This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld
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 10.3503 2461323.8503 12.69 02:49:10.10 +17:42:24.1
158.73448 -36.84953 galactic Ari Second-epoch detections are separated by 0.5" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.419 Aurelia -0 0 0 12.8 -0 -0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:49:10.10 +17:42:24.1: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:49:10.10 +17:42:24.1: 16.11 +/- 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 10.3504* 02 49 10.10 +17 42 24.1 12.7 U Ari 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,2461323.8503,12.69,0.05,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 20261010.3503 12.69CV 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 10.3503 2461323.8503 13.30 03:01:59.79 +15:44:52.9
163.27817 -36.69482 galactic Ari Second-epoch detections are separated by 0.4" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.149 Medusa -0 -0 0 13.1 0 0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:01:59.79 +15:44:52.9: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:01:59.79 +15:44:52.9: 16.06 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 10.3504* 03 01 59.79 +15 44 52.9 13.3 U Ari 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,2461323.8503,13.30,0.05,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 20261010.3503 13.30CV 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 10.3503 2461323.8503 13.45 02:24:49.31 +14:03:13.2
154.63988 -42.99536 galactic Ari Second-epoch detections are separated by 0.8" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.257 Silesia 0 0 0 13.8 -0 -0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:24:49.31 +14:03:13.2: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:24:49.31 +14:03:13.2: 16.19 +/- 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 10.3504* 02 24 49.31 +14 03 13.2 13.4 U Ari 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,2461323.8503,13.45,0.05,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 20261010.3503 13.45CV 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 10.3503 2461323.8503 13.99 02:46:53.36 +13:04:55.7
161.46418 -40.99490 galactic Ari Second-epoch detections are separated by 0.3" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1621 Druzhba -1 0 1 14.2 0 0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:46:53.36 +13:04:55.7: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:46:53.36 +13:04:55.7: 16.25 +/- 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 10.3504* 02 46 53.36 +13 04 55.7 14.0 U Ari 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,2461323.8503,13.99,0.05,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 20261010.3503 13.99CV 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 10.3503 2461323.8503 13.97 02:46:29.29 +15:36:15.0
159.51612 -38.95960 galactic Ari Second-epoch detections are separated by 1.6" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.494 Virtus -0 -0 0 14.1 -0 -0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:46:29.29 +15:36:15.0: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:46:29.29 +15:36:15.0: 16.24 +/- 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 10.3504* 02 46 29.29 +15 36 15.0 14.0 U Ari 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,2461323.8503,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261010.3503 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 10.3503 2461323.8503 14.01 02:24:18.56 +10:19:42.3
157.07874 -46.29473 galactic Cet Second-epoch detections are separated by 1.1" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.99 Dike -0 -0 0 14.1 0 -0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:24:18.56 +10:19:42.3: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:24:18.56 +10:19:42.3: 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 10.3504* 02 24 18.56 +10 19 42.3 14.0 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,2461323.8503,14.01,0.05,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 20261010.3503 14.01CV 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 10.3503 2461323.8503 14.16 02:33:28.00 +18:50:27.2
153.98331 -37.80294 galactic Ari Second-epoch detections are separated by 1.8" and 10.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.248 Lameia 0 0 0 14.1 -0 0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:33:28.00 +18:50:27.2: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:33:28.00 +18:50:27.2: 16.00 +/- 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 10.3504* 02 33 28.00 +18 50 27.2 14.2 U Ari 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,2461323.8503,14.16,0.05,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 20261010.3503 14.16CV 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 10.3503 2461323.8503 14.71 02:55:30.72 +15:10:31.4
162.11710 -38.07982 galactic Ari Second-epoch detections are separated by 0.5" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.936 Kunigunde -1 1 1 15.1 -0 0
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:55:30.72 +15:10:31.4: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:55:30.72 +15:10:31.4: 16.14 +/- 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 10.3504* 02 55 30.72 +15 10 31.4 14.7 U Ari 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,2461323.8503,14.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261010.3503 14.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.65708573 09.01.2026 03:46:02.207 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
First image: 2461049.65708573 09.01.2026 03:46:02.207 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Last image: 2461323.85069181 10.10.2026 08:24:49.772 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
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): 7820
Objects passed selection criteria: 7814
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 7446.25
Average stars matched: 7184.25 (96.4815 %)
Memory usage VmPeak: 234128 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 Sat Oct 10 04:40:30 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: 2461049.65708573 09.01.2026 03:46:02.207 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
First image: 2461049.65708573 09.01.2026 03:46:02.207 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Last image: 2461323.85069181 10.10.2026 08:24:49.772 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 62
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.07
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: 15 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): 42738
Objects passed selection criteria: 42650
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 41112.2
Average stars matched: 39372 (95.7671 %)
Memory usage VmPeak: 262688 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 Sat Oct 10 04:41:27 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/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
SExtractor catalog cache: saved Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.cat to cache
SExtractor catalog cache: saved Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.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: 2461323.84999888
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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits exists and is non-empty
wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits exists and is non-empty
wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits exists and is non-empty
wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits (1st reference image)
verification OK: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Image size: 941.6'x627.0' 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: 02:40:00.532 +13:59:54.76 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_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits (1st new image)
verification OK: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
Image size: 941.3'x626.7' 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: 02:40:05.922 +14:02:35.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:40:00.532 +13:59:54.76
Second-epoch image center 02:40:05.922 +14:02:35.49
Angular distance between the image centers 0.0497 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits (2nd new image)
verification OK: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
Image size: 941.3'x626.7' 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: 02:40:08.858 +14:01:55.03 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:40:00.532 +13:59:54.76
Second-epoch image center 02:40:08.858 +14:01:55.03
Angular distance between the image centers 0.0474 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 02:40:05.922 +14:02:35.49
Second-epoch second image center 02:40:08.858 +14:01:55.03
Angular distance between the image centers 0.01634 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/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits &> /tmp/tmp.6G6Ow1f1Zx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits &> /tmp/tmp.6KtBmj21ZD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits &> /tmp/tmp.gsCKYF9bJn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits &> /tmp/tmp.orGiQdNQCi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits and wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits and wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat
Found non-empty wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits and wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat
The reference image (wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits) and catalog (wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat) found
'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat' -> 'wcsmag.cat'
Read 7398 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 31.7516 to 48.3015 deg, Dec +8.6571 to +19.2857 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 31.7516 to 48.3015 deg, Dec 8.6571 to 19.2857 deg
Loaded 4349 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): 3551 out of 3736 total matches.
