This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6
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 05 07.4518 2461167.9518 11.50 15:49:22.39 -09:11:41.4
359.11485 33.63768 galactic Lib Second-epoch detections are separated by 0.4" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.92 Undina 1 -0 1 11.5 -0 0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 15:49:22.39 -09:11:41.4: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 15:49:22.39 -09:11:41.4: 14.94 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461167.9518,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260507.4518 11.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 07.4518 2461167.9518 11.98 16:11:55.24 -13:44:13.3
359.32817 26.48944 galactic Sco Second-epoch detections are separated by 0.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.346 Hermentaria 1 -0 1 11.7 -0 0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:11:55.24 -13:44:13.3: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:11:55.24 -13:44:13.3: 15.22 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461167.9518,11.98,0.05,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 20260507.4518 11.98CV 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 05 07.4518 2461167.9518 12.50 15:54:13.84 -08:48:51.9
0.40057 32.98284 galactic Lib Second-epoch detections are separated by 1.4" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.776 Berbericia 1 -0 1 12.6 0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 15:54:13.84 -08:48:51.9: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 15:54:13.84 -08:48:51.9: 15.27 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461167.9518,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260507.4518 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 07.4518 2461167.9518 13.19 16:42:46.11 -05:51:31.9
11.39415 25.13821 galactic Oph Second-epoch detections are separated by 2.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.97 Klotho 1 -2 2 12.9 -0 0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:42:46.11 -05:51:31.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:42:46.11 -05:51:31.9: 15.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461167.9518,13.19,0.05,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 20260507.4518 13.19CV 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 05 07.4518 2461167.9518 12.97 16:13:45.34 -08:28:48.2
4.27121 29.45429 galactic Sco Second-epoch detections are separated by 0.3" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.559 Nanon 1 1 2 13.1 -0 -0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:13:45.34 -08:28:48.2: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:13:45.34 -08:28:48.2: 15.36 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461167.9518,12.97,0.05,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 20260507.4518 12.97CV 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 05 07.4518 2461167.9518 13.12 16:03:25.68 -13:43:09.4
357.82522 28.06105 galactic Sco Second-epoch detections are separated by 2.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.563 Suleika 1 1 1 13.3 -0 0
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:03:25.68 -13:43:09.4: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:03:25.68 -13:43:09.4: 15.18 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461167.9518,13.12,0.05,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 20260507.4518 13.12CV 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 05 07.4518 2461167.9518 11.60 16:21:24.50 -07:42:01.7
6.28988 28.41768 galactic Oph Second-epoch detections are separated by 1.2" and 5.4 pix
The object was found in VSX 1" W Oph
Type: M
# Max. Min./Amp. JD0 Period
9.100 V 14.900 V 2438414.00000 332.680000000000 M6-M8e
The object was not found in astcheck.
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:21:24.50 -07:42:01.7: 12.80 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:21:24.50 -07:42:01.7: 12.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
W Oph,2461167.9518,11.60,0.05,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
W Oph 20260507.4518 11.60CV 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 05 07.4518 2461167.9518 12.22 16:16:19.19 -12:47:11.9
0.90804 26.27498 galactic Sco Second-epoch detections are separated by 0.6" and 5.2 pix
The object was found in VSX 1" V0814 Sco
Type: SR:
# Max. Min./Amp. JD0 Period
12.950 V Y 0.920 V 2452426.90000 198.028824000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:16:19.19 -12:47:11.9: 13.50 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:16:19.19 -12:47:11.9: 12.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0814 Sco,2461167.9518,12.22,0.05,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
V0814 Sco 20260507.4518 12.22CV 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: 2461098.97005181 27.02.2026 11:16:42.476 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
First image: 2461098.97005181 27.02.2026 11:16:42.476 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Last image: 2461167.95210588 07.05.2026 10:50:51.948 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.84
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 5172
Objects passed selection criteria: 5166
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 5081
Average stars matched: 5047 (99.3308 %)
Memory usage VmPeak: 112236 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 6 12:14:36 CDT 2026
VaST build number 1.0rc89-43-g0c21e0c3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 7 05:59:12 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: 2461098.97005181 27.02.2026 11:16:42.476 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
First image: 2461098.97005181 27.02.2026 11:16:42.476 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Last image: 2461167.95210588 07.05.2026 10:50:51.948 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 27
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
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: 17 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 43242
Objects passed selection criteria: 43143
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 42862.8
Average stars matched: 42423.8 (98.9758 %)
Memory usage VmPeak: 150500 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 6 12:14:36 CDT 2026
VaST build number 1.0rc89-43-g0c21e0c3
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu May 7 06:01:25 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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461167.95144200
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_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits'
wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits exists and is non-empty
Saving wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits to local_wcs_cache/
'wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits' -> 'local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits'
wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits exists and is non-empty
Saving wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits'
wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits exists and is non-empty
Saving wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits (1st reference image)
verification OK: wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Image size: 941.5'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:09.052 -09:59:57.66 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits (1st new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:12.318 -09:59:59.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:09.052 -09:59:57.66
Second-epoch image center 16:17:12.318 -09:59:59.42
Angular distance between the image centers 0.0134 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits (2nd new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:14.425 -10:00:05.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:17:09.052 -09:59:57.66
Second-epoch image center 16:17:14.425 -10:00:05.70
