This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ
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 06 20.2532 2461211.7532 12.07 00:27:59.20 +51:36:52.5
119.22605 -11.08834 galactic Cas Second-epoch detections are separated by 0.7" and 1.9 pix
The object was found in VSX 2" ASASSN-V J002759.35+513654.0
Type: SRS
# Max. Min./Amp. JD0 Period
14.100 g Y 0.230 g 2459404.93800 25.592000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:27:59.20 +51:36:52.5: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:27:59.20 +51:36:52.5: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 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!
TCP 2026 06 20.2532* 00 27 59.20 +51 36 52.5 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J002759.35+513654.0,2461211.7532,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J002759.35+513654.0 20260620.2532 12.07CV 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 06 20.2532 2461211.7532 11.96 23:32:11.74 +50:01:12.0
110.12089 -10.87033 galactic And Second-epoch detections are separated by 2.5" and 1.9 pix
The object was found in VSX 1" ASASSN-V J233211.68+500112.5
Type: YSO
# Max. Min./Amp. JD0 Period
12.770 V 13.180 V
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:32:11.74 +50:01:12.0: 13.12 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:32:11.74 +50:01:12.0: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 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!
TCP 2026 06 20.2532* 23 32 11.74 +50 01 12.0 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J233211.68+500112.5,2461211.7532,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J233211.68+500112.5 20260620.2532 11.96CV 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 06 20.2532 2461211.7532 11.45 00:29:58.93 +53:42:32.6
119.72026 -9.02884 galactic Cas Second-epoch detections are separated by 0.7" and 1.8 pix
The object was found in VSX 1" ASASSN-V J002959.02+534233.4
Type: LPV
# Max. Min./Amp. JD0 Period
12.270 V 12.720 V 711.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:29:58.93 +53:42:32.6: 12.35 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:29:58.93 +53:42:32.6: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.2532* 00 29 58.93 +53 42 32.6 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J002959.02+534233.4,2461211.7532,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J002959.02+534233.4 20260620.2532 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.2532 2461211.7532 12.06 23:58:59.21 +54:51:07.6
115.36654 -7.24735 galactic Cas Second-epoch detections are separated by 1.1" and 1.7 pix
The object was found in VSX 1" EV Cas
Type: LB
# Max. Min./Amp. JD0 Period
14.700 pg 15.500 pg 134.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:58:59.21 +54:51:07.6: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:58:59.21 +54:51:07.6: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 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!
TCP 2026 06 20.2532* 23 58 59.21 +54 51 07.6 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EV Cas,2461211.7532,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
EV Cas 20260620.2532 12.06CV 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 06 20.2532 2461211.7532 12.52 00:19:48.83 +54:03:26.7
118.24909 -8.52655 galactic Cas Second-epoch detections are separated by 1.0" and 1.6 pix
The object was found in VSX 1" ASASSN-V J001948.93+540327.5
Type: SR
# Max. Min./Amp. JD0 Period
14.440 g Y 0.670 g 2458893.58100 151.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:19:48.83 +54:03:26.7: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:19:48.83 +54:03:26.7: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 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!
TCP 2026 06 20.2532* 00 19 48.83 +54 03 26.7 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J001948.93+540327.5,2461211.7532,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J001948.93+540327.5 20260620.2532 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 20.2532 2461211.7532 11.66 23:34:44.03 +50:31:11.5
110.66808 -10.51643 galactic And Second-epoch detections are separated by 1.8" and 1.4 pix
The object was found in VSX 1" V0427 And
Type: SRB
# Max. Min./Amp. JD0 Period
14.400 pg 16.200 pg 180.000000000000 :
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:34:44.03 +50:31:11.5: 12.71 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:34:44.03 +50:31:11.5: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.2532* 23 34 44.03 +50 31 11.5 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0427 And,2461211.7532,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
V0427 And 20260620.2532 11.66CV 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 06 20.2532 2461211.7532 12.19 00:02:03.87 +53:58:57.9
115.63580 -8.18809 galactic Cas Second-epoch detections are separated by 1.4" and 1.9 pix
The object was found in VSX 1" NSVS J0002034+535901
Type: SR
# Max. Min./Amp. JD0 Period
14.378 g Y 1.167 g 2458357.13120 216.381785400000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:02:03.87 +53:58:57.9: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:02:03.87 +53:58:57.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 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!