Matched with Tycho-2 3736 out of 7398 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.949700
a=0.000000 b=1.000000 c=22.949700
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7398 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 31.7516 to 48.3015 deg, Dec +8.6571 to +19.2857 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 31.7516 to 48.3015 deg, Dec 8.6571 to 19.2857 deg
Loaded 4349 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): 3551 out of 3736 total matches.
Matched with Tycho-2 3736 out of 7398 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Forced-photometry filter: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits -> calib.txt_param_ref_wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits (aperture=6.1)
Read 7374 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 31.7516 to 48.3014 deg, Dec +8.6570 to +19.2905 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 31.7516 to 48.3014 deg, Dec 8.6570 to 19.2905 deg
Loaded 4352 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): 3558 out of 3742 total matches.
Matched with Tycho-2 3742 out of 7374 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
Forced-photometry filter: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits -> calib.txt_param_ref_wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
2.0 pix Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
2.5 pix fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
2.5 pix fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
Limiting magnitude estimates:
15.6 mag. Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
15.6 mag. Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
15.6 mag. fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
15.6 mag. fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
All-image limiting magnitude estimate: 15.6 (SNR ) 12.3 (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.6G6Ow1f1Zx (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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits' -> 'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
WCS_IMAGE_NAME=wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
WCS-calibrated image found: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Checking if the catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits alredy exist and is non-empty...
Catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
WCS catalog name: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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=508, bad_region=0, passed=7398
Got 7398 stars (including 6885 good ones) from the SExtractor catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat
util/solve_plate_with_UCAC5 got 7398 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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 4882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 7398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 7398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 7398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4882 stars left (next iteration limit 5370)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits N_match=4882 sigma_overall_arcsec=0.258 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.253 sigma_q3_arcsec=0.237 sigma_q4_arcsec=0.213 n_q1=1360 n_q2=1218 n_q3=1081 n_q4=1223 worst_quadrant_to_overall_ratio=1.288
The image catalog is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits -region wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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.6KtBmj21ZD (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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits' -> 'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
WCS_IMAGE_NAME=wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
WCS-calibrated image found: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
Checking if the catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits alredy exist and is non-empty...
Catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
WCS catalog name: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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=503, bad_region=0, passed=7374
Got 7374 stars (including 6862 good ones) from the SExtractor catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat
util/solve_plate_with_UCAC5 got 7374 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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 4887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 7374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 7374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 7374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4887 stars left (next iteration limit 5375)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits N_match=4887 sigma_overall_arcsec=0.272 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.261 sigma_q3_arcsec=0.250 sigma_q4_arcsec=0.233 n_q1=1370 n_q2=1212 n_q3=1075 n_q4=1230 worst_quadrant_to_overall_ratio=1.256
The image catalog is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits -region wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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.gsCKYF9bJn (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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
WCS_IMAGE_NAME=wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
WCS-calibrated image found: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
Checking if the catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
WCS catalog name: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.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=423, bad_region=0, passed=7576
Got 7576 stars (including 7141 good ones) from the SExtractor catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat
util/solve_plate_with_UCAC5 got 7576 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 491 to 549 (Dec 8.3 to 19.6)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 4877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 7576 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 491 to 549 (Dec 8.3 to 19.6)
Done reading UCAC5 zone files...
