This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 10.94 16:16:10.23 -37:04:12.4
342.04829 9.80314 galactic Sco Second-epoch detections are separated by 1.6" and 8.1 pix
The object was found in VSX 1" ASASSN-V J161610.13-370412.4
Type: SR
# Max. Min./Amp. JD0 Period
14.530 g Y 0.310 g 2459376.25800 33.210000000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:16:10.23 -37:04:12.4: 11.99 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:16:10.23 -37:04:12.4: 11.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.96 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J161610.13-370412.4,2461259.6038,10.94,0.05,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 J161610.13-370412.4 20260807.1038 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 11.26 16:48:26.73 -36:07:14.4
347.16933 5.66763 galactic Sco Second-epoch detections are separated by 1.1" and 8.4 pix
The object was found in VSX 2" ASASSN-V J164826.91-360715.5
Type: L
# Max. Min./Amp. JD0 Period
12.680 V 12.890 V
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:48:26.73 -36:07:14.4: 12.18 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:48:26.73 -36:07:14.4: 12.20 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.19 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J164826.91-360715.5,2461259.6038,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J164826.91-360715.5 20260807.1038 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 11.14 16:30:51.63 -37:27:48.8
343.81657 7.42839 galactic Sco Second-epoch detections are separated by 1.1" and 8.2 pix
The object was found in VSX 1" ASASSN-V J163051.61-372749.2
Type: SR
# Max. Min./Amp. JD0 Period
12.870 V 13.020 V 2457649.52600 42.610000000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:30:51.63 -37:27:48.8: 12.26 +/- 0.04 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:30:51.63 -37:27:48.8: 12.30 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.28 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J163051.61-372749.2,2461259.6038,11.14,0.05,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 J163051.61-372749.2 20260807.1038 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 11.27 16:04:02.54 -35:26:27.8
341.39667 12.67053 galactic Lup Second-epoch detections are separated by 2.3" and 7.7 pix
The object was found in VSX 5" ASASSN-V J160402.16-352627.8
Type: L
# Max. Min./Amp. JD0 Period
13.610 V 13.940 V
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:04:02.54 -35:26:27.8: 12.46 +/- 0.06 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:04:02.54 -35:26:27.8: 12.25 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.36 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J160402.16-352627.8,2461259.6038,11.27,0.05,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 J160402.16-352627.8 20260807.1038 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 11.84 16:42:54.09 -31:11:54.6
350.22850 9.71359 galactic Sco Second-epoch detections are separated by 2.1" and 8.3 pix
The object was found in VSX 1" ASASSN-V J164254.19-311155.2
Type: L
# Max. Min./Amp. JD0 Period
13.150 V 13.550 V
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:42:54.09 -31:11:54.6: 12.75 +/- 0.05 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:42:54.09 -31:11:54.6: 12.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.79 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J164254.19-311155.2,2461259.6038,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J164254.19-311155.2 20260807.1038 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 11.68 16:37:14.17 -31:45:27.3
348.99928 10.26683 galactic Sco Second-epoch detections are separated by 1.1" and 8.6 pix
The object was found in VSX 0" ASAS J163714-3145.4
Type: MISC
# Max. Min./Amp. JD0 Period
8.901 Ic Y 0.187 Ic 2452608.70000 59.060000000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:37:14.17 -31:45:27.3: 12.71 +/- 0.05 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:37:14.17 -31:45:27.3: 12.61 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.67 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J163714-3145.4,2461259.6038,11.68,0.05,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
ASAS J163714-3145.4 20260807.1038 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 11.52 16:53:57.32 -37:32:57.6
346.76295 3.90912 galactic Sco Second-epoch detections are separated by 0.8" and 8.3 pix
The object was found in VSX 2" ASASSN-V J165357.44-373258.3
Type: SR
# Max. Min./Amp. JD0 Period
13.160 V 13.410 V 2458207.87500 55.670000000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:53:57.32 -37:32:57.6: 12.46 +/- 0.05 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:53:57.32 -37:32:57.6: 12.50 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.47 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J165357.44-373258.3,2461259.6038,11.52,0.05,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 J165357.44-373258.3 20260807.1038 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 11.31 16:38:45.04 -37:19:05.7
344.98378 6.36328 galactic Sco Second-epoch detections are separated by 0.1" and 8.2 pix
The object was found in VSX 3" ASASSN-V J163845.08-371908.8
Type: L
# Max. Min./Amp. JD0 Period
12.880 V 13.200 V
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:38:45.04 -37:19:05.7: 12.33 +/- 0.04 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:38:45.04 -37:19:05.7: 12.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.29 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J163845.08-371908.8,2461259.6038,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J163845.08-371908.8 20260807.1038 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 11.25 16:55:15.10 -30:34:35.0
352.41021 8.05193 galactic Sco Second-epoch detections are separated by 0.3" and 8.6 pix
The object was found in VSX 3" HM Sco
Type: SRA:
# Max. Min./Amp. JD0 Period
11.800 V 13.500 : V 2453639.00000 178.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:55:15.10 -30:34:35.0: 12.20 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:55:15.10 -30:34:35.0: 12.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.21 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HM Sco,2461259.6038,11.25,0.05,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