TCP 2026 06 20.2532* 00 02 03.87 +53 58 57.9 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0002034+535901,2461211.7532,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
NSVS J0002034+535901 20260620.2532 12.19CV 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 06 20.2532 2461211.7532 13.09 00:18:42.86 +54:02:20.7
118.08487 -8.52441 galactic Cas Second-epoch detections are separated by 1.8" and 1.6 pix
The object was found in VSX 1" V1029 Cas
Type: CWA
# Max. Min./Amp. JD0 Period
13.400 R 14.400 R 2451339.90000 15.510000000000
The object was not found in astcheck.
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:18:42.86 +54:02:20.7: 14.30 +/- 0.08 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:18:42.86 +54:02:20.7: 14.37 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 20.2532* 00 18 42.86 +54 02 20.7 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1029 Cas,2461211.7532,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
V1029 Cas 20260620.2532 13.09CV 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: 2461082.59778519 11.02.2026 02:20:38.640 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
First image: 2461082.59778519 11.02.2026 02:20:38.640 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Last image: 2461211.75346977 20.06.2026 06:04:49.788 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.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.: -7.78
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): 20675
Objects passed selection criteria: 20544
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 12593.5
Average stars matched: 11925.2 (94.6937 %)
Memory usage VmPeak: 126736 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jun 20 01:14:43 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: 2461082.59778519 11.02.2026 02:20:38.640 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
First image: 2461082.59778519 11.02.2026 02:20:38.640 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Last image: 2461211.75346977 20.06.2026 06:04:49.788 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 148
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
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: 40 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): 165396
Objects passed selection criteria: 164876
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 107450
Average stars matched: 100430 (93.4672 %)
Memory usage VmPeak: 1931892 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Jun 20 01:20:12 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/TTUQ2b1x1/TTUQ2_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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.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/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.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: 2461211.75302022
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_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits'
wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits exists and is non-empty
Saving wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits to local_wcs_cache/
'wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits' -> 'local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits'
wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits'
wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Image size: 941.8'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:52.581 +53:59:29.78 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_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.565 +53:58:38.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:52.581 +53:59:29.78
Second-epoch image center 23:59:59.565 +53:58:38.91
Angular distance between the image centers 0.0222 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:58.763 +53:58:31.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:52.581 +53:59:29.78
Second-epoch image center 23:59:58.763 +53:58:31.84
Angular distance between the image centers 0.0221 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 23:59:59.565 +53:58:38.91
Second-epoch second image center 23:59:58.763 +53:58:31.84
Angular distance between the image centers 0.00278 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/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits &> /tmp/tmp.t7KUIOtxpx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits &> /tmp/tmp.ahuFHsHg0A
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits &> /tmp/tmp.lQzPM6L7Jp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits &> /tmp/tmp.hstqmojys8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.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_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat' -> 'wcsmag.cat'
Read 29225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9995 deg, Dec +47.7049 to +59.3705 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 0.0002 to 359.9995 deg, Dec 47.7049 to 59.3705 deg
Loaded 162590 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): 14935 out of 16561 total matches.
Matched with Tycho-2 16561 out of 29225 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.842700
a=0.000000 b=1.000000 c=22.842700
From vast_summary.log: estimated ref. image limiting mag.: -7.78
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.06
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.06
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9995 deg, Dec +47.7049 to +59.3705 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 0.0002 to 359.9995 deg, Dec 47.7049 to 59.3705 deg
Loaded 162590 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): 14935 out of 16561 total matches.
Matched with Tycho-2 16561 out of 29225 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits (aperture=6.0)
Read 29065 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0009 to 359.9998 deg, Dec +47.6373 to +59.3623 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 0.0009 to 359.9998 deg, Dec 47.6373 to 59.3623 deg
Loaded 163448 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): 14807 out of 16429 total matches.
