This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx
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 10 01.4132 2461314.9132 7.92 01:40:59.38 -02:13:08.0
150.50178 -62.40816 galactic Cet Second-epoch detections are separated by 0.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.4 Vesta 1 2 3 6.6 0 0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:40:59.38 -02:13:08.0: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:40:59.38 -02:13:08.0: 15.98 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 01.4132* 01 40 59.38 -02 13 08.0 7.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461314.9132,7.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261001.4132 7.92CV 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 10 01.4132 2461314.9132 12.65 01:14:53.92 -03:13:55.6
137.14898 -65.45422 galactic Cet Second-epoch detections are separated by 0.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.191 Kolga -0 -0 0 12.7 0 0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:14:53.92 -03:13:55.6: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:14:53.92 -03:13:55.6: 15.81 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 01.4132* 01 14 53.92 -03 13 55.6 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461314.9132,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261001.4132 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 01.4132 2461314.9132 12.92 01:38:33.45 +01:06:17.2
146.70145 -59.57473 galactic Cet Second-epoch detections are separated by 0.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.329 Svea -0 0 0 13.1 0 0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:38:33.45 +01:06:17.2: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:38:33.45 +01:06:17.2: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 01.4132* 01 38 33.45 +01 06 17.2 12.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461314.9132,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261001.4132 12.92CV 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 10 01.4132 2461314.9132 13.57 01:36:04.06 -04:52:57.8
150.45618 -65.34136 galactic Cet Second-epoch detections are separated by 1.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.783 Nora -1 -0 1 13.6 -0 -0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:36:04.06 -04:52:57.8: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:36:04.06 -04:52:57.8: 16.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 01.4132* 01 36 04.06 -04 52 57.8 13.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461314.9132,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261001.4132 13.57CV 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 10 01.4132 2461314.9132 13.72 01:37:33.39 -02:53:58.0
149.38523 -63.37748 galactic Cet Second-epoch detections are separated by 0.1" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1689 Floris-Jan -0 0 0 13.8 0 0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:37:33.39 -02:53:58.0: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:37:33.39 -02:53:58.0: 16.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 01.4132* 01 37 33.39 -02 53 58.0 13.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461314.9132,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261001.4132 13.72CV 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 10 01.4132 2461314.9132 13.95 01:13:57.22 +01:10:18.4
134.67164 -61.18571 galactic Cet Second-epoch detections are separated by 0.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.522 Helga -0 0 0 13.8 0 -0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:13:57.22 +01:10:18.4: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:13:57.22 +01:10:18.4: 15.76 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 01.4132* 01 13 57.22 +01 10 18.4 13.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461314.9132,13.95,0.05,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
VARIABLE_NAME 20261001.4132 13.95CV 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 10 01.4132 2461314.9132 14.25 02:04:03.72 +00:07:12.2
158.53816 -57.64191 galactic Cet Second-epoch detections are separated by 0.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.861 Aida 0 1 1 14.3 0 0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 02:04:03.72 +00:07:12.2: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 02:04:03.72 +00:07:12.2: 15.83 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 01.4132* 02 04 03.72 +00 07 12.2 14.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461314.9132,14.25,0.05,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
VARIABLE_NAME 20261001.4132 14.25CV 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 10 01.4132 2461314.9132 14.51 02:12:38.36 +00:44:49.2
161.23438 -55.96465 galactic Cet Second-epoch detections are separated by 1.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.3066 McFadden -0 1 1 14.2 -0 -0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 02:12:38.36 +00:44:49.2: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 02:12:38.36 +00:44:49.2: 15.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 01.4132* 02 12 38.36 +00 44 49.2 14.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461314.9132,14.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261001.4132 14.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 01.4132 2461314.9132 13.78 01:38:32.51 -00:03:43.5
147.54843 -60.66265 galactic Cet Second-epoch detections are separated by 1.0" and 5.5 pix
The object was found in VSX 0" FASTT 47
Type: SRA
# Max. Min./Amp. JD0 Period
13.000 CV 14.400 CV 2453700.00000 169.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:38:32.51 -00:03:43.5: 15.11 +/- 0.14 detection
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:38:32.51 -00:03:43.5: 15.35 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.11
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 01.4132* 01 38 32.51 +00 03 43.5 13.8 U Cet 9 0
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
FASTT 47,2461314.9132,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FASTT 47 20261001.4132 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.62882272 09.01.2026 03:05:20.283 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
First image: 2461049.62882272 09.01.2026 03:05:20.283 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
Last image: 2461314.91352692 01.10.2026 09:55:18.726 /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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): 5776
Objects passed selection criteria: 5771
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 5334.25
Average stars matched: 5204.25 (97.5629 %)
Memory usage VmPeak: 232156 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 25 15:05:03 CDT 2026
VaST build number 1.0rc89-225-g3a72982a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-25)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Oct 1 04:57:57 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: 2461049.62882272 09.01.2026 03:05:20.283 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
First image: 2461049.62882272 09.01.2026 03:05:20.283 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
Last image: 2461314.91352692 01.10.2026 09:55:18.726 /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.17
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: 9 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): 30691
Objects passed selection criteria: 30626
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 28658.2
Average stars matched: 27752.5 (96.8395 %)