Angular distance between the image centers 0.0222 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:17:12.318 -09:59:59.42
Second-epoch second image center 16:17:14.425 -10:00:05.70
Angular distance between the image centers 0.00882 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.HxzPLxsYRp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits &> /tmp/tmp.bPhhtWVVz6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits &> /tmp/tmp.N82POBXlrI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits &> /tmp/tmp.8MKKfgIF3k
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits and wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits and wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
Found non-empty wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits and wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
The reference image (wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits) and catalog (wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat) found
'wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat' -> 'wcsmag.cat'
Read 7722 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 236.1744 to 252.3750 deg, Dec -15.2624 to -4.6754 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 236.1744 to 252.3750 deg, Dec -15.2624 to -4.6754 deg
Loaded 4809 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): 3998 out of 4171 total matches.
Matched with Tycho-2 4171 out of 7722 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.912750
a=0.000000 b=1.000000 c=22.912750
From vast_summary.log: estimated ref. image limiting mag.: -7.84
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7722 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 236.1744 to 252.3750 deg, Dec -15.2624 to -4.6754 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 236.1744 to 252.3750 deg, Dec -15.2624 to -4.6754 deg
Loaded 4809 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): 3998 out of 4171 total matches.
Matched with Tycho-2 4171 out of 7722 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits (aperture=5.8)
Read 5066 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 236.2082 to 252.3187 deg, Dec -15.2481 to -4.6756 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 236.2082 to 252.3187 deg, Dec -15.2481 to -4.6756 deg
Loaded 4791 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): 3538 out of 3621 total matches.
Matched with Tycho-2 3621 out of 5066 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits:
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
2.4 pix Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
2.2 pix fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
2.2 pix fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
2.0 pix wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
2.4 pix wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Limiting magnitude estimates:
15.1 mag. Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
14.5 mag. Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
14.2 mag. fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
14.1 mag. fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.3 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.HxzPLxsYRp (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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits' -> 'wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=451, passed=7719
Got 7719 stars (including 7254 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 7719 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 7517 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 7520 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 7520 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bPhhtWVVz6 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits' -> 'wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat corresponding to the image wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat corresponding to the image wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=289, passed=5066
Got 5066 stars (including 4773 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat
util/solve_plate_with_UCAC5 got 5066 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 4960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 4958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 4958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits -region wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.N82POBXlrI (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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=314, passed=3884
Got 3884 stars (including 3563 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat
util/solve_plate_with_UCAC5 got 3884 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 3812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 3813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 3813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits -region wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8MKKfgIF3k (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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=8, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=316, passed=3780
Got 3780 stars (including 3459 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat
util/solve_plate_with_UCAC5 got 3780 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 3713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 3715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 3715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits -region wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits'
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits'
Preparing the HTML report for the field Sco-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 15:49:22.39 -09:11:41.4: 15.56 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:21:24.52 -07:42:01.4: 12.58 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 15:49:22.39 -09:11:41.4: 14.94 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:21:24.52 -07:42:01.4: 12.46 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.54 +/- 0.02
Forced photometry filter KEPT candidate at 16:21:24.52 -07:42:01.4: ref_mag=12.54 +/- 0.02 new_mean_mag=11.2561 delta=1.29 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out20099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20126.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20099_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 20099_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 16:21:24.52 -07:42:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 1.436 4351886131050162048 245.35188659603 -07.70010221838 9.4737 7.8441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20126_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 20126_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Sco-01-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 ####
15:49:22.39 -09:11:41.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits exists and is non-empty
wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits exists and is non-empty
wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits (1st reference image)
verification OK: wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Image size: 941.5'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:09.052 -09:59:57.66 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits (1st new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:12.318 -09:59:59.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:17:09.052 -09:59:57.66
Second-epoch image center 16:17:12.318 -09:59:59.42
Angular distance between the image centers 0.0134 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits (2nd new image)
verification OK: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:17:14.425 -10:00:05.70 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:17:09.052 -09:59:57.66
Second-epoch image center 16:17:14.425 -10:00:05.70
Angular distance between the image centers 0.0222 deg.