Matched with Tycho-2 16429 out of 29065 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
2.1 pix Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
2.4 pix fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
2.5 pix fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
2.1 pix wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
2.1 pix wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Limiting magnitude estimates:
15.1 mag. Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
15.1 mag. Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
13.0 mag. fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
12.9 mag. fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 10.5 (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.t7KUIOtxpx (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/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3209, passed=29225
Got 29225 stars (including 25982 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
util/solve_plate_with_UCAC5 got 29225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
RA wraps around 0/360 boundary: field RA 345.4494 through 0 to 15.3164, gap 15.3164 to 345.4494
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 27679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4490 through 0 to 15.3182, gap 15.3182 to 345.4490
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 27676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 27675 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits N_match=976 sigma_overall_arcsec=0.504 sigma_q1_arcsec=0.579 sigma_q2_arcsec=0.471 sigma_q3_arcsec=0.575 sigma_q4_arcsec=0.424 n_q1=194 n_q2=269 n_q3=218 n_q4=295 worst_quadrant_to_overall_ratio=1.147
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits -region wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ahuFHsHg0A (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/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3195, passed=29065
Got 29065 stars (including 25829 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 29065 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
RA wraps around 0/360 boundary: field RA 345.4479 through 0 to 15.3165, gap 15.3165 to 345.4479
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 27619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4484 through 0 to 15.3183, gap 15.3183 to 345.4484
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 27619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 27619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits N_match=976 sigma_overall_arcsec=0.538 sigma_q1_arcsec=0.643 sigma_q2_arcsec=0.467 sigma_q3_arcsec=0.695 sigma_q4_arcsec=0.452 n_q1=196 n_q2=274 n_q3=213 n_q4=293 worst_quadrant_to_overall_ratio=1.292
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits -region wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.lQzPM6L7Jp (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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=282, passed=5837
Got 5837 stars (including 5549 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat
util/solve_plate_with_UCAC5 got 5837 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9182 through 0 to 14.6553, gap 14.6553 to 344.9182
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 5453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.9172 through 0 to 14.6572, gap 14.6572 to 344.9172
Reading UCAC5 zone files...
Searching UCAC5 zones 690 to 748 (Dec 48.0 to 59.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 961 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits N_match=961 sigma_overall_arcsec=0.772 sigma_q1_arcsec=0.646 sigma_q2_arcsec=0.707 sigma_q3_arcsec=0.731 sigma_q4_arcsec=0.915 n_q1=272 n_q2=218 n_q3=67 n_q4=404 worst_quadrant_to_overall_ratio=1.186
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits -region wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.hstqmojys8 (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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=278, passed=5776
Got 5776 stars (including 5488 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat
util/solve_plate_with_UCAC5 got 5776 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8495 through 0 to 14.6552, gap 14.6552 to 344.8495
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.2)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 5382 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8487 through 0 to 14.6577, gap 14.6577 to 344.8487
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.2)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 5382 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 5382 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits N_match=958 sigma_overall_arcsec=0.817 sigma_q1_arcsec=0.818 sigma_q2_arcsec=0.766 sigma_q3_arcsec=0.741 sigma_q4_arcsec=0.822 n_q1=150 n_q2=268 n_q3=100 n_q4=440 worst_quadrant_to_overall_ratio=1.006
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits -region wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits sigma_overall=0.504 worst_q_ratio=1.147
ref2=Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits sigma_overall=0.538 worst_q_ratio=1.292
new1=fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits sigma_overall=0.772 worst_q_ratio=1.186
new2=fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits sigma_overall=0.817 worst_q_ratio=1.006
reference average sigma_overall=0.521 worst_q_ratio=1.2195
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006_astrometric_residuals.png (976 matched stars from wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007_astrometric_residuals.png (976 matched stars from wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.50 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202_astrometric_residuals.png (961 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.65 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203_astrometric_residuals.png (958 matched stars from wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.73 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits'
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32478_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 32478_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:20:53.31 +50:09:07.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.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_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits exists and is non-empty
wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits exists and is non-empty
wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits (1st reference image)
verification OK: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Image size: 941.8'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 23:59:52.581 +53:59:29.78 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_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits (1st new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.565 +53:58:38.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:52.581 +53:59:29.78
Second-epoch image center 23:59:59.565 +53:58:38.91
Angular distance between the image centers 0.0222 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits (2nd new image)
verification OK: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
Image size: 938.9'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:58.763 +53:58:31.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:52.581 +53:59:29.78
Second-epoch image center 23:59:58.763 +53:58:31.84
Angular distance between the image centers 0.0221 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 23:59:59.565 +53:58:38.91
Second-epoch second image center 23:59:58.763 +53:58:31.84
Angular distance between the image centers 0.00278 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/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits &> /tmp/tmp.Qq4Z7AcNpu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits &> /tmp/tmp.amdcqfM4NE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits &> /tmp/tmp.UPTpJujnn6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits &> /tmp/tmp.oon10X4vbF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.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_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
Found non-empty wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits and wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
The reference image (wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits) and catalog (wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat) found
'wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat' -> 'wcsmag.cat'
Read 217609 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9999 deg, Dec +47.6392 to +59.3793 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 0.0001 to 359.9999 deg, Dec 47.6392 to 59.3793 deg
Loaded 163629 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): 11705 out of 17839 total matches.
