06.77 22.15
23:51:06.360 +01:51:14.34 AT 2026ync 2026-08-06.76 22.21
23:15:09.720 +02:58:45.37 AT 2026ynb 2026-08-06.75 22.52
22:50:40.350 +05:31:47.83 AT 2026yna 2026-08-05.73 21.56
22:48:01.050 +02:29:57.95 AT 2026ymz 2026-08-05.73 21.98
22:56:40.110 +02:46:51.37 AT 2026ymy 2026-08-04.80 21.96
01:44:34.660 +05:27:13.55 AT 2026ymx 2026-08-01.88 21.27
01:29:50.630 +00:07:42.35 AT 2026ymw 2026-07-21.86 22.34
01:20:55.160 +01:31:29.58 AT 2026ymv 2026-07-20.88 22.17
23:25:01.600 +02:19:39.37 AT 2026ymu 2026-07-20.78 22.49
22:52:58.240 +03:42:25.38 AT 2026ymt 2026-08-05.73 21.81
23:42:43.162 +19:31:30.19 AT 2026yms 2026-08-09.94 19.57
21:20:13.290 -37:42:51.98 AT 2026ymr 2026-08-09.45 19.171
17:37:51.010 -21:58:53.20 AT 2026ymq 2026-08-09.59 14.86
22:57:17.960 +47:07:41.80 AT 2026ymp 2026-08-09.33 14.3
21:11:14.725 +16:08:57.69 AT 2026ymo 2026-08-04.97 19.97
00:45:33.395 +25:23:53.86 AT 2026ymn 2026-08-10.09 19.737
-rw-r--r-- 1 apache apache 88K Sep 6 02:09 tns_transients_list.txt