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# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:17:12.318 -09:59:59.42
Second-epoch second image center 16:17:14.425 -10:00:05.70
Angular distance between the image centers 0.00882 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.yUtdLHwmeo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits &> /tmp/tmp.c1pPbsQKMA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits &> /tmp/tmp.QulFJvyaj1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits &> /tmp/tmp.J7GmxoolAr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits and wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits and wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
Found non-empty wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits and wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
The reference image (wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits) and catalog (wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat) found
'wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat' -> 'wcsmag.cat'
Read 62439 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 236.1591 to 252.4002 deg, Dec -15.2898 to -4.6725 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 236.1591 to 252.4002 deg, Dec -15.2898 to -4.6725 deg
Loaded 4831 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): 3832 out of 4290 total matches.
Matched with Tycho-2 4290 out of 62439 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.794400
a=0.000000 b=1.000000 c=22.794400
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.24
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.24
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 62439 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 236.1591 to 252.4002 deg, Dec -15.2898 to -4.6725 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 236.1591 to 252.4002 deg, Dec -15.2898 to -4.6725 deg
Loaded 4831 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): 3832 out of 4290 total matches.
Matched with Tycho-2 4290 out of 62439 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits:
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits (aperture=4.5)
Read 40555 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 236.1835 to 252.3628 deg, Dec -15.2669 to -4.6542 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 236.1835 to 252.3628 deg, Dec -15.2669 to -4.6542 deg
Loaded 4815 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): 3958 out of 4238 total matches.
Matched with Tycho-2 4238 out of 40555 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits:
Forced-photometry filter: calibrated wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits -> calib.txt_param_ref_wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
2.1 pix Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
2.0 pix fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
2.0 pix fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
1.9 pix wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
2.1 pix wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Limiting magnitude estimates:
15.2 mag. Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
14.7 mag. Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
14.4 mag. fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
14.4 mag. fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.9 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.yUtdLHwmeo (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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits' -> 'wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2730, passed=62428
Got 62428 stars (including 59597 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 62428 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 61048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 61049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 61049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.c1pPbsQKMA (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits' -> 'wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS-calibrated image found: wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Checking if the catalog wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat corresponding to the image wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat corresponding to the image wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS catalog name: wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1580, passed=40542
Got 40542 stars (including 38911 good ones) from the SExtractor catalog wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat
util/solve_plate_with_UCAC5 got 40542 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 39938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 39937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 39937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits -region wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QulFJvyaj1 (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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1261, passed=35317
Got 35317 stars (including 33979 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat
util/solve_plate_with_UCAC5 got 35317 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits -region wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.J7GmxoolAr (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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
Checking if the catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat corresponding to the image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
WCS catalog name: wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1246, passed=34442
Got 34442 stars (including 33140 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat
util/solve_plate_with_UCAC5 got 34442 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34007 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 430 (Dec -15.6 to -4.2)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34007 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 34008 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits -region wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-49-54_20.00sec_-5.00C_LIGHTs_0098.fits
Saving fully-calibrated image wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.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_2026-05-07_CI_Sco-01-Q1b1x1_055149_TTUQ1b1x1_3917809_ObYRG7S6/wcs_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099.fits
Preparing the HTML report for the field Sco-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:12:26.75 -13:37:54.1: 13.53 +/- 0.05 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:11:55.24 -13:44:13.3: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:44:58.12 -13:41:56.8: 13.42 +/- 0.05 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:35:13.06 -13:09:10.8: 12.80 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 15:54:13.84 -08:48:51.9: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:13:45.34 -08:28:48.2: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:07:19.85 -13:09:11.0: 13.10 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:42:46.11 -05:51:31.9: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:32:19.25 -06:25:29.0: 12.96 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:44:58.12 -13:41:56.8: 13.33 +/- 0.08 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:12:26.75 -13:37:54.1: 13.41 +/- 0.07 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:35:13.06 -13:09:10.8: 12.71 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:11:55.24 -13:44:13.3: 15.22 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.40 +/- 0.04