Matched 4886 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 7576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4877 matched stars entering correct_measured_positions(), 7576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4877 stars left (next iteration limit 5364)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4877 robust_rms=13.002 arcsec worst_region_rms=29.253 arcsec outer_annulus_rms=29.253 arcsec
SIP_REFIT: SIP order 3 trial: matched=4877 robust_rms=0.416 arcsec worst_region_rms=0.817 arcsec outer_annulus_rms=0.817 arcsec
SIP_REFIT: SIP order 5 trial: matched=4877 robust_rms=0.259 arcsec worst_region_rms=0.297 arcsec outer_annulus_rms=0.297 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4877 robust_rms_before=0.983 arcsec robust_rms_before_corrected=0.254 arcsec robust_rms_after=0.259 arcsec worst_region_rms_before=0.324 worst_region_rms_after=0.297 outer_annulus_rms_before=1.187 outer_annulus_rms_after=0.297
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.324 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits worst_region_rms_kept=0.324 arcsec robust_rms_kept=0.254 arcsec matched=4877
WCS_QUALITY_DIAG: file=fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits N_match=4877 sigma_overall_arcsec=0.265 sigma_q1_arcsec=0.291 sigma_q2_arcsec=0.291 sigma_q3_arcsec=0.242 sigma_q4_arcsec=0.245 n_q1=1374 n_q2=1197 n_q3=1093 n_q4=1213 worst_quadrant_to_overall_ratio=1.097
The image catalog is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits -region wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.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.orGiQdNQCi (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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
WCS_IMAGE_NAME=wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
WCS-calibrated image found: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
Checking if the catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
WCS catalog name: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.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=426, bad_region=0, passed=7608
Got 7608 stars (including 7170 good ones) from the SExtractor catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat
util/solve_plate_with_UCAC5 got 7608 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 491 to 549 (Dec 8.3 to 19.6)
Done reading UCAC5 zone files...
Matched 4888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 4879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 7608 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 491 to 549 (Dec 8.3 to 19.6)
Done reading UCAC5 zone files...
Matched 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 7608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 7608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4879 stars left (next iteration limit 5366)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4879 robust_rms=13.007 arcsec worst_region_rms=29.018 arcsec outer_annulus_rms=29.018 arcsec
SIP_REFIT: SIP order 3 trial: matched=4879 robust_rms=0.413 arcsec worst_region_rms=0.768 arcsec outer_annulus_rms=0.768 arcsec
SIP_REFIT: SIP order 5 trial: matched=4879 robust_rms=0.249 arcsec worst_region_rms=0.304 arcsec outer_annulus_rms=0.304 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4879 robust_rms_before=0.974 arcsec robust_rms_before_corrected=0.251 arcsec robust_rms_after=0.249 arcsec worst_region_rms_before=0.321 worst_region_rms_after=0.304 outer_annulus_rms_before=1.130 outer_annulus_rms_after=0.304
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.321 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits worst_region_rms_kept=0.321 arcsec robust_rms_kept=0.251 arcsec matched=4879
WCS_QUALITY_DIAG: file=fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits N_match=4879 sigma_overall_arcsec=0.259 sigma_q1_arcsec=0.281 sigma_q2_arcsec=0.279 sigma_q3_arcsec=0.238 sigma_q4_arcsec=0.239 n_q1=1384 n_q2=1194 n_q3=1089 n_q4=1212 worst_quadrant_to_overall_ratio=1.083
The image catalog is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits -region wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits to local_wcs_cache/
'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits' -> 'local_wcs_cache/wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits'
Saving the final (post-refit) wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits to local_wcs_cache/
'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits' -> 'local_wcs_cache/wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits'
Saving the final (post-refit) wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits to local_wcs_cache/
'wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits' -> 'local_wcs_cache/wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits'
Saving the final (post-refit) wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits to local_wcs_cache/
'wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits' -> 'local_wcs_cache/wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits sigma_overall=0.258 worst_q_ratio=1.288
ref2=Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits sigma_overall=0.272 worst_q_ratio=1.256
new1=fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits sigma_overall=0.265 worst_q_ratio=1.097
new2=fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits sigma_overall=0.259 worst_q_ratio=1.083
reference average sigma_overall=0.265 worst_q_ratio=1.272
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117_astrometric_residuals.png (4882 matched stars from wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118_astrometric_residuals.png (4887 matched stars from wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428_astrometric_residuals.png (4877 matched stars from wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429_astrometric_residuals.png (4879 matched stars from wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits'
Saving fully-calibrated image wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits'
Preparing the HTML report for the field Ari-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:35:24.22 +14:00:37.2: 12.49 +/- 0.01 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:45:05.29 +14:28:38.5: 12.52 +/- 0.01 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:35:24.22 +14:00:37.2: 12.49 +/- 0.01 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:45:05.29 +14:28:38.5: 12.49 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 02:35:24.22 +14:00:37.2: ref_mag=12.49 +/- 0.01 new_mean_mag=12.4490 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter REJECTED candidate at 02:45:05.29 +14:28:38.5: ref_mag=12.50 +/- 0.01 new_mean_mag=12.4753 delta=0.03 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20498_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 20498_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20499_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 20499_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05052_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 05052_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
**** FOUND 02:44:45.56 +12:19:01.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Ari-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
SExtractor catalog cache: saved Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.cat to cache
SExtractor catalog cache: saved Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Creating symlink local_wcs_cache/wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits exists and is non-empty
wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits exists and is non-empty
wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits exists and is non-empty
wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits (1st reference image)
verification OK: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Image size: 941.6'x627.0' 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: 02:40:00.532 +13:59:54.76 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_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits (1st new image)
verification OK: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
Image size: 941.3'x626.7' 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: 02:40:05.922 +14:02:35.49 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:40:00.532 +13:59:54.76
Second-epoch image center 02:40:05.922 +14:02:35.49
Angular distance between the image centers 0.0497 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits (2nd new image)
verification OK: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
Image size: 941.3'x626.7' 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: 02:40:08.858 +14:01:55.03 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:40:00.532 +13:59:54.76
Second-epoch image center 02:40:08.858 +14:01:55.03
Angular distance between the image centers 0.0474 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 02:40:05.922 +14:02:35.49
Second-epoch second image center 02:40:08.858 +14:01:55.03
Angular distance between the image centers 0.01634 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/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits &> /tmp/tmp.8JwwYRIIod
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits &> /tmp/tmp.eXDRvZN1Zz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits &> /tmp/tmp.Ijil40ehDD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits &> /tmp/tmp.zDiRcm5O5h
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits and wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits and wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat
Found non-empty wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits and wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat
The reference image (wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits) and catalog (wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat) found
'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat' -> 'wcsmag.cat'
Read 42040 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 31.7291 to 48.3263 deg, Dec +8.6136 to +19.2864 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 31.7291 to 48.3263 deg, Dec 8.6136 to 19.2864 deg
Loaded 4379 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): 3380 out of 3762 total matches.
