This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R
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 11.4230 2461324.9230 7.55 01:31:52.03 -03:11:52.9
146.66375 -64.19091 galactic Cet Second-epoch detections are separated by 3.4" 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.4 Vesta 4 3 5 6.5 0 0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:31:52.03 -03:11:52.9: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:31:52.03 -03:11:52.9: 15.91 +/- 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 11.4230* 01 31 52.03 -03 11 52.9 7.5 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,2461324.9230,7.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.4230 7.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4230 2461324.9230 12.78 01:30:59.91 -00:51:00.7
144.43358 -62.05909 galactic Cet Second-epoch detections are separated by 3.1" 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 -1 0 1 12.9 0 0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:30:59.91 -00:51:00.7: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:30:59.91 -00:51:00.7: 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 11.4230* 01 30 59.91 +00 51 00.7 12.8 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
VARIABLE_NAME,2461324.9230,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.4230 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4230 2461324.9230 13.50 01:30:19.08 -04:04:35.6
146.55568 -65.14959 galactic Cet Second-epoch detections are separated by 1.5" and 6.1 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 13.7 0 0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:30:19.08 -04:04:35.6: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:30:19.08 -04:04:35.6: 16.02 +/- 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 11.4230* 01 30 19.08 -04 04 35.6 13.5 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,2461324.9230,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.4230 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4230 2461324.9230 14.15 01:57:18.27 -00:42:43.7
156.55781 -59.21418 galactic Cet Second-epoch detections are separated by 3.2" and 5.4 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 0 0 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 01:57:18.27 -00:42:43.7: 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 01:57:18.27 -00:42:43.7: 16.02 +/- 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 11.4230* 01 57 18.27 +00 42 43.7 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,2461324.9230,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.4230 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4230 2461324.9230 14.21 02:06:49.12 -01:33:04.2
161.33874 -58.68412 galactic Cet Second-epoch detections are separated by 4.4" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.3066 McFadden 3 -0 3 14.0 -0 -0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 02:06:49.12 -01:33:04.2: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 02:06:49.12 -01:33:04.2: 15.88 +/- 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 11.4230* 02 06 49.12 -01 33 04.2 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,2461324.9230,14.21,0.05,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 20261011.4230 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4230 2461324.9230 14.48 01:52:11.09 -05:50:30.8
159.82443 -64.27111 galactic Cet Second-epoch detections are separated by 2.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1702 Kalahari -1 -1 1 14.5 -0 -0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:52:11.09 -05:50:30.8: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:52:11.09 -05:50:30.8: 15.97 +/- 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 11.4230* 01 52 11.09 -05 50 30.8 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,2461324.9230,14.48,0.05,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 20261011.4230 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 11.4230 2461324.9230 14.51 02:10:17.46 -03:05:38.8
164.44026 -59.45372 galactic Cet Second-epoch detections are separated by 4.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1903 Adzhimushkaj 1 -0 1 15.0 0 0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 02:10:17.46 -03:05:38.8: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 02:10:17.46 -03:05:38.8: 15.80 +/- 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 11.4230* 02 10 17.46 -03 05 38.8 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,2461324.9230,14.51,0.05,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 20261011.4230 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 11.4230 2461324.9230 14.79 02:02:59.68 -01:58:36.6
160.23248 -59.56276 galactic Cet Second-epoch detections are separated by 6.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.3225 Hoag 1 -2 2 14.9 -0 0
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 02:02:59.68 -01:58:36.6: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 02:02:59.68 -01:58:36.6: 15.91 +/- 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 11.4230* 02 02 59.68 -01 58 36.6 14.8 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
VARIABLE_NAME,2461324.9230,14.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261011.4230 14.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461324.92431267 11.10.2026 10:10:50.615 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
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): 5704
Objects passed selection criteria: 5698
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 5025
Average stars matched: 4899.5 (97.5025 %)
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 Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 11 05:12:59 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: 2461324.92431267 11.10.2026 10:10:50.615 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 48
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: 11 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): 30361
Objects passed selection criteria: 30308
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 26755
Average stars matched: 25861.5 (96.6604 %)
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 Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 11 05:13:47 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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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: 2461324.92167638
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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits exists and is non-empty
wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits (1st new image)
verification OK: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
Image size: 941.6'x626.9' 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: 01:42:49.131 -01:59:53.99 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 01:42:49.131 -01:59:53.99
Angular distance between the image centers 0.0490 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits (2nd new image)
verification OK: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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: 01:42:48.662 -01:59:20.93 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 01:42:48.662 -01:59:20.93
Angular distance between the image centers 0.0482 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 01:42:49.131 -01:59:53.99
Second-epoch second image center 01:42:48.662 -01:59:20.93
Angular distance between the image centers 0.00939 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.VNdhJIjyNG
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.Z11juax0ye
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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits &> /tmp/tmp.83wjcHStc3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits &> /tmp/tmp.LyFcepJQWD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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
2.5 pix fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
2.7 pix fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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
14.8 mag. fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
14.8 mag. fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.7 (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.VNdhJIjyNG (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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/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.Z11juax0ye (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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/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.83wjcHStc3 (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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.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=315, bad_region=0, passed=4455
Got 4455 stars (including 4138 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat
util/solve_plate_with_UCAC5 got 4455 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 4053 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4050 matched stars entering correct_measured_positions(), 4050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4050 matched stars entering correct_measured_positions(), 4455 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.6)
Done reading UCAC5 zone files...