HM Sco 20260807.1038 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 11.02 16:26:47.78 -37:57:49.1
342.89401 7.67270 galactic Sco Second-epoch detections are separated by 0.3" and 8.1 pix
The object was found in VSX 1" ASASSN-V J162647.71-375750.1
Type: L
# Max. Min./Amp. JD0 Period
12.900 V 13.050 V
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:26:47.78 -37:57:49.1: 12.03 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:26:47.78 -37:57:49.1: 12.05 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.04 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J162647.71-375750.1,2461259.6038,11.02,0.05,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
ASASSN-V J162647.71-375750.1 20260807.1038 11.02CV 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 08 07.1038 2461259.6038 10.79 16:16:20.92 -36:19:10.3
342.61105 10.31068 galactic Sco Second-epoch detections are separated by 1.0" and 7.8 pix
The object was found in VSX 2" ASAS J161621-3619.2
Type: SR
# Max. Min./Amp. JD0 Period
8.651 Ic Y 0.222 Ic 2452769.40000 147.100000000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:16:20.92 -36:19:10.3: 12.04 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:16:20.92 -36:19:10.3: 11.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.96 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J161621-3619.2,2461259.6038,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J161621-3619.2 20260807.1038 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 11.08 16:20:13.10 -37:20:53.4
342.42582 9.03622 galactic Sco Second-epoch detections are separated by 7.9" and 8.1 pix
The object was found in VSX 4" ASASSN-V J162012.99-372056.9
Type: SR
# Max. Min./Amp. JD0 Period
13.100 V 13.230 V 2457650.00000 149.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:20:13.10 -37:20:53.4: 12.06 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:20:13.10 -37:20:53.4: 12.09 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.07 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J162012.99-372056.9,2461259.6038,11.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J162012.99-372056.9 20260807.1038 11.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 10.97 16:29:22.94 -37:33:38.8
343.54344 7.57687 galactic Sco Second-epoch detections are separated by 0.9" and 8.0 pix
The object was found in VSX 3" ASAS J162923-3733.6
Type: MISC
# Max. Min./Amp. JD0 Period
8.889 Ic Y 0.215 Ic 2452836.20000 220.200000000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:29:22.94 -37:33:38.8: 11.98 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:29:22.94 -37:33:38.8: 12.00 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J162923-3733.6,2461259.6038,10.97,0.05,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
ASAS J162923-3733.6 20260807.1038 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 10.95 16:37:01.77 -37:29:47.4
344.62128 6.50054 galactic Sco Second-epoch detections are separated by 1.2" and 8.2 pix
The object was found in VSX 1" ASASSN-V J163701.71-372946.4
Type: SR
# Max. Min./Amp. JD0 Period
12.320 V 12.490 V 2458341.69400 39.550000000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:37:01.77 -37:29:47.4: 11.82 +/- 0.02 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:37:01.77 -37:29:47.4: 11.97 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.87 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J163701.71-372946.4,2461259.6038,10.95,0.05,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 J163701.71-372946.4 20260807.1038 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 10.76 16:50:59.26 -36:22:53.6
347.29531 5.10637 galactic Sco Second-epoch detections are separated by 1.8" and 8.1 pix
The object was found in VSX 2" ASASSN-V J165059.42-362253.9
Type: L
# Max. Min./Amp. JD0 Period
12.280 V 12.730 V
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:50:59.26 -36:22:53.6: 11.80 +/- 0.02 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:50:59.26 -36:22:53.6: 11.73 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.77 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J165059.42-362253.9,2461259.6038,10.76,0.05,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 J165059.42-362253.9 20260807.1038 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 10.26 16:32:37.24 -37:00:39.5
344.39170 7.47700 galactic Sco Second-epoch detections are separated by 0.8" and 8.0 pix
The object was found in VSX 0" ASASSN-V J163237.25-370039.9
Type: SR
# Max. Min./Amp. JD0 Period
12.030 V 12.190 V 2457546.71600 40.450000000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:32:37.24 -37:00:39.5: 11.34 +/- 0.02 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:32:37.24 -37:00:39.5: 11.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.31 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J163237.25-370039.9,2461259.6038,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J163237.25-370039.9 20260807.1038 10.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 11.84 16:36:40.78 -37:22:39.2
344.66400 6.63157 galactic Sco Second-epoch detections are separated by 0.6" and 8.2 pix
The object was found in VSX 1" ASASSN-V J163640.78-372239.9
Type: SR
# Max. Min./Amp. JD0 Period
13.840 V 14.140 V 2457457.00000 155.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:36:40.78 -37:22:39.2: 12.97 +/- 0.08 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:36:40.78 -37:22:39.2: 13.00 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.98 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J163640.78-372239.9,2461259.6038,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J163640.78-372239.9 20260807.1038 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 07.1038 2461259.6038 9.05 16:08:28.13 -36:58:53.6
340.98775 10.93558 galactic Sco Second-epoch detections are separated by 1.0" and 7.9 pix
The object was found in VSX 4" ASAS J160828-3658.9
Type: MISC|SR
# Max. Min./Amp. JD0 Period
11.430 V Y 0.690 V 2452162.30000 87.116104000000
The object was not found in astcheck.