Matched with Tycho-2 3762 out of 42040 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.840350
a=0.000000 b=1.000000 c=22.840350
From vast_summary.log: estimated ref. image limiting mag.: -7.07
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.77
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.77
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 42040 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 31.7291 to 48.3263 deg, Dec +8.6136 to +19.2864 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 31.7291 to 48.3263 deg, Dec 8.6136 to 19.2864 deg
Loaded 4379 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): 3380 out of 3762 total matches.
Matched with Tycho-2 3762 out of 42040 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Forced-photometry filter: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits -> calib.txt_param_ref_wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits (aperture=4.8)
Read 42245 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 31.7296 to 48.3258 deg, Dec +8.6525 to +19.2994 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 31.7296 to 48.3258 deg, Dec 8.6525 to 19.2994 deg
Loaded 4373 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): 3358 out of 3765 total matches.
Matched with Tycho-2 3765 out of 42245 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
Forced-photometry filter: calibrated wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits -> calib.txt_param_ref_wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 55 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
1.9 pix Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
2.4 pix fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
2.4 pix fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
Limiting magnitude estimates:
15.8 mag. Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
15.8 mag. Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
15.7 mag. fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
15.7 mag. fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
All-image limiting magnitude estimate: 15.7 (SNR ) 14.8 (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.8JwwYRIIod (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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits' -> 'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
WCS_IMAGE_NAME=wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
WCS-calibrated image found: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
Checking if the catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits alredy exist and is non-empty...
Catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits
WCS catalog name: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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=13, blended=1797, bad_region=5, passed=42027
Got 42027 stars (including 40158 good ones) from the SExtractor catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat
util/solve_plate_with_UCAC5 got 42027 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4894 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: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 42027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4894 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(), 42027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 42027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4891 stars left (next iteration limit 5380)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits N_match=4891 sigma_overall_arcsec=0.248 sigma_q1_arcsec=0.313 sigma_q2_arcsec=0.247 sigma_q3_arcsec=0.228 sigma_q4_arcsec=0.214 n_q1=1345 n_q2=1226 n_q3=1098 n_q4=1222 worst_quadrant_to_overall_ratio=1.263
The image catalog is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits -region wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.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.eXDRvZN1Zz (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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits' -> 'wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
WCS_IMAGE_NAME=wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
WCS-calibrated image found: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
Checking if the catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits alredy exist and is non-empty...
Catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat corresponding to the image wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits
WCS catalog name: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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=1828, bad_region=7, passed=42231
Got 42231 stars (including 40335 good ones) from the SExtractor catalog wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat
util/solve_plate_with_UCAC5 got 42231 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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 4890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 42231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 42231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 42231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4890 stars left (next iteration limit 5379)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits N_match=4890 sigma_overall_arcsec=0.262 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.250 sigma_q3_arcsec=0.246 sigma_q4_arcsec=0.224 n_q1=1345 n_q2=1220 n_q3=1098 n_q4=1227 worst_quadrant_to_overall_ratio=1.269
The image catalog is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits -region wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.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.Ijil40ehDD (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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
WCS_IMAGE_NAME=wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
WCS-calibrated image found: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
Checking if the catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
WCS catalog name: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.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=1538, bad_region=44, passed=40585
Got 40585 stars (including 38935 good ones) from the SExtractor catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat
util/solve_plate_with_UCAC5 got 40585 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 491 to 549 (Dec 8.3 to 19.6)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 4872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 40585 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 491 to 549 (Dec 8.3 to 19.6)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 40585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4872 matched stars entering correct_measured_positions(), 40585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4872 stars left (next iteration limit 5359)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.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=4872 robust_rms=13.098 arcsec worst_region_rms=29.074 arcsec outer_annulus_rms=29.074 arcsec
SIP_REFIT: SIP order 3 trial: matched=4872 robust_rms=0.421 arcsec worst_region_rms=0.773 arcsec outer_annulus_rms=0.773 arcsec