Memory usage VmPeak: 253424 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 25 15:05:03 CDT 2026
VaST build number 1.0rc89-225-g3a72982a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-25)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Oct 1 04:58:43 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/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
SExtractor catalog cache: saved Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.cat to cache
SExtractor catalog cache: saved Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.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/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461314.91287012
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits exists and is non-empty
wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits exists and is non-empty
wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits exists and is non-empty
wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits (1st reference image)
verification OK: wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:43:00.023 -01:58:47.42 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_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits (1st new image)
verification OK: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:56.306 -02:01:15.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:43:00.023 -01:58:47.42
Second-epoch image center 01:42:56.306 -02:01:15.53
Angular distance between the image centers 0.0440 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits (2nd new image)
verification OK: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:57.393 -02:00:46.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:43:00.023 -01:58:47.42
Second-epoch image center 01:42:57.393 -02:00:46.27
Angular distance between the image centers 0.0348 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 01:42:56.306 -02:01:15.53
Second-epoch second image center 01:42:57.393 -02:00:46.27
Angular distance between the image centers 0.00930 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/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits &> /tmp/tmp.nMp3hrNA61
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits &> /tmp/tmp.hORm8wS01W
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits &> /tmp/tmp.6P8Hob0G0M
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits &> /tmp/tmp.hk76RAqHbm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.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_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits and wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.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_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits and wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat
Found non-empty wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits and wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat
The reference image (wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits) and catalog (wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat) found
'wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat' -> 'wcsmag.cat'
Read 5890 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.8513 to 33.6869 deg, Dec -7.2828 to +3.3396 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 17.8513 to 33.6869 deg, Dec -7.2828 to 3.3396 deg
Loaded 4101 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): 3360 out of 3515 total matches.
Matched with Tycho-2 3515 out of 5890 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.897750
a=0.000000 b=1.000000 c=22.897750
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5890 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.8513 to 33.6869 deg, Dec -7.2828 to +3.3396 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 17.8513 to 33.6869 deg, Dec -7.2828 to 3.3396 deg
Loaded 4101 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): 3360 out of 3515 total matches.
Matched with Tycho-2 3515 out of 5890 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
Forced-photometry filter: calibrated wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits -> calib.txt_param_ref_wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits (aperture=5.9)
Read 5840 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.8340 to 33.6849 deg, Dec -7.2949 to +3.3140 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 17.8340 to 33.6849 deg, Dec -7.2949 to 3.3140 deg
Loaded 4102 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): 3373 out of 3516 total matches.
Matched with Tycho-2 3516 out of 5840 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
Forced-photometry filter: calibrated wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits -> calib.txt_param_ref_wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
2.0 pix Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
2.2 pix fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
2.2 pix fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Limiting magnitude estimates:
15.5 mag. Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
15.5 mag. Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
15.1 mag. fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
15.1 mag. fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.nMp3hrNA61 (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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits' -> 'wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.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/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
WCS-calibrated image found: wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
Checking if the catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat corresponding to the image wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat corresponding to the image wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
WCS catalog name: wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.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=428, bad_region=0, passed=5890
Got 5890 stars (including 5451 good ones) from the SExtractor catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat
util/solve_plate_with_UCAC5 got 5890 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 4896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 5890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 5890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 5890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4896 stars left (next iteration limit 5385)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits N_match=4896 sigma_overall_arcsec=0.292 sigma_q1_arcsec=0.378 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.264 sigma_q4_arcsec=0.261 n_q1=1255 n_q2=1225 n_q3=1248 n_q4=1168 worst_quadrant_to_overall_ratio=1.293
The image catalog is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits -region wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.hORm8wS01W (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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits' -> 'wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.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/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
WCS_IMAGE_NAME=wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
WCS-calibrated image found: wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
Checking if the catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat corresponding to the image wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits alredy exist and is non-empty...
Catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat corresponding to the image wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
WCS catalog name: wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.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=411, bad_region=0, passed=5840
Got 5840 stars (including 5424 good ones) from the SExtractor catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat
util/solve_plate_with_UCAC5 got 5840 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 4891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 5840 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 5840 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 5840 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4891 stars left (next iteration limit 5380)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits N_match=4891 sigma_overall_arcsec=0.287 sigma_q1_arcsec=0.374 sigma_q2_arcsec=0.283 sigma_q3_arcsec=0.264 sigma_q4_arcsec=0.251 n_q1=1265 n_q2=1219 n_q3=1244 n_q4=1163 worst_quadrant_to_overall_ratio=1.304
The image catalog is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits -region wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.6P8Hob0G0M (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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.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=347, bad_region=0, passed=4901
Got 4901 stars (including 4541 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat
util/solve_plate_with_UCAC5 got 4901 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 411 to 470 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 4440 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4436 matched stars entering correct_measured_positions(), 4436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4436 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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 411 to 470 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 4443 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4438 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4438 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4438 stars left (next iteration limit 4879)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4438 robust_rms=13.738 arcsec worst_region_rms=28.251 arcsec outer_annulus_rms=28.251 arcsec
SIP_REFIT: SIP order 3 trial: matched=4438 robust_rms=0.431 arcsec worst_region_rms=0.691 arcsec outer_annulus_rms=0.691 arcsec
SIP_REFIT: SIP order 5 trial: matched=4438 robust_rms=0.259 arcsec worst_region_rms=0.305 arcsec outer_annulus_rms=0.305 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4438 robust_rms_before=0.981 arcsec robust_rms_before_corrected=0.254 arcsec robust_rms_after=0.259 arcsec worst_region_rms_before=0.300 worst_region_rms_after=0.305 outer_annulus_rms_before=1.152 outer_annulus_rms_after=0.305
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.300 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits worst_region_rms_kept=0.300 arcsec robust_rms_kept=0.254 arcsec matched=4438
WCS_QUALITY_DIAG: file=fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits N_match=4438 sigma_overall_arcsec=0.259 sigma_q1_arcsec=0.271 sigma_q2_arcsec=0.282 sigma_q3_arcsec=0.242 sigma_q4_arcsec=0.252 n_q1=1128 n_q2=1076 n_q3=1156 n_q4=1078 worst_quadrant_to_overall_ratio=1.089
The image catalog is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits -region wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.hk76RAqHbm (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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.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=351, bad_region=0, passed=4847
Got 4847 stars (including 4490 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat
util/solve_plate_with_UCAC5 got 4847 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 411 to 470 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 4392 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4388 matched stars entering correct_measured_positions(), 4388 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4388 matched stars entering correct_measured_positions(), 4847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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 411 to 470 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 4394 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4389 matched stars entering correct_measured_positions(), 4847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4389 matched stars entering correct_measured_positions(), 4847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4389 stars left (next iteration limit 4826)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4389 robust_rms=13.771 arcsec worst_region_rms=28.119 arcsec outer_annulus_rms=28.119 arcsec
SIP_REFIT: SIP order 3 trial: matched=4389 robust_rms=0.458 arcsec worst_region_rms=0.706 arcsec outer_annulus_rms=0.706 arcsec
SIP_REFIT: SIP order 5 trial: matched=4389 robust_rms=0.261 arcsec worst_region_rms=0.291 arcsec outer_annulus_rms=0.291 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4389 robust_rms_before=0.994 arcsec robust_rms_before_corrected=0.260 arcsec robust_rms_after=0.261 arcsec worst_region_rms_before=0.304 worst_region_rms_after=0.291 outer_annulus_rms_before=1.161 outer_annulus_rms_after=0.291
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.304 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits worst_region_rms_kept=0.304 arcsec robust_rms_kept=0.260 arcsec matched=4389
WCS_QUALITY_DIAG: file=fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits N_match=4389 sigma_overall_arcsec=0.263 sigma_q1_arcsec=0.276 sigma_q2_arcsec=0.286 sigma_q3_arcsec=0.242 sigma_q4_arcsec=0.262 n_q1=1109 n_q2=1077 n_q3=1129 n_q4=1074 worst_quadrant_to_overall_ratio=1.088
The image catalog is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits -region wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits to local_wcs_cache/
'wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits' -> 'local_wcs_cache/wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits'
Saving the final (post-refit) wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits to local_wcs_cache/
'wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits' -> 'local_wcs_cache/wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits'
Saving the final (post-refit) wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits to local_wcs_cache/
'wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits' -> 'local_wcs_cache/wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits'
Saving the final (post-refit) wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits to local_wcs_cache/
'wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits' -> 'local_wcs_cache/wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits sigma_overall=0.292 worst_q_ratio=1.293
ref2=Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits sigma_overall=0.287 worst_q_ratio=1.304
new1=fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits sigma_overall=0.259 worst_q_ratio=1.089
new2=fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits sigma_overall=0.263 worst_q_ratio=1.088
reference average sigma_overall=0.2895 worst_q_ratio=1.2985
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077_astrometric_residuals.png (4896 matched stars from wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078_astrometric_residuals.png (4891 matched stars from wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256_astrometric_residuals.png (4438 matched stars from wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257_astrometric_residuals.png (4389 matched stars from wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits'
Saving fully-calibrated image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits'
Preparing the HTML report for the field Cet-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:40:59.38 -02:13:08.0: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:40:59.38 -02:13:08.0: 15.98 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20290.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20290_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
Preparing report for the candidate 20290_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Cet-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 ####
01:40:59.38 -02:13:08.0
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/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
SExtractor catalog cache: saved Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.cat to cache
SExtractor catalog cache: saved Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
Creating symlink local_wcs_cache/wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Checking 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_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits exists and is non-empty
wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits exists and is non-empty
wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits exists and is non-empty
wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits (1st reference image)
verification OK: wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:43:00.023 -01:58:47.42 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_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits (1st new image)
verification OK: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:56.306 -02:01:15.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:43:00.023 -01:58:47.42
Second-epoch image center 01:42:56.306 -02:01:15.53
Angular distance between the image centers 0.0440 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits (2nd new image)
verification OK: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:42:57.393 -02:00:46.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:43:00.023 -01:58:47.42
Second-epoch image center 01:42:57.393 -02:00:46.27
Angular distance between the image centers 0.0348 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 01:42:56.306 -02:01:15.53
Second-epoch second image center 01:42:57.393 -02:00:46.27
Angular distance between the image centers 0.00930 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/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits &> /tmp/tmp.ap0MnOSrNv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits &> /tmp/tmp.JFWbBquoWi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits &> /tmp/tmp.hi7TlRiLkY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits &> /tmp/tmp.uOG63MNrtI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.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_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits and wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.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_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits and wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat
Found non-empty wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits and wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat
The reference image (wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits) and catalog (wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat) found
'wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat' -> 'wcsmag.cat'
Read 31778 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.8476 to 33.6869 deg, Dec -7.2828 to +3.3396 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 17.8476 to 33.6869 deg, Dec -7.2828 to 3.3396 deg
Loaded 4102 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): 3266 out of 3563 total matches.
Matched with Tycho-2 3563 out of 31778 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.795000
a=0.000000 b=1.000000 c=22.795000
From vast_summary.log: estimated ref. image limiting mag.: -7.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.63
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.63
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31778 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.8476 to 33.6869 deg, Dec -7.2828 to +3.3396 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 17.8476 to 33.6869 deg, Dec -7.2828 to 3.3396 deg
Loaded 4102 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): 3266 out of 3563 total matches.
Matched with Tycho-2 3563 out of 31778 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
Forced-photometry filter: calibrated wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits -> calib.txt_param_ref_wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits (aperture=4.7)
Read 31614 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 17.8341 to 33.6849 deg, Dec -7.2951 to +3.3303 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 17.8341 to 33.6849 deg, Dec -7.2951 to 3.3303 deg
Loaded 4106 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): 3278 out of 3571 total matches.