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:08:28.13 -36:58:53.6: 10.11 +/- 0.01 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:08:28.13 -36:58:53.6: 10.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.09 +/- 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 Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J160828-3658.9,2461259.6038,9.05,0.05,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
ASAS J160828-3658.9 20260807.1038 9.05CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461140.87939870 10.04.2026 09:06:10.048 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
First image: 2461140.87939870 10.04.2026 09:06:10.048 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
Last image: 2461259.60418318 07.08.2026 02:29:51.427 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.63
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: 3 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): 5885
Objects passed selection criteria: 5876
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 4461.5
Average stars matched: 4446.25 (99.6582 %)
Memory usage VmPeak: 233044 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 21:32:01 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: 2461140.87939870 10.04.2026 09:06:10.048 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
First image: 2461140.87939870 10.04.2026 09:06:10.048 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
Last image: 2461259.60418318 07.08.2026 02:29:51.427 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 127
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.24
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 16 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): 76023
Objects passed selection criteria: 75843
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 54701.5
Average stars matched: 53771.5 (98.2999 %)
Memory usage VmPeak: 561172 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Aug 6 21:35:07 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/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
SExtractor catalog cache: saved Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.cat to cache
SExtractor catalog cache: saved Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.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/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.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: 2461259.60344740
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits exists and is non-empty
Saving wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits to local_wcs_cache/
'wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits' -> 'local_wcs_cache/wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits'
wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits exists and is non-empty
Saving wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits to local_wcs_cache/
'wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits' -> 'local_wcs_cache/wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits'
wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits exists and is non-empty
Saving wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits to local_wcs_cache/
'wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits' -> 'local_wcs_cache/wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits'
wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits exists and is non-empty
Saving wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits to local_wcs_cache/
'wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits' -> 'local_wcs_cache/wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits (1st reference image)
verification OK: wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
Image size: 941.6'x627.6' 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: 16:41:53.786 -34:00:13.61 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_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits (1st new image)
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
Image size: 940.4'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:41:45.276 -34:00:04.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:41:53.786 -34:00:13.61
Second-epoch image center 16:41:45.276 -34:00:04.91
Angular distance between the image centers 0.0295 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits (2nd new image)
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Image size: 940.5'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:41:42.501 -33:59:29.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:41:53.786 -34:00:13.61
Second-epoch image center 16:41:42.501 -33:59:29.23
Angular distance between the image centers 0.0409 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 16:41:45.276 -34:00:04.91
Second-epoch second image center 16:41:42.501 -33:59:29.23
Angular distance between the image centers 0.01379 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/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits &> /tmp/tmp.gFmvUSo8tH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits &> /tmp/tmp.A67UDOepeT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits &> /tmp/tmp.nIR0T94OQ8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits &> /tmp/tmp.zLoMHLN32I
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.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_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits and wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
'tns_transients_list.txt' -> '../tns_transients_list.txt'
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_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits and wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat
Found non-empty wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits and wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat
The reference image (wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits) and catalog (wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat) found
'wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat' -> 'wcsmag.cat'
Read 7689 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.0332 to 260.1409 deg, Dec -39.4739 to -28.0868 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 240.0332 to 260.1409 deg, Dec -39.4739 to -28.0868 deg
Loaded 14003 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): 6036 out of 6244 total matches.
Matched with Tycho-2 6244 out of 7689 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.618600
a=0.000000 b=1.000000 c=22.618600
From vast_summary.log: estimated ref. image limiting mag.: -8.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.99
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.99
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7689 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.0332 to 260.1409 deg, Dec -39.4739 to -28.0868 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 240.0332 to 260.1409 deg, Dec -39.4739 to -28.0868 deg
Loaded 14003 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): 6036 out of 6244 total matches.
Matched with Tycho-2 6244 out of 7689 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
Forced-photometry filter: calibrated wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits -> calib.txt_param_ref_wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits (aperture=6.2)
Read 5944 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.0333 to 260.1077 deg, Dec -39.5114 to -28.0869 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 240.0333 to 260.1077 deg, Dec -39.5114 to -28.0869 deg
Loaded 14020 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): 4805 out of 4909 total matches.
Matched with Tycho-2 4909 out of 5944 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Forced-photometry filter: calibrated wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits -> calib.txt_param_ref_wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
2.2 pix Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
3.6 pix fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
3.6 pix fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Limiting magnitude estimates:
14.0 mag. Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
13.7 mag. Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
12.4 mag. fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
12.3 mag. fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
All-image limiting magnitude estimate: 12.3 (SNR ) 10.0 (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
############ /tmp/tmp.gFmvUSo8tH (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits' -> 'wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.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/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
WCS-calibrated image found: wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
Checking if the catalog wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat corresponding to the image wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat corresponding to the image wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
WCS catalog name: wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.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=670, bad_region=0, passed=7689
Got 7689 stars (including 7009 good ones) from the SExtractor catalog wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat
util/solve_plate_with_UCAC5 got 7689 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 252 to 311 (Dec -39.5 to -28.1)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 4850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 7689 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 252 to 311 (Dec -39.5 to -28.1)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 7689 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 7689 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4848 stars left (next iteration limit 5335)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits N_match=4848 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.424 sigma_q2_arcsec=0.476 sigma_q3_arcsec=0.398 sigma_q4_arcsec=0.538 n_q1=921 n_q2=1308 n_q3=1101 n_q4=1518 worst_quadrant_to_overall_ratio=1.158
The image catalog is written to wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits -region wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.A67UDOepeT (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits' -> 'wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.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/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS-calibrated image found: wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Checking if the catalog wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat corresponding to the image wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat corresponding to the image wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS catalog name: wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.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=444, bad_region=0, passed=5944
Got 5944 stars (including 5491 good ones) from the SExtractor catalog wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat
util/solve_plate_with_UCAC5 got 5944 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 252 to 311 (Dec -39.5 to -28.1)
Done reading UCAC5 zone files...