SIP_REFIT: SIP order 5 trial: matched=4872 robust_rms=0.255 arcsec worst_region_rms=0.302 arcsec outer_annulus_rms=0.302 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4872 robust_rms_before=0.988 arcsec robust_rms_before_corrected=0.250 arcsec robust_rms_after=0.255 arcsec worst_region_rms_before=0.325 worst_region_rms_after=0.302 outer_annulus_rms_before=1.183 outer_annulus_rms_after=0.302
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.325 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits worst_region_rms_kept=0.325 arcsec robust_rms_kept=0.250 arcsec matched=4872
WCS_QUALITY_DIAG: file=fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits N_match=4872 sigma_overall_arcsec=0.258 sigma_q1_arcsec=0.278 sigma_q2_arcsec=0.284 sigma_q3_arcsec=0.234 sigma_q4_arcsec=0.237 n_q1=1385 n_q2=1185 n_q3=1108 n_q4=1194 worst_quadrant_to_overall_ratio=1.099
The image catalog is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits -region wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.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.zDiRcm5O5h (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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
WCS_IMAGE_NAME=wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
WCS-calibrated image found: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
Checking if the catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
WCS catalog name: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.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=1464, bad_region=48, passed=40647
Got 40647 stars (including 39076 good ones) from the SExtractor catalog wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat
util/solve_plate_with_UCAC5 got 40647 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 491 to 549 (Dec 8.3 to 19.6)
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: 4875 matched stars entering correct_measured_positions(), 4875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 40647 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 491 to 549 (Dec 8.3 to 19.6)
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: 4875 matched stars entering correct_measured_positions(), 40647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 40647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4875 stars left (next iteration limit 5362)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.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=4875 robust_rms=13.143 arcsec worst_region_rms=28.561 arcsec outer_annulus_rms=28.561 arcsec
SIP_REFIT: SIP order 3 trial: matched=4875 robust_rms=0.416 arcsec worst_region_rms=0.734 arcsec outer_annulus_rms=0.734 arcsec
SIP_REFIT: SIP order 5 trial: matched=4875 robust_rms=0.247 arcsec worst_region_rms=0.298 arcsec outer_annulus_rms=0.298 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4875 robust_rms_before=0.976 arcsec robust_rms_before_corrected=0.247 arcsec robust_rms_after=0.247 arcsec worst_region_rms_before=0.318 worst_region_rms_after=0.298 outer_annulus_rms_before=1.121 outer_annulus_rms_after=0.298
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.318 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits worst_region_rms_kept=0.318 arcsec robust_rms_kept=0.247 arcsec matched=4875
WCS_QUALITY_DIAG: file=fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits N_match=4875 sigma_overall_arcsec=0.255 sigma_q1_arcsec=0.274 sigma_q2_arcsec=0.275 sigma_q3_arcsec=0.236 sigma_q4_arcsec=0.236 n_q1=1384 n_q2=1199 n_q3=1094 n_q4=1198 worst_quadrant_to_overall_ratio=1.077
The image catalog is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits -region wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.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_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-23-49_20.00sec_0.00C_LIGHTs_0428.fits
Saving fully-calibrated image wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.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_2026-10-10_CI_Ari-04-Q1b1x1_034935_TTUQ1b1x1_891108_PP0qbmld/wcs_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429.fits
Preparing the HTML report for the field Ari-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:40:08.86 +15:57:50.4: 14.96 +/- 0.12 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:23:34.73 +17:36:21.6: 14.82 +/- 0.11 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:14:20.04 +14:35:10.9: 14.52 +/- 0.09 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:43:26.87 +16:39:49.0: 14.78 +/- 0.09 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:44:05.58 +15:39:23.4: 14.99 +/- 0.11 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:35:07.34 +18:57:46.7: 13.25 +/- 0.03 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:27:05.98 +14:26:27.1: 13.25 +/- 0.02 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:44:21.76 +18:55:53.3: 15.26 +/- 0.16 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:03:31.74 +14:18:56.3: 13.40 +/- 0.03 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:49:10.10 +17:42:24.1: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:23:34.73 +17:36:21.6: 14.67 +/- 0.10 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:44:05.58 +15:39:23.4: 14.90 +/- 0.11 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:43:26.87 +16:39:49.0: 14.96 +/- 0.12 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:27:05.98 +14:26:27.1: 13.24 +/- 0.02 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:14:20.04 +14:35:10.9: 14.77 +/- 0.11 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:40:08.86 +15:57:50.4: 15.01 +/- 0.12 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:49:10.10 +17:42:24.1: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:44:21.76 +18:55:53.3: 15.04 +/- 0.14 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:03:31.74 +14:18:56.3: 13.44 +/- 0.03 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:35:07.34 +18:57:46.7: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.94 +/- 0.08
Forced photometry reference-image weighted average: 14.73 +/- 0.07
Forced photometry reference-image weighted average: 14.85 +/- 0.07
Forced photometry reference-image weighted average: 14.98 +/- 0.08
Forced photometry reference-image weighted average: 14.62 +/- 0.07
Forced photometry filter REJECTED candidate at 02:44:05.58 +15:39:23.4: ref_mag=14.94 +/- 0.08 new_mean_mag=14.8816 delta=0.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter REJECTED candidate at 02:23:34.73 +17:36:21.6: ref_mag=14.73 +/- 0.07 new_mean_mag=14.8479 delta=-0.12 (need > 0.90)
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry reference-image weighted average: 15.13 +/- 0.10
Forced photometry filter REJECTED candidate at 02:40:08.86 +15:57:50.4: ref_mag=14.98 +/- 0.08 new_mean_mag=14.9059 delta=0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:14:20.04 +14:35:10.9: ref_mag=14.62 +/- 0.07 new_mean_mag=14.7683 delta=-0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:43:26.87 +16:39:49.0: ref_mag=14.85 +/- 0.07 new_mean_mag=14.7700 delta=0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:44:21.76 +18:55:53.3: ref_mag=15.13 +/- 0.10 new_mean_mag=14.8966 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:27:05.98 +14:26:27.1: ref_mag=13.24 +/- 0.02 new_mean_mag=13.5550 delta=-0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:03:31.74 +14:18:56.3: ref_mag=13.42 +/- 0.02 new_mean_mag=13.6943 delta=-0.27 (need > 0.90)