Matched 4055 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4051 matched stars entering correct_measured_positions(), 4455 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4051 matched stars entering correct_measured_positions(), 4455 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4051 stars left (next iteration limit 4455)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4051 robust_rms=12.405 arcsec worst_region_rms=30.665 arcsec outer_annulus_rms=30.665 arcsec
SIP_REFIT: SIP order 3 trial: matched=4051 robust_rms=0.547 arcsec worst_region_rms=0.700 arcsec outer_annulus_rms=0.700 arcsec
SIP_REFIT: SIP order 5 trial: matched=4051 robust_rms=0.337 arcsec worst_region_rms=0.355 arcsec outer_annulus_rms=0.327 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4051 robust_rms_before=1.144 arcsec robust_rms_before_corrected=0.331 arcsec robust_rms_after=0.337 arcsec worst_region_rms_before=0.362 worst_region_rms_after=0.355 outer_annulus_rms_before=1.400 outer_annulus_rms_after=0.327
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.362 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits worst_region_rms_kept=0.362 arcsec robust_rms_kept=0.331 arcsec matched=4051
WCS_QUALITY_DIAG: file=fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits N_match=4051 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.338 sigma_q3_arcsec=0.327 sigma_q4_arcsec=0.315 n_q1=1005 n_q2=1051 n_q3=1132 n_q4=863 worst_quadrant_to_overall_ratio=1.118
The image catalog is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits -region wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.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.LyFcepJQWD (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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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=224, bad_region=0, passed=4050
Got 4050 stars (including 3824 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat
util/solve_plate_with_UCAC5 got 4050 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 3733 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3729 matched stars entering correct_measured_positions(), 3727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3729 matched stars entering correct_measured_positions(), 4047 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 3735 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3730 matched stars entering correct_measured_positions(), 4047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 3730 matched stars entering correct_measured_positions(), 4047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 3730 stars left (next iteration limit 4101)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3730 robust_rms=12.812 arcsec worst_region_rms=26.016 arcsec outer_annulus_rms=26.016 arcsec
SIP_REFIT: SIP order 3 trial: matched=3730 robust_rms=0.412 arcsec worst_region_rms=0.735 arcsec outer_annulus_rms=0.735 arcsec
SIP_REFIT: SIP order 5 trial: matched=3730 robust_rms=0.270 arcsec worst_region_rms=0.374 arcsec outer_annulus_rms=0.374 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3730 robust_rms_before=1.029 arcsec robust_rms_before_corrected=0.260 arcsec robust_rms_after=0.270 arcsec worst_region_rms_before=0.355 worst_region_rms_after=0.374 outer_annulus_rms_before=1.197 outer_annulus_rms_after=0.374
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.355 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits worst_region_rms_kept=0.355 arcsec robust_rms_kept=0.260 arcsec matched=3730
WCS_QUALITY_DIAG: file=fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits N_match=3730 sigma_overall_arcsec=0.267 sigma_q1_arcsec=0.269 sigma_q2_arcsec=0.294 sigma_q3_arcsec=0.239 sigma_q4_arcsec=0.276 n_q1=1066 n_q2=866 n_q3=941 n_q4=857 worst_quadrant_to_overall_ratio=1.102
The image catalog is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits -region wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits to local_wcs_cache/
'wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits' -> 'local_wcs_cache/wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits'
Saving the final (post-refit) wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits to local_wcs_cache/
'wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits' -> 'local_wcs_cache/wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits sigma_overall=0.340 worst_q_ratio=1.118
new2=fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits sigma_overall=0.267 worst_q_ratio=1.102
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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317_astrometric_residuals.png (4051 matched stars from wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318_astrometric_residuals.png (3730 matched stars from wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits'
Saving fully-calibrated image wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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 01:31:52.03 -03:11:52.9: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:31:52.03 -03:11:52.9: 15.91 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20289.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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20289_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
Preparing report for the candidate 20289_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
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 ####
01:31:52.03 -03:11:52.9
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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits exists and is non-empty
wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits (1st new image)
verification OK: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
Image size: 941.6'x626.9' 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: 01:42:49.131 -01:59:53.99 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 01:42:49.131 -01:59:53.99
Angular distance between the image centers 0.0490 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits (2nd new image)
verification OK: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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: 01:42:48.662 -01:59:20.93 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 01:42:48.662 -01:59:20.93
Angular distance between the image centers 0.0482 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 01:42:49.131 -01:59:53.99
Second-epoch second image center 01:42:48.662 -01:59:20.93
Angular distance between the image centers 0.00939 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.8ce6JyzJ3N
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.ffYcaMFoED