Forced photometry reference-image weighted average: 13.49 +/- 0.04
Forced photometry filter REJECTED candidate at 16:44:58.12 -13:41:56.8: ref_mag=13.40 +/- 0.04 new_mean_mag=13.7059 delta=-0.31 (need > 0.90)
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Forced photometry filter REJECTED candidate at 16:12:26.75 -13:37:54.1: ref_mag=13.49 +/- 0.04 new_mean_mag=13.5388 delta=-0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 16:35:13.06 -13:09:10.8: ref_mag=12.78 +/- 0.02 new_mean_mag=13.0066 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:45:34.76 -09:27:47.8: 13.08 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:07:19.85 -13:09:11.0: 13.04 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.03
Forced photometry filter REJECTED candidate at 16:07:19.85 -13:09:11.0: ref_mag=13.08 +/- 0.03 new_mean_mag=12.9747 delta=0.11 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 15:54:13.84 -08:48:51.9: 15.27 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:32:19.25 -06:25:29.0: 12.64 +/- 0.03 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:13:45.34 -08:28:48.2: 15.36 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.85 +/- 0.02
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:42:46.11 -05:51:31.9: 15.12 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 16:32:19.25 -06:25:29.0: ref_mag=12.85 +/- 0.02 new_mean_mag=13.1371 delta=-0.29 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:45:34.76 -09:27:47.8: 12.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.03
Forced photometry filter REJECTED candidate at 16:45:34.76 -09:27:47.8: ref_mag=12.97 +/- 0.03 new_mean_mag=13.1416 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:17:36.26 -05:14:47.9: 13.36 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:03:25.68 -13:43:09.4: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:36:24.13 -08:16:10.8: 15.32 +/- 0.22 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:17:36.26 -05:14:47.9: 13.00 +/- 0.04 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:03:25.68 -13:43:09.4: 15.18 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.22 +/- 0.03
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:16:19.19 -12:47:11.9: 13.50 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 16:17:36.26 -05:14:47.9: ref_mag=13.22 +/- 0.03 new_mean_mag=13.4818 delta=-0.26 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits at 16:21:24.50 -07:42:01.7: 12.80 +/- 0.02 detection
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:36:24.13 -08:16:10.8: 15.19 +/- 0.34 detection
Forced photometry reference-image weighted average: 15.28 +/- 0.18
Forced photometry filter KEPT candidate at 16:36:24.13 -08:16:10.8: ref_mag=15.28 +/- 0.18 new_mean_mag=14.2631 delta=1.02 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:16:19.19 -12:47:11.9: 12.86 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.03
Forced photometry filter KEPT candidate at 16:16:19.19 -12:47:11.9: ref_mag=13.17 +/- 0.03 new_mean_mag=12.2243 delta=0.94 (need > 0.90)
Forced photometry on wcs_Sco-01-Q1b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits at 16:21:24.50 -07:42:01.7: 12.78 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry filter KEPT candidate at 16:21:24.50 -07:42:01.7: ref_mag=12.80 +/- 0.02 new_mean_mag=11.5951 delta=1.20 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out73892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out14434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73362.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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 72902_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 72902_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 16:30:13.49 -14:40:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72904_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 72904_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 16:43:57.20 -12:21:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72907_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 72907_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
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Considering the candidate 72908_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 72908_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 16:15:47.40 -12:59:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72910_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 72910_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
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Considering the candidate 72913_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 72913_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
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Considering the candidate 72914_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 72914_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 15:55:30.78 -05:50:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72915_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 72915_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 16:40:06.28 -12:33:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73027_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 73027_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 15:49:22.39 -09:11:41.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 73074_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 73074_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 73174_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 73174_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 73236_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 73236_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 16:02:58.22 -05:49:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73252_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 73252_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 73279_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 73279_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 73308_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 73308_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
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Considering the candidate 73314_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 73314_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
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Considering the candidate 73327_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 73327_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
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Considering the candidate 73362_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 73362_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 73490_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 73490_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
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Considering the candidate 73602_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 73602_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 16:44:50.40 -06:11:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73892_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099
The candidate 73892_fd_Sco-01-Q1b1x1_2026-05-07_05-50-51_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