Matched with Tycho-2 3571 out of 31614 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
Forced-photometry filter: calibrated wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits -> calib.txt_param_ref_wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 18 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
1.9 pix Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
2.2 pix fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
2.1 pix fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Limiting magnitude estimates:
15.6 mag. Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
15.6 mag. Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
15.2 mag. fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
15.2 mag. fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ap0MnOSrNv (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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits' -> 'wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.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/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
WCS-calibrated image found: wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
Checking if the catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat corresponding to the image wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat corresponding to the image wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits
WCS catalog name: wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1245, bad_region=1, passed=31770
Got 31770 stars (including 30476 good ones) from the SExtractor catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat
util/solve_plate_with_UCAC5 got 31770 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 4900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 31770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 31770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 31770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4900 stars left (next iteration limit 5390)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits N_match=4900 sigma_overall_arcsec=0.289 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.265 sigma_q4_arcsec=0.253 n_q1=1275 n_q2=1207 n_q3=1258 n_q4=1160 worst_quadrant_to_overall_ratio=1.262
The image catalog is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits -region wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.JFWbBquoWi (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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits' -> 'wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.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/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
WCS_IMAGE_NAME=wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
WCS-calibrated image found: wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
Checking if the catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat corresponding to the image wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits alredy exist and is non-empty...
Catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat corresponding to the image wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits
WCS catalog name: wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.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=14, blended=1210, bad_region=3, passed=31600
Got 31600 stars (including 30334 good ones) from the SExtractor catalog wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat
util/solve_plate_with_UCAC5 got 31600 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 413 to 468 (Dec -7.3 to 3.3)
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: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 31600 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 31600 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 31600 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4901 stars left (next iteration limit 5391)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits N_match=4901 sigma_overall_arcsec=0.284 sigma_q1_arcsec=0.354 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.260 sigma_q4_arcsec=0.255 n_q1=1283 n_q2=1199 n_q3=1263 n_q4=1156 worst_quadrant_to_overall_ratio=1.247
The image catalog is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits -region wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.hi7TlRiLkY (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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.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=9, blended=876, bad_region=42, passed=25918
Got 25918 stars (including 24963 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat
util/solve_plate_with_UCAC5 got 25918 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 4887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 25918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 25918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 25918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4887 stars left (next iteration limit 5375)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4887 robust_rms=13.492 arcsec worst_region_rms=28.603 arcsec outer_annulus_rms=28.603 arcsec
SIP_REFIT: SIP order 3 trial: matched=4887 robust_rms=0.426 arcsec worst_region_rms=0.736 arcsec outer_annulus_rms=0.736 arcsec
SIP_REFIT: SIP order 5 trial: matched=4887 robust_rms=0.259 arcsec worst_region_rms=0.310 arcsec outer_annulus_rms=0.310 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4887 robust_rms_before=0.975 arcsec robust_rms_before_corrected=0.254 arcsec robust_rms_after=0.259 arcsec worst_region_rms_before=0.312 worst_region_rms_after=0.310 outer_annulus_rms_before=1.143 outer_annulus_rms_after=0.310
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.312 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits worst_region_rms_kept=0.312 arcsec robust_rms_kept=0.254 arcsec matched=4887
WCS_QUALITY_DIAG: file=fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits N_match=4887 sigma_overall_arcsec=0.262 sigma_q1_arcsec=0.275 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.243 sigma_q4_arcsec=0.256 n_q1=1319 n_q2=1174 n_q3=1268 n_q4=1126 worst_quadrant_to_overall_ratio=1.083
The image catalog is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits -region wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.uOG63MNrtI (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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=880, bad_region=42, passed=26077
Got 26077 stars (including 25116 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat
util/solve_plate_with_UCAC5 got 26077 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 4887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 26077 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 26077 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 26077 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4887 stars left (next iteration limit 5375)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4887 robust_rms=13.600 arcsec worst_region_rms=28.795 arcsec outer_annulus_rms=28.795 arcsec
SIP_REFIT: SIP order 3 trial: matched=4887 robust_rms=0.458 arcsec worst_region_rms=0.738 arcsec outer_annulus_rms=0.738 arcsec
SIP_REFIT: SIP order 5 trial: matched=4887 robust_rms=0.260 arcsec worst_region_rms=0.296 arcsec outer_annulus_rms=0.296 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4887 robust_rms_before=0.989 arcsec robust_rms_before_corrected=0.256 arcsec robust_rms_after=0.260 arcsec worst_region_rms_before=0.308 worst_region_rms_after=0.296 outer_annulus_rms_before=1.149 outer_annulus_rms_after=0.296