Matched 4916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 4836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 5944 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 252 to 311 (Dec -39.5 to -28.1)
Done reading UCAC5 zone files...
Matched 4916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 5944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 5944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 4831 stars left (next iteration limit 5316)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits N_match=4831 sigma_overall_arcsec=0.448 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.430 sigma_q3_arcsec=0.388 sigma_q4_arcsec=0.550 n_q1=915 n_q2=1155 n_q3=1186 n_q4=1575 worst_quadrant_to_overall_ratio=1.230
The image catalog is written to wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits -region wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nIR0T94OQ8 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
Checking if the catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
WCS catalog name: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.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=218, bad_region=0, passed=2172
Got 2172 stars (including 1950 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat
util/solve_plate_with_UCAC5 got 2172 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.4'
Seting catalog search parameters based on the expected field of view 940.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013061 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010449 (37.6 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 253 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 1918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1882 matched stars entering correct_measured_positions(), 1875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1882 matched stars entering correct_measured_positions(), 2162 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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 253 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 1918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1881 matched stars entering correct_measured_positions(), 2162 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 1881 matched stars entering correct_measured_positions(), 2162 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 1881 stars left (next iteration limit 2070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1881 robust_rms=7.024 arcsec worst_quadrant_rms=25.573 arcsec
SIP_REFIT: SIP order 3 trial: matched=1881 robust_rms=0.581 arcsec worst_quadrant_rms=0.736 arcsec
SIP_REFIT: SIP order 5 trial: matched=1881 robust_rms=0.483 arcsec worst_quadrant_rms=0.733 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=1881 robust_rms_before=1.065 arcsec robust_rms_before_corrected=0.680 arcsec robust_rms_after=0.581 arcsec worst_quadrant_rms_before=0.919 worst_quadrant_rms_after=0.736
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
Image size: 940.4'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:41:45.260 -34:00:05.48 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 2172 stars ###
'wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/correct_sextractor_wcs_catalog_usingxy2sky3906664.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 1.065 -> 0.581 arcsec)
WCS_QUALITY_DIAG: file=fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits N_match=1881 sigma_overall_arcsec=0.628 sigma_q1_arcsec=0.595 sigma_q2_arcsec=0.792 sigma_q3_arcsec=0.579 sigma_q4_arcsec=0.573 n_q1=262 n_q2=493 n_q3=377 n_q4=749 worst_quadrant_to_overall_ratio=1.262
The image catalog is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits -region wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.zLoMHLN32I (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Checking if the catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
WCS catalog name: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.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=194, bad_region=0, passed=2130
Got 2130 stars (including 1935 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat
util/solve_plate_with_UCAC5 got 2130 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.5'
Seting catalog search parameters based on the expected field of view 940.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013063 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010450 (37.6 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 253 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 1902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1865 matched stars entering correct_measured_positions(), 1859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1865 matched stars entering correct_measured_positions(), 2120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 253 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 1903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1867 matched stars entering correct_measured_positions(), 2120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 1867 matched stars entering correct_measured_positions(), 2120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 1867 stars left (next iteration limit 2051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1867 robust_rms=6.541 arcsec worst_quadrant_rms=28.861 arcsec
SIP_REFIT: SIP order 3 trial: matched=1867 robust_rms=0.580 arcsec worst_quadrant_rms=0.750 arcsec
SIP_REFIT: SIP order 5 trial: matched=1867 robust_rms=0.505 arcsec worst_quadrant_rms=0.719 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=1867 robust_rms_before=1.070 arcsec robust_rms_before_corrected=0.717 arcsec robust_rms_after=0.580 arcsec worst_quadrant_rms_before=0.989 worst_quadrant_rms_after=0.750
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Image size: 940.4'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:41:42.487 -33:59:29.77 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 2130 stars ###
'wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/correct_sextractor_wcs_catalog_usingxy2sky3906663.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 3, robust RMS 1.070 -> 0.580 arcsec)
WCS_QUALITY_DIAG: file=fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits N_match=1867 sigma_overall_arcsec=0.633 sigma_q1_arcsec=0.668 sigma_q2_arcsec=0.853 sigma_q3_arcsec=0.550 sigma_q4_arcsec=0.561 n_q1=250 n_q2=505 n_q3=333 n_q4=779 worst_quadrant_to_overall_ratio=1.347
The image catalog is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits -region wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits sigma_overall=0.464 worst_q_ratio=1.158
ref2=Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits sigma_overall=0.448 worst_q_ratio=1.230
new1=fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits sigma_overall=0.628 worst_q_ratio=1.262
new2=fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits sigma_overall=0.633 worst_q_ratio=1.347
reference average sigma_overall=0.456 worst_q_ratio=1.194
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227_astrometric_residuals.png (4848 matched stars from wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236_astrometric_residuals.png (4831 matched stars from wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000_astrometric_residuals.png (1881 matched stars from wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001_astrometric_residuals.png (1867 matched stars from wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.49 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits'
Saving fully-calibrated image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits'
Preparing the HTML report for the field Sco-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20051_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 20051_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:14:51.36 -33:25:55.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20055_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 20055_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:07:35.65 -31:49:30.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06022_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 06022_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:08:21.01 -31:03:20.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Sco-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 ####
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/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
SExtractor catalog cache: saved Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.cat to cache
SExtractor catalog cache: saved Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
Creating symlink local_wcs_cache/wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits exists and is non-empty
wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits exists and is non-empty
wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits exists and is non-empty
wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits (1st reference image)
verification OK: wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
Image size: 941.6'x627.6' 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: 16:41:53.786 -34:00:13.61 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_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits (1st new image)
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
Image size: 940.4'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:41:45.276 -34:00:04.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:41:53.786 -34:00:13.61
Second-epoch image center 16:41:45.276 -34:00:04.91
Angular distance between the image centers 0.0295 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits (2nd new image)
verification OK: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Image size: 940.5'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:41:42.501 -33:59:29.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:41:53.786 -34:00:13.61
Second-epoch image center 16:41:42.501 -33:59:29.23
Angular distance between the image centers 0.0409 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 16:41:45.276 -34:00:04.91
Second-epoch second image center 16:41:42.501 -33:59:29.23