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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits &> /tmp/tmp.cx1OE89eQb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits &> /tmp/tmp.uKZHYrU8Cu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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 35 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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
2.6 pix fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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
15.1 mag. fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
15.0 mag. fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.8ce6JyzJ3N (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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/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.ffYcaMFoED (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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/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.cx1OE89eQb (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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=992, bad_region=44, passed=24033
Got 24033 stars (including 22966 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat
util/solve_plate_with_UCAC5 got 24033 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 4880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 24033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 24033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 24033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4880 stars left (next iteration limit 5368)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.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=4880 robust_rms=12.066 arcsec worst_region_rms=32.646 arcsec outer_annulus_rms=32.646 arcsec
SIP_REFIT: SIP order 3 trial: matched=4880 robust_rms=0.545 arcsec worst_region_rms=0.753 arcsec outer_annulus_rms=0.753 arcsec
SIP_REFIT: SIP order 5 trial: matched=4880 robust_rms=0.339 arcsec worst_region_rms=0.355 arcsec outer_annulus_rms=0.335 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4880 robust_rms_before=1.172 arcsec robust_rms_before_corrected=0.326 arcsec robust_rms_after=0.339 arcsec worst_region_rms_before=0.353 worst_region_rms_after=0.355 outer_annulus_rms_before=1.427 outer_annulus_rms_after=0.335
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.353 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits worst_region_rms_kept=0.353 arcsec robust_rms_kept=0.326 arcsec matched=4880
WCS_QUALITY_DIAG: file=fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits N_match=4880 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.371 sigma_q2_arcsec=0.336 sigma_q3_arcsec=0.329 sigma_q4_arcsec=0.323 n_q1=1226 n_q2=1279 n_q3=1321 n_q4=1054 worst_quadrant_to_overall_ratio=1.090
The image catalog is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits -region wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.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.uKZHYrU8Cu (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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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=10, blended=632, bad_region=40, passed=20412
Got 20412 stars (including 19716 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat
util/solve_plate_with_UCAC5 got 20412 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 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 4861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 20408 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 20408 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 20408 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4865 stars left (next iteration limit 5349)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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=4865 robust_rms=12.607 arcsec worst_region_rms=25.678 arcsec outer_annulus_rms=25.678 arcsec
SIP_REFIT: SIP order 3 trial: matched=4865 robust_rms=0.430 arcsec worst_region_rms=0.762 arcsec outer_annulus_rms=0.762 arcsec
SIP_REFIT: SIP order 5 trial: matched=4865 robust_rms=0.288 arcsec worst_region_rms=0.402 arcsec outer_annulus_rms=0.402 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4865 robust_rms_before=1.039 arcsec robust_rms_before_corrected=0.276 arcsec robust_rms_after=0.288 arcsec worst_region_rms_before=0.390 worst_region_rms_after=0.402 outer_annulus_rms_before=1.204 outer_annulus_rms_after=0.402
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.390 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits worst_region_rms_kept=0.390 arcsec robust_rms_kept=0.276 arcsec matched=4865
WCS_QUALITY_DIAG: file=fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits N_match=4865 sigma_overall_arcsec=0.282 sigma_q1_arcsec=0.276 sigma_q2_arcsec=0.312 sigma_q3_arcsec=0.268 sigma_q4_arcsec=0.283 n_q1=1451 n_q2=1086 n_q3=1247 n_q4=1081 worst_quadrant_to_overall_ratio=1.107
The image catalog is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits -region wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-07-02_20.00sec_-0.00C_LIGHTs_0317.fits
Saving fully-calibrated image wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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_2026-10-11_CI_Cet-03-Q1b1x1_051137_TTUQ1b1x1_783016_wp3ScC1R/wcs_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318.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 01:30:59.91 -00:51:00.7: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:30:19.08 -04:04:35.6: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 02:06:49.12 -01:33:04.2: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:30:59.91 -00:51:00.7: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:52:11.09 -05:50:30.8: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 01:57:18.27 -00:42:43.7: 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 01:57:53.75 -06:10:31.4: 15.18 +/- 0.20 detection
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 02:10:17.46 -03:05:38.8: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:30:19.08 -04:04:35.6: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-05-20_20.00sec_-14.90C_LIGHT_0077.fits at 02:02:59.68 -01:58:36.6: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:57:18.27 -00:42:43.7: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 02:06:49.12 -01:33:04.2: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:52:11.09 -05:50:30.8: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 02:10:17.46 -03:05:38.8: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 01:57:53.75 -06:10:31.4: 15.39 +/- 0.25 detection
Forced photometry on wcs_Cet-03-Q1b1x1_2026-01-08_21-06-09_20.00sec_-14.90C_LIGHT_0078.fits at 02:02:59.68 -01:58:36.6: 15.91 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.26 +/- 0.15
Forced photometry filter REJECTED candidate at 01:57:53.75 -06:10:31.4: ref_mag=15.26 +/- 0.15 new_mean_mag=14.6302 delta=0.63 (need > 0.90)