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.308 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits worst_region_rms_kept=0.308 arcsec robust_rms_kept=0.256 arcsec matched=4887
WCS_QUALITY_DIAG: file=fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits N_match=4887 sigma_overall_arcsec=0.259 sigma_q1_arcsec=0.271 sigma_q2_arcsec=0.287 sigma_q3_arcsec=0.236 sigma_q4_arcsec=0.258 n_q1=1322 n_q2=1171 n_q3=1258 n_q4=1136 worst_quadrant_to_overall_ratio=1.109
The image catalog is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits -region wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-54-21_20.00sec_-0.00C_LIGHTs_0256.fits
Saving fully-calibrated image wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.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_2026-10-01_CI_Cet-03-Q1b1x1_045631_TTUQ1b1x1_393375_bzH8hTIx/wcs_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257.fits
Preparing the HTML report for the field Cet-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:37:33.39 -02:53:58.0: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:43:45.08 +00:54:36.6: 11.50 +/- 0.01 detection
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:13:57.22 +01:10:18.4: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:30:58.73 +00:53:25.8: 12.66 +/- 0.02 detection
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:38:33.45 +01:06:17.2: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:14:53.92 -03:13:55.6: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:36:04.06 -04:52:57.8: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 02:04:03.72 +00:07:12.2: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 02:12:38.36 +00:44:49.2: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:38:33.45 +01:06:17.2: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:30:58.73 +00:53:25.8: 12.60 +/- 0.02 detection
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:43:45.08 +00:54:36.6: 11.46 +/- 0.01 detection
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:14:53.92 -03:13:55.6: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:13:57.22 +01:10:18.4: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:37:33.39 -02:53:58.0: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:36:04.06 -04:52:57.8: 16.05 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry reference-image weighted average: 11.48 +/- 0.00
Forced photometry filter REJECTED candidate at 01:30:58.73 +00:53:25.8: ref_mag=12.63 +/- 0.01 new_mean_mag=12.8014 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:43:45.08 +00:54:36.6: ref_mag=11.48 +/- 0.00 new_mean_mag=11.6264 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 02:04:03.72 +00:07:12.2: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 02:12:38.36 +00:44:49.2: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:38:32.51 -00:03:43.5: 15.11 +/- 0.14 detection
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:38:32.51 -00:03:43.5: 15.35 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.11
Forced photometry filter KEPT candidate at 01:38:32.51 -00:03:43.5: ref_mag=15.21 +/- 0.11 new_mean_mag=13.7740 delta=1.43 (need > 0.90)
Adding exclusion_list_local.txt__out10485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52981.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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: 5s
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Considering the candidate 52093_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
The candidate 52093_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257 did not pass the final checks
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Considering the candidate 52128_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
The candidate 52128_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257 did not pass the final checks
**** FOUND 01:38:24.96 +02:35:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52252_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
Preparing report for the candidate 52252_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
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Considering the candidate 52289_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
The candidate 52289_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257 did not pass the final checks
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Considering the candidate 52319_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
Preparing report for the candidate 52319_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
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Considering the candidate 52546_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
Preparing report for the candidate 52546_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
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Considering the candidate 52563_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
The candidate 52563_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257 did not pass the final checks
**** FOUND 01:30:27.31 +02:57:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52607_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
Preparing report for the candidate 52607_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
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Considering the candidate 52646_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
The candidate 52646_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257 did not pass the final checks
**** FOUND 01:45:05.06 +02:28:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52724_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
Preparing report for the candidate 52724_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
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Considering the candidate 52768_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
The candidate 52768_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257 did not pass the final checks
**** FOUND 01:32:56.21 +00:06:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52806_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
Preparing report for the candidate 52806_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
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Considering the candidate 52981_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
Preparing report for the candidate 52981_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
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Considering the candidate 53017_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
The candidate 53017_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
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Considering the candidate 17515_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
The candidate 17515_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257 did not pass the final checks
**** FOUND 01:40:59.38 -02:13:08.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 13319_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
The candidate 13319_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257 did not pass the final checks
Rejecting candidate due to large distance (33.3") between the two second-epoch detections
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Considering the candidate 10485_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
Preparing report for the candidate 10485_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
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Considering the candidate 03135_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257
The candidate 03135_fd_Cet-03-Q1b1x1_2026-10-01_04-55-18_20.00sec_-0.00C_LIGHTs_0257 did not pass the final checks