Angular distance between the image centers 0.01379 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/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits &> /tmp/tmp.A1L88VwtPC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits &> /tmp/tmp.71AXyPftU2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits &> /tmp/tmp.H1YMUJFRNs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits &> /tmp/tmp.6cbOBLPczD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.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_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits and wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.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_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits and wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat
Found non-empty wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits and wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat
The reference image (wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits) and catalog (wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat) found
'wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat' -> 'wcsmag.cat'
Read 99579 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.0233 to 260.1458 deg, Dec -39.4792 to -27.9369 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 240.0233 to 260.1458 deg, Dec -39.4792 to -27.9369 deg
Loaded 14194 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): 9889 out of 11284 total matches.
Matched with Tycho-2 11284 out of 99579 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.386800
a=0.000000 b=1.000000 c=22.386800
From vast_summary.log: estimated ref. image limiting mag.: -8.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.15
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 99579 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.0233 to 260.1458 deg, Dec -39.4792 to -27.9369 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 240.0233 to 260.1458 deg, Dec -39.4792 to -27.9369 deg
Loaded 14194 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): 9889 out of 11284 total matches.
Matched with Tycho-2 11284 out of 99579 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
Forced-photometry filter: calibrated wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits -> calib.txt_param_ref_wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits (aperture=4.4)
Read 79602 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.0333 to 260.1381 deg, Dec -39.5211 to -27.9819 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 240.0333 to 260.1381 deg, Dec -39.5211 to -27.9819 deg
Loaded 14186 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): 10242 out of 11282 total matches.
Matched with Tycho-2 11282 out of 79602 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Forced-photometry filter: calibrated wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits -> calib.txt_param_ref_wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits (aperture=4.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 113 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
2.0 pix Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
3.0 pix fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
3.0 pix fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Limiting magnitude estimates:
14.1 mag. Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
13.9 mag. Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
12.6 mag. fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
12.6 mag. fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 12.1 (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.A1L88VwtPC (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits' -> 'wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.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/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
WCS-calibrated image found: wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
Checking if the catalog wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat corresponding to the image wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat corresponding to the image wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits
WCS catalog name: wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.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=1, no_mag_err=0, low_SNR=22, blended=6459, bad_region=1, passed=99556
Got 99556 stars (including 92953 good ones) from the SExtractor catalog wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat
util/solve_plate_with_UCAC5 got 99556 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 252 to 312 (Dec -39.5 to -27.9)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 4859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4859 matched stars entering correct_measured_positions(), 99556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 252 to 312 (Dec -39.5 to -27.9)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 99556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 99556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 4857 stars left (next iteration limit 5344)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits N_match=4857 sigma_overall_arcsec=0.443 sigma_q1_arcsec=0.403 sigma_q2_arcsec=0.455 sigma_q3_arcsec=0.394 sigma_q4_arcsec=0.520 n_q1=955 n_q2=1387 n_q3=1084 n_q4=1431 worst_quadrant_to_overall_ratio=1.174
The image catalog is written to wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits -region wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.71AXyPftU2 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits' -> 'wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.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/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS-calibrated image found: wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
Checking if the catalog wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat corresponding to the image wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat corresponding to the image wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits
WCS catalog name: wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.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=17, blended=4102, bad_region=1, passed=79585
Got 79585 stars (including 75362 good ones) from the SExtractor catalog wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat
util/solve_plate_with_UCAC5 got 79585 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 252 to 312 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 4855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 79585 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 252 to 312 (Dec -39.5 to -28.0)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4851 matched stars entering correct_measured_positions(), 79585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4851 matched stars entering correct_measured_positions(), 79585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4851 stars left (next iteration limit 5340)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits N_match=4851 sigma_overall_arcsec=0.437 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.426 sigma_q3_arcsec=0.387 sigma_q4_arcsec=0.539 n_q1=954 n_q2=1263 n_q3=1160 n_q4=1474 worst_quadrant_to_overall_ratio=1.231
The image catalog is written to wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits -region wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.H1YMUJFRNs (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
Checking if the catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
WCS catalog name: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.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=1, no_mag_err=0, low_SNR=1, blended=721, bad_region=1, passed=20760
Got 20760 stars (including 20012 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat
util/solve_plate_with_UCAC5 got 20760 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.4'
Seting catalog search parameters based on the expected field of view 940.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013061 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010449 (37.6 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 252 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 4818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 20760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 252 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 4904 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(), 20760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 20760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 4815 stars left (next iteration limit 5297)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits N_match=4815 sigma_overall_arcsec=0.673 sigma_q1_arcsec=0.800 sigma_q2_arcsec=0.977 sigma_q3_arcsec=0.516 sigma_q4_arcsec=0.577 n_q1=642 n_q2=1276 n_q3=927 n_q4=1970 worst_quadrant_to_overall_ratio=1.452
The image catalog is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits -region wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6cbOBLPczD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Checking if the catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
WCS catalog name: wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.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=2, blended=772, bad_region=1, passed=20431
Got 20431 stars (including 19615 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat
util/solve_plate_with_UCAC5 got 20431 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.5'
Seting catalog search parameters based on the expected field of view 940.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013063 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010450 (37.6 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 252 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 4906 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: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 20431 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 252 to 311 (Dec -39.4 to -28.1)
Done reading UCAC5 zone files...