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry filter REJECTED candidate at 02:35:07.34 +18:57:46.7: ref_mag=13.27 +/- 0.02 new_mean_mag=13.2597 delta=0.01 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:24:18.56 +10:19:42.3: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:01:59.79 +15:44:52.9: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:46:53.36 +13:04:55.7: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:24:49.31 +14:03:13.2: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:46:29.29 +15:36:15.0: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:43:47.98 +10:39:44.3: 14.25 +/- 0.07 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:33:28.00 +18:50:27.2: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:50:24.18 +13:25:45.9: 14.53 +/- 0.10 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:07:31.65 +17:02:01.2: 14.51 +/- 0.10 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:33:28.00 +18:50:27.2: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:01:59.79 +15:44:52.9: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:43:47.98 +10:39:44.3: 14.35 +/- 0.07 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:46:29.29 +15:36:15.0: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:24:18.56 +10:19:42.3: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:24:49.31 +14:03:13.2: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:46:53.36 +13:04:55.7: 16.25 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.30 +/- 0.05
Forced photometry filter REJECTED candidate at 02:43:47.98 +10:39:44.3: ref_mag=14.30 +/- 0.05 new_mean_mag=14.4482 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:50:24.18 +13:25:45.9: 14.49 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.51 +/- 0.06
Forced photometry filter REJECTED candidate at 02:50:24.18 +13:25:45.9: ref_mag=14.51 +/- 0.06 new_mean_mag=14.5901 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:07:31.65 +17:02:01.2: 14.55 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.07
Forced photometry filter REJECTED candidate at 03:07:31.65 +17:02:01.2: ref_mag=14.53 +/- 0.07 new_mean_mag=14.6384 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:10:43.36 +16:27:53.1: 15.16 +/- 0.17 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:55:30.72 +15:10:31.4: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:10:45.41 +18:25:59.9: 15.03 +/- 0.16 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:10:43.36 +16:27:53.1: 15.28 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.13
Forced photometry filter REJECTED candidate at 02:10:43.36 +16:27:53.1: ref_mag=15.21 +/- 0.13 new_mean_mag=14.7488 delta=0.46 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:55:30.72 +15:10:31.4: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:10:45.41 +18:25:59.9: 14.94 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.98 +/- 0.11
Forced photometry filter REJECTED candidate at 02:10:45.41 +18:25:59.9: ref_mag=14.98 +/- 0.11 new_mean_mag=14.7761 delta=0.21 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:10:46.81 +10:27:15.1: 14.89 +/- 0.15 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:09:15.80 +17:42:59.4: 14.98 +/- 0.16 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:10:46.81 +10:27:15.1: 14.96 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.92 +/- 0.11
Forced photometry filter REJECTED candidate at 02:10:46.81 +10:27:15.1: ref_mag=14.92 +/- 0.11 new_mean_mag=14.7449 delta=0.18 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:09:15.80 +17:42:59.4: 14.70 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.81 +/- 0.10
Forced photometry filter REJECTED candidate at 03:09:15.80 +17:42:59.4: ref_mag=14.81 +/- 0.10 new_mean_mag=14.7447 delta=0.06 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:06:09.71 +16:11:50.3: 15.33 +/- 0.19 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:59:54.16 +18:46:40.0: 14.94 +/- 0.15 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:06:09.71 +16:11:50.3: 15.38 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.36 +/- 0.14
Forced photometry filter REJECTED candidate at 03:06:09.71 +16:11:50.3: ref_mag=15.36 +/- 0.14 new_mean_mag=14.8278 delta=0.53 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:59:54.16 +18:46:40.0: 14.81 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.10
Forced photometry filter REJECTED candidate at 02:59:54.16 +18:46:40.0: ref_mag=14.86 +/- 0.10 new_mean_mag=14.7671 delta=0.10 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:06:25.32 +09:44:56.6: 14.95 +/- 0.16 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:09:56.29 +16:20:52.1: 14.81 +/- 0.13 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:06:25.32 +09:44:56.6: 15.28 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.13
Forced photometry filter REJECTED candidate at 03:06:25.32 +09:44:56.6: ref_mag=15.07 +/- 0.13 new_mean_mag=14.9064 delta=0.16 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:09:56.29 +16:20:52.1: 14.91 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.85 +/- 0.10
Forced photometry filter REJECTED candidate at 02:09:56.29 +16:20:52.1: ref_mag=14.85 +/- 0.10 new_mean_mag=14.7128 delta=0.14 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:05:03.49 +16:25:18.5: 15.41 +/- 0.21 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:11:41.26 +12:06:51.0: 15.17 +/- 0.17 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:05:03.49 +16:25:18.5: 15.63 +/- 0.27 detection
Forced photometry reference-image weighted average: 15.49 +/- 0.16
Forced photometry filter REJECTED candidate at 03:05:03.49 +16:25:18.5: ref_mag=15.49 +/- 0.16 new_mean_mag=15.0084 delta=0.48 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:11:41.26 +12:06:51.0: 15.14 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.12
Forced photometry filter REJECTED candidate at 02:11:41.26 +12:06:51.0: ref_mag=15.15 +/- 0.12 new_mean_mag=14.8935 delta=0.26 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:21:12.89 +11:15:23.9: 14.72 +/- 0.11 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:12:24.96 +16:33:04.0: 14.87 +/- 0.13 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:21:12.89 +11:15:23.9: 14.77 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.08
Forced photometry filter REJECTED candidate at 02:21:12.89 +11:15:23.9: ref_mag=14.74 +/- 0.08 new_mean_mag=14.7659 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:12:24.96 +16:33:04.0: 15.99 +/- 0.36 detection
Forced photometry reference-image weighted average: 15.00 +/- 0.12
Forced photometry filter REJECTED candidate at 02:12:24.96 +16:33:04.0: ref_mag=15.00 +/- 0.12 new_mean_mag=14.9017 delta=0.10 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:21:03.95 +15:02:35.3: 15.12 +/- 0.14 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:13:32.75 +18:53:49.0: 15.39 +/- 0.23 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:21:03.95 +15:02:35.3: 15.23 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.17 +/- 0.11
Forced photometry filter REJECTED candidate at 02:21:03.95 +15:02:35.3: ref_mag=15.17 +/- 0.11 new_mean_mag=14.9431 delta=0.22 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:13:32.75 +18:53:49.0: 15.32 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.35 +/- 0.15