Adding exclusion_list_local.txt__out52287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53114.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 51972_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 51972_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 51985_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 51985_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
**** FOUND 01:31:52.03 -03:11:52.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52114_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52114_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
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Considering the candidate 52133_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52133_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 52138_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52138_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (29.3") between the two second-epoch detections
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Considering the candidate 52144_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52144_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (27.3") between the two second-epoch detections
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Considering the candidate 52146_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52146_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (29.5") between the two second-epoch detections
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Considering the candidate 52178_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52178_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
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Considering the candidate 52287_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
Preparing report for the candidate 52287_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
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Considering the candidate 52346_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52346_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (28.6") between the two second-epoch detections
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Considering the candidate 52354_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52354_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (29.7") between the two second-epoch detections
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Considering the candidate 52425_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52425_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 52439_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52439_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 52443_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52443_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 52460_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52460_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 52498_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
Preparing report for the candidate 52498_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
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Considering the candidate 52523_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52523_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (29.9") between the two second-epoch detections
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Considering the candidate 52537_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52537_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (27.2") between the two second-epoch detections
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Considering the candidate 52629_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52629_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
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Considering the candidate 52662_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52662_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 52667_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52667_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (28.6") between the two second-epoch detections
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Considering the candidate 52672_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52672_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 52681_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52681_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (28.0") between the two second-epoch detections
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Considering the candidate 52690_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52690_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (28.0") between the two second-epoch detections
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Considering the candidate 52737_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52737_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 52752_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52752_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (27.7") between the two second-epoch detections
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Considering the candidate 52779_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52779_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
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Considering the candidate 52866_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
Preparing report for the candidate 52866_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
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Considering the candidate 52949_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
Preparing report for the candidate 52949_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
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Considering the candidate 52957_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 52957_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
Rejecting candidate due to large distance (30.2") between the two second-epoch detections
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Considering the candidate 52989_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
Preparing report for the candidate 52989_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
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Considering the candidate 53049_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
Preparing report for the candidate 53049_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
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Considering the candidate 53088_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 53088_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
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Considering the candidate 53096_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318
The candidate 53096_fd_Cet-03-Q1b1x1_2026-10-11_05-10-50_20.00sec_-0.00C_LIGHTs_0318 did not pass the final checks