Matched 4906 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(), 20431 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 20431 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits N_match=4823 sigma_overall_arcsec=0.692 sigma_q1_arcsec=0.851 sigma_q2_arcsec=0.993 sigma_q3_arcsec=0.559 sigma_q4_arcsec=0.585 n_q1=628 n_q2=1306 n_q3=843 n_q4=2046 worst_quadrant_to_overall_ratio=1.435
The image catalog is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits -region wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.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_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-28-47_20.00sec_-0.00C_LIGHTs_0000.fits
Saving fully-calibrated image wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.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_2026-08-06_CI_Sco-03-Q1b1x1_213033_TTUQ1b1x1_3895752_g0OAqhhj/wcs_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001.fits
Preparing the HTML report for the field Sco-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:44:07.63 -30:59:57.9: 10.92 +/- 0.01 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 17:00:59.09 -29:39:19.9: 10.69 +/- 0.01 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:44:07.63 -30:59:57.9: 10.82 +/- 0.02 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 17:00:59.09 -29:39:19.9: 10.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.88 +/- 0.01
Forced photometry filter REJECTED candidate at 16:44:07.63 -30:59:57.9: ref_mag=10.88 +/- 0.01 new_mean_mag=10.8454 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 10.63 +/- 0.01
Forced photometry filter REJECTED candidate at 17:00:59.09 -29:39:19.9: ref_mag=10.63 +/- 0.01 new_mean_mag=10.6088 delta=0.02 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:16:10.23 -37:04:12.4: 11.99 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:04:02.54 -35:26:27.8: 12.46 +/- 0.06 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:30:51.63 -37:27:48.8: 12.26 +/- 0.04 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:48:26.73 -36:07:14.4: 12.18 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:16:10.23 -37:04:12.4: 11.92 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.03
Forced photometry filter KEPT candidate at 16:16:10.23 -37:04:12.4: ref_mag=11.96 +/- 0.03 new_mean_mag=10.9394 delta=1.02 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:04:02.54 -35:26:27.8: 12.25 +/- 0.06 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:30:51.63 -37:27:48.8: 12.30 +/- 0.05 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:42:54.09 -31:11:54.6: 12.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.04
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:48:26.73 -36:07:14.4: 12.20 +/- 0.04 detection
Forced photometry filter KEPT candidate at 16:04:02.54 -35:26:27.8: ref_mag=12.36 +/- 0.04 new_mean_mag=11.2676 delta=1.10 (need > 0.90)
Forced photometry reference-image weighted average: 12.28 +/- 0.03
Forced photometry filter KEPT candidate at 16:30:51.63 -37:27:48.8: ref_mag=12.28 +/- 0.03 new_mean_mag=11.1379 delta=1.14 (need > 0.90)
Forced photometry reference-image weighted average: 12.19 +/- 0.03
Forced photometry filter KEPT candidate at 16:48:26.73 -36:07:14.4: ref_mag=12.19 +/- 0.03 new_mean_mag=11.2458 delta=0.94 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:37:14.17 -31:45:27.3: 12.71 +/- 0.05 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:42:54.09 -31:11:54.6: 12.85 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.04
Forced photometry filter KEPT candidate at 16:42:54.09 -31:11:54.6: ref_mag=12.79 +/- 0.04 new_mean_mag=11.8305 delta=0.96 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:37:14.17 -31:45:27.3: 12.61 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.04
Forced photometry filter KEPT candidate at 16:37:14.17 -31:45:27.3: ref_mag=12.67 +/- 0.04 new_mean_mag=11.6789 delta=0.99 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:53:57.32 -37:32:57.6: 12.46 +/- 0.05 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:53:57.32 -37:32:57.6: 12.50 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.04
Forced photometry filter KEPT candidate at 16:53:57.32 -37:32:57.6: ref_mag=12.47 +/- 0.04 new_mean_mag=11.5143 delta=0.96 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:38:45.04 -37:19:05.7: 12.33 +/- 0.04 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:55:15.10 -30:34:35.0: 12.20 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:38:45.04 -37:19:05.7: 12.24 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.29 +/- 0.03
Forced photometry filter KEPT candidate at 16:38:45.04 -37:19:05.7: ref_mag=12.29 +/- 0.03 new_mean_mag=11.3125 delta=0.98 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:55:15.10 -30:34:35.0: 12.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.03
Forced photometry filter KEPT candidate at 16:55:15.10 -30:34:35.0: ref_mag=12.21 +/- 0.03 new_mean_mag=11.2504 delta=0.96 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:12:49.70 -35:46:51.6: 11.87 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:12:49.70 -35:46:51.6: 11.93 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.89 +/- 0.02
Forced photometry filter REJECTED candidate at 16:12:49.70 -35:46:51.6: ref_mag=11.89 +/- 0.02 new_mean_mag=11.0935 delta=0.79 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:26:47.78 -37:57:49.1: 12.03 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:16:20.92 -36:19:10.3: 12.04 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:20:13.10 -37:20:53.4: 12.06 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:26:47.78 -37:57:49.1: 12.05 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.04 +/- 0.03
Forced photometry filter KEPT candidate at 16:26:47.78 -37:57:49.1: ref_mag=12.04 +/- 0.03 new_mean_mag=11.0185 delta=1.02 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:29:22.94 -37:33:38.8: 11.98 +/- 0.03 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:16:20.92 -36:19:10.3: 11.85 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.96 +/- 0.02
Forced photometry filter KEPT candidate at 16:16:20.92 -36:19:10.3: ref_mag=11.96 +/- 0.02 new_mean_mag=10.7924 delta=1.16 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:20:13.10 -37:20:53.4: 12.09 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.03
Forced photometry filter KEPT candidate at 16:20:13.10 -37:20:53.4: ref_mag=12.07 +/- 0.03 new_mean_mag=11.0733 delta=1.00 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:29:22.94 -37:33:38.8: 12.00 +/- 0.04 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.02
Forced photometry filter KEPT candidate at 16:29:22.94 -37:33:38.8: ref_mag=11.99 +/- 0.02 new_mean_mag=10.9674 delta=1.02 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:50:59.26 -36:22:53.6: 11.80 +/- 0.02 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:37:01.77 -37:29:47.4: 11.82 +/- 0.02 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:37:01.77 -37:29:47.4: 11.97 +/- 0.04 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:50:59.26 -36:22:53.6: 11.73 +/- 0.03 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.02
Forced photometry filter KEPT candidate at 16:37:01.77 -37:29:47.4: ref_mag=11.87 +/- 0.02 new_mean_mag=10.9487 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 11.77 +/- 0.02
Forced photometry filter KEPT candidate at 16:50:59.26 -36:22:53.6: ref_mag=11.77 +/- 0.02 new_mean_mag=10.7583 delta=1.01 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:36:29.39 -36:15:49.1: 11.30 +/- 0.01 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:32:37.24 -37:00:39.5: 11.34 +/- 0.02 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:36:29.39 -36:15:49.1: 11.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.29 +/- 0.01
Forced photometry filter REJECTED candidate at 16:36:29.39 -36:15:49.1: ref_mag=11.29 +/- 0.01 new_mean_mag=10.3957 delta=0.89 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:32:37.24 -37:00:39.5: 11.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.31 +/- 0.01
Forced photometry filter KEPT candidate at 16:32:37.24 -37:00:39.5: ref_mag=11.31 +/- 0.01 new_mean_mag=10.2540 delta=1.05 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:36:40.78 -37:22:39.2: 12.97 +/- 0.08 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-10_04-06-10_20.00sec_-5.00C_LIGHTs_0227.fits at 16:08:28.13 -36:58:53.6: 10.11 +/- 0.01 detection
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:36:40.78 -37:22:39.2: 13.00 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.06
Forced photometry filter KEPT candidate at 16:36:40.78 -37:22:39.2: ref_mag=12.98 +/- 0.06 new_mean_mag=11.8236 delta=1.16 (need > 0.90)
Forced photometry on wcs_Sco-03-Q1b1x1_2026-04-17_03-39-05_20.00sec_-5.00C_LIGHTs_0236.fits at 16:08:28.13 -36:58:53.6: 10.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.09 +/- 0.01
Forced photometry filter KEPT candidate at 16:08:28.13 -36:58:53.6: ref_mag=10.09 +/- 0.01 new_mean_mag=9.0462 delta=1.04 (need > 0.90)
Adding exclusion_list_local.txt__out07784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89406.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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: 8s
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Considering the candidate 112959_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 112959_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:11:03.09 -30:02:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112982_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 112982_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:15:14.42 -30:31:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112983_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 112983_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:52:35.19 -38:28:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112986_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 112986_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