Forced photometry filter REJECTED candidate at 02:13:32.75 +18:53:49.0: ref_mag=15.35 +/- 0.15 new_mean_mag=14.9975 delta=0.35 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:45:30.53 +17:23:33.0: 14.85 +/- 0.11 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:49:02.66 +13:56:54.1: 14.88 +/- 0.12 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:45:30.53 +17:23:33.0: 14.65 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.74 +/- 0.07
Forced photometry filter REJECTED candidate at 02:45:30.53 +17:23:33.0: ref_mag=14.74 +/- 0.07 new_mean_mag=15.0408 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:49:02.66 +13:56:54.1: 15.03 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.09
Forced photometry filter REJECTED candidate at 02:49:02.66 +13:56:54.1: ref_mag=14.95 +/- 0.09 new_mean_mag=14.9535 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:15:57.65 +10:51:25.8: 14.91 +/- 0.13 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:15:52.65 +12:00:18.7: 15.28 +/- 0.18 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 03:04:57.33 +14:33:31.1: 15.29 +/- 0.19 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:15:57.65 +10:51:25.8: 14.85 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.88 +/- 0.09
Forced photometry filter REJECTED candidate at 02:15:57.65 +10:51:25.8: ref_mag=14.88 +/- 0.09 new_mean_mag=14.7922 delta=0.09 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:58:33.82 +14:59:56.1: 15.17 +/- 0.16 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:17:29.41 +17:34:59.3: 15.23 +/- 0.18 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:15:52.65 +12:00:18.7: 15.23 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.25 +/- 0.13
Forced photometry filter REJECTED candidate at 02:15:52.65 +12:00:18.7: ref_mag=15.25 +/- 0.13 new_mean_mag=14.9913 delta=0.26 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:38:50.12 +18:09:00.3: 15.87 +/- 0.29 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 03:04:57.33 +14:33:31.1: 15.48 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.37 +/- 0.15
Forced photometry filter REJECTED candidate at 03:04:57.33 +14:33:31.1: ref_mag=15.37 +/- 0.15 new_mean_mag=15.0935 delta=0.27 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:08:52.68 +10:11:59.5: 15.15 +/- 0.20 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:08:55.66 +14:01:14.4: 15.21 +/- 0.18 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:49:36.71 +17:59:48.6: 15.37 +/- 0.18 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:17:29.41 +17:34:59.3: 15.27 +/- 0.18 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:58:33.82 +14:59:56.1: 15.38 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.25 +/- 0.13
Forced photometry reference-image weighted average: 15.26 +/- 0.12
Forced photometry filter REJECTED candidate at 02:58:33.82 +14:59:56.1: ref_mag=15.26 +/- 0.12 new_mean_mag=15.0538 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:17:29.41 +17:34:59.3: ref_mag=15.25 +/- 0.13 new_mean_mag=15.0242 delta=0.23 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:09:45.43 +17:14:21.8: 15.04 +/- 0.17 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:38:50.12 +18:09:00.3: 15.86 +/- 0.29 detection
Forced photometry reference-image weighted average: 15.86 +/- 0.20
Forced photometry filter REJECTED candidate at 02:38:50.12 +18:09:00.3: ref_mag=15.86 +/- 0.20 new_mean_mag=15.0959 delta=0.77 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:08:52.68 +10:11:59.5: 15.20 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.17 +/- 0.14
Forced photometry filter REJECTED candidate at 02:08:52.68 +10:11:59.5: ref_mag=15.17 +/- 0.14 new_mean_mag=14.8730 delta=0.30 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:49:36.71 +17:59:48.6: 15.48 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.42 +/- 0.13
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:08:55.66 +14:01:14.4: 15.08 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 02:49:36.71 +17:59:48.6: ref_mag=15.42 +/- 0.13 new_mean_mag=15.0654 delta=0.36 (need > 0.90)
Forced photometry reference-image weighted average: 15.14 +/- 0.12
Forced photometry filter REJECTED candidate at 02:08:55.66 +14:01:14.4: ref_mag=15.14 +/- 0.12 new_mean_mag=14.9932 delta=0.14 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:17:17.38 +14:58:03.4: 15.49 +/- 0.22 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:17:04.80 +13:15:45.4: 15.41 +/- 0.21 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:09:45.43 +17:14:21.8: 15.77 +/- 0.32 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.15
Forced photometry filter REJECTED candidate at 02:09:45.43 +17:14:21.8: ref_mag=15.19 +/- 0.15 new_mean_mag=15.0993 delta=0.09 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:25:17.63 +10:22:51.1: 15.25 +/- 0.17 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:14:50.53 +09:39:39.2: 15.33 +/- 0.21 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:17:17.38 +14:58:03.4: 15.14 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.27 +/- 0.13
Forced photometry filter REJECTED candidate at 02:17:17.38 +14:58:03.4: ref_mag=15.27 +/- 0.13 new_mean_mag=14.9761 delta=0.29 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:09:39.84 +09:25:01.3: 15.19 +/- 0.20 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:17:04.80 +13:15:45.4: 15.20 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.28 +/- 0.13
Forced photometry filter REJECTED candidate at 02:17:04.80 +13:15:45.4: ref_mag=15.28 +/- 0.13 new_mean_mag=15.0571 delta=0.22 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-02_20.00sec_-15.00C_LIGHT_0117.fits at 02:11:39.40 +12:41:01.9: 15.09 +/- 0.16 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:25:17.63 +10:22:51.1: 15.43 +/- 0.20 detection
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:14:50.53 +09:39:39.2: 15.10 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.13
Forced photometry reference-image weighted average: 15.32 +/- 0.13
Forced photometry filter REJECTED candidate at 02:14:50.53 +09:39:39.2: ref_mag=15.19 +/- 0.13 new_mean_mag=15.0201 delta=0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:25:17.63 +10:22:51.1: ref_mag=15.32 +/- 0.13 new_mean_mag=14.9724 delta=0.35 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:09:39.84 +09:25:01.3: 15.01 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.09 +/- 0.13
Forced photometry filter REJECTED candidate at 02:09:39.84 +09:25:01.3: ref_mag=15.09 +/- 0.13 new_mean_mag=14.9438 delta=0.14 (need > 0.90)
Forced photometry on wcs_Ari-04-Q1b1x1_2026-01-08_21-46-45_20.00sec_-15.00C_LIGHT_0118.fits at 02:11:39.40 +12:41:01.9: 15.18 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.12
Forced photometry filter REJECTED candidate at 02:11:39.40 +12:41:01.9: ref_mag=15.13 +/- 0.12 new_mean_mag=14.9113 delta=0.22 (need > 0.90)