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Considering the candidate 112991_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 112991_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:18:47.52 -28:45:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112992_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 112992_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
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Considering the candidate 113009_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113009_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:49:39.97 -33:41:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113010_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113010_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:17:54.42 -30:11:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113012_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113012_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:05:00.97 -32:59:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113015_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113015_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:54:32.19 -37:06:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113023_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113023_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:12:32.41 -31:38:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113027_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113027_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:07:23.17 -31:43:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113035_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113035_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:28:38.51 -38:18:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113036_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113036_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:06:21.65 -35:48:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113038_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113038_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:07:24.39 -32:35:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113040_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113040_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:58:06.14 -31:04:04.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113041_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113041_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:37:50.72 -34:48:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113043_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113043_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:05:11.55 -29:06:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113045_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113045_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:13:08.09 -35:41:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113046_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113046_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:28:00.19 -30:24:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113049_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113049_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:37:25.06 -36:13:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113051_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113051_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:09:07.13 -31:32:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113054_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113054_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:15:19.63 -29:05:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113055_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113055_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:03:48.68 -32:25:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113056_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113056_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:08:43.40 -35:02:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113058_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113058_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:56:45.58 -32:19:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113060_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113060_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:12:39.05 -29:16:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113061_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113061_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:03:51.83 -37:33:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113063_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113063_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:01:30.70 -31:04:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113064_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113064_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:00:44.45 -36:38:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113065_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113065_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:55:51.10 -37:22:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113073_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113073_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:21:55.62 -35:55:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113074_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113074_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:16:40.94 -29:53:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113085_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113085_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:41:57.11 -32:12:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113086_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113086_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:09:39.64 -35:02:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113087_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113087_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:40:27.12 -34:33:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113088_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113088_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:53:16.90 -29:44:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113095_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113095_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:58:35.84 -31:46:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113098_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113098_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:18:05.38 -35:36:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113103_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 113103_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:42:43.81 -33:54:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30713_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 30713_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:31:03.63 -35:09:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22037_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 22037_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:30:11.36 -36:15:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10911_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 10911_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:46:37.11 -37:54:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12801_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 12801_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 25190_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 25190_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 12448_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 12448_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09949_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 09949_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:37:32.86 -37:54:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22673_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 22673_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 19389_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 19389_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:58:55.86 -36:56:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06778_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 06778_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:43:00.78 -38:22:59.