Adding exclusion_list_local.txt__out53294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54216.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 53076_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 53076_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53078_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 53078_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53084_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 53084_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53089_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 53089_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53092_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 53092_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53093_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 53093_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53103_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 53103_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53104_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 53104_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53105_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 53105_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 53294_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
Preparing report for the candidate 53294_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
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Considering the candidate 53428_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
Preparing report for the candidate 53428_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
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Considering the candidate 53490_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
Preparing report for the candidate 53490_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
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Considering the candidate 53710_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 53710_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
**** FOUND 02:57:25.87 +10:28:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53720_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 53720_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
**** FOUND 02:53:51.18 +15:25:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53745_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
Preparing report for the candidate 53745_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
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Considering the candidate 53746_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
Preparing report for the candidate 53746_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
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Considering the candidate 53749_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
Preparing report for the candidate 53749_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
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Considering the candidate 53859_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
Preparing report for the candidate 53859_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
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Considering the candidate 54039_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54039_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54131_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54131_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54165_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54165_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54203_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54203_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54216_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
Preparing report for the candidate 54216_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
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Considering the candidate 54226_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54226_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54231_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54231_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54235_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54235_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54237_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54237_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54283_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54283_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54286_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54286_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54309_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54309_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54325_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54325_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54338_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54338_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54359_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54359_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54367_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54367_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54375_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54375_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54380_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54380_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54384_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54384_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54387_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54387_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54389_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54389_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54399_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54399_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54403_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54403_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54417_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54417_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54421_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54421_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54424_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54424_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54429_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54429_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54444_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54444_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54456_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54456_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54465_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54465_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54471_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54471_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54477_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54477_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54486_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54486_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54504_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54504_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54505_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54505_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 54521_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 54521_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
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Considering the candidate 41054_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429
The candidate 41054_fd_Ari-04-Q1b1x1_2026-10-10_03-24-49_20.00sec_0.00C_LIGHTs_0429 did not pass the final checks