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02166_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 02166_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:29:27.43 -38:46:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35989_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 35989_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:31:53.03 -34:35:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71665_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 71665_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:05:18.58 -31:23:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66446_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 66446_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:31:59.82 -32:46:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111071_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 111071_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:43:57.82 -34:43:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89406_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 89406_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 110174_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 110174_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:47:40.58 -36:07:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28966_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 28966_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:48:15.55 -35:38:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83681_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 83681_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 15700_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 15700_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:20:50.26 -36:48:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51474_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 51474_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:22:25.74 -32:57:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95633_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 95633_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:40:45.08 -31:56:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15246_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 15246_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:18:53.20 -36:49:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20560_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 20560_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:35:29.12 -36:31:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05886_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 05886_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:55:28.42 -38:37:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14050_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 14050_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:24:21.14 -37:07:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18045_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 18045_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:52:15.55 -37:02:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73790_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 73790_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:09:42.74 -32:48:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14302_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 14302_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 21241_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 21241_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:58:10.79 -36:41:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38455_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 38455_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:39:08.41 -34:28:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09874_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 09874_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:33:00.78 -37:50:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04058_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 04058_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:01:33.28 -38:53:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10779_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 10779_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:09:08.64 -37:06:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23355_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 23355_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:44:11.08 -36:18:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14724_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 14724_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 10583_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 10583_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:09:51.71 -37:09:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83454_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 83454_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 18556_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 18556_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:29:55.69 -36:39:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21709_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 21709_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:46:01.24 -36:33:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92808_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 92808_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:07:35.61 -31:49:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10854_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 10854_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 22228_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 22228_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
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Considering the candidate 17440_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 17440_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:48:32.76 -37:06:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19362_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 19362_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:28:04.74 -36:31:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07784_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 07784_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 18565_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 18565_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 09127_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 09127_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:37:36.58 -38:00:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11444_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 11444_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 11407_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 11407_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 22405_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 22405_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:37:33.25 -36:19:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90423_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 90423_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:43:30.32 -31:19:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35419_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 35419_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:32:05.85 -34:39:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12123_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 12123_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:27:21.54 -37:25:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16722_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 16722_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:22:36.54 -36:43:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13105_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 13105_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 23344_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 23344_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 92651_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 92651_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:27:22.24 -31:18:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96687_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 96687_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:55:10.63 -32:16:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12738_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 12738_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:19:09.37 -37:08:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09149_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 09149_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:50:44.50 -38:06:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22618_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 22618_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
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Considering the candidate 16090_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 16090_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 19514_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 19514_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:22:43.55 -36:23:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14009_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 14009_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 86409_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 86409_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:08:20.97 -31:03:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11391_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 11391_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 22718_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 22718_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:37:36.84 -36:17:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71173_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 71173_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:02:38.30 -31:13:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52957_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 52957_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:14:51.29 -33:25:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29999_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 29999_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 17:01:45.01 -35:37:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14181_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 14181_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:47:48.69 -37:30:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03729_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001
The candidate 03729_fd_Sco-03-Q1b1x1_2026-08-06_21-29-51_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