Matched with Tycho-2 17839 out of 217609 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.676500
a=0.000000 b=1.000000 c=22.676500
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 217609 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9999 deg, Dec +47.6392 to +59.3793 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 0.0001 to 359.9999 deg, Dec 47.6392 to 59.3793 deg
Loaded 163629 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): 11705 out of 17839 total matches.
Matched with Tycho-2 17839 out of 217609 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits (aperture=4.4)
Read 217552 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9999 deg, Dec +47.6349 to +59.3691 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 0.0001 to 359.9999 deg, Dec 47.6349 to 59.3691 deg
Loaded 163556 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): 11613 out of 17712 total matches.
Matched with Tycho-2 17712 out of 217552 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits:
Forced-photometry filter: calibrated wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits -> calib.txt_param_ref_wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 56 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
1.9 pix Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
2.2 pix fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
2.1 pix fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
1.9 pix wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
1.9 pix wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Limiting magnitude estimates:
15.3 mag. Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
15.3 mag. Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
13.3 mag. fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
13.2 mag. fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.9 (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.Qq4Z7AcNpu (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/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits' -> 'wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=32857, passed=217571
Got 217571 stars (including 184418 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat
util/solve_plate_with_UCAC5 got 217571 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
RA wraps around 0/360 boundary: field RA 345.4355 through 0 to 15.4567, gap 15.4567 to 345.4355
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 211761 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4349 through 0 to 15.4584, gap 15.4584 to 345.4349
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 211763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 211761 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits N_match=976 sigma_overall_arcsec=0.491 sigma_q1_arcsec=0.581 sigma_q2_arcsec=0.455 sigma_q3_arcsec=0.514 sigma_q4_arcsec=0.430 n_q1=213 n_q2=264 n_q3=237 n_q4=262 worst_quadrant_to_overall_ratio=1.183
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits -region wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.amdcqfM4NE (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/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits' -> 'wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS-calibrated image found: wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
Checking if the catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat corresponding to the image wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits
WCS catalog name: wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=32499, passed=217519
Got 217519 stars (including 184678 good ones) from the SExtractor catalog wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 217519 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
RA wraps around 0/360 boundary: field RA 345.4449 through 0 to 15.4097, gap 15.4097 to 345.4449
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 212427 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4450 through 0 to 15.4115, gap 15.4115 to 345.4450
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 212426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 212423 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits N_match=978 sigma_overall_arcsec=0.511 sigma_q1_arcsec=0.559 sigma_q2_arcsec=0.441 sigma_q3_arcsec=0.580 sigma_q4_arcsec=0.464 n_q1=220 n_q2=266 n_q3=235 n_q4=257 worst_quadrant_to_overall_ratio=1.135
The image catalog is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits -region wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.UPTpJujnn6 (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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=2530, passed=52884
Got 52884 stars (including 50265 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat
util/solve_plate_with_UCAC5 got 52884 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8492 through 0 to 14.7496, gap 14.7496 to 344.8492
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 48378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8493 through 0 to 14.7517, gap 14.7517 to 344.8493
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 48378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 48378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits N_match=961 sigma_overall_arcsec=0.730 sigma_q1_arcsec=0.678 sigma_q2_arcsec=0.657 sigma_q3_arcsec=0.772 sigma_q4_arcsec=0.875 n_q1=274 n_q2=208 n_q3=66 n_q4=413 worst_quadrant_to_overall_ratio=1.199
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits -region wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.oon10X4vbF (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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
Checking if the catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat corresponding to the image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
WCS catalog name: wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2412, passed=52705
Got 52705 stars (including 50194 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat
util/solve_plate_with_UCAC5 got 52705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8495 through 0 to 14.7500, gap 14.7500 to 344.8495
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 48573 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 344.8497 through 0 to 14.7530, gap 14.7530 to 344.8497
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 48574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 48575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits N_match=958 sigma_overall_arcsec=0.748 sigma_q1_arcsec=0.822 sigma_q2_arcsec=0.686 sigma_q3_arcsec=0.640 sigma_q4_arcsec=0.793 n_q1=163 n_q2=253 n_q3=107 n_q4=435 worst_quadrant_to_overall_ratio=1.099
The image catalog is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits -region wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-10_20.00sec_4.90C_LIGHT_0202.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.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_2026-06-20_CI_Cas-04-Q2b1x1_010922_TTUQ2b1x1_1602846_aFobyCjJ/wcs_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203.fits
Preparing the HTML report for the field Cas-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:37:39.04 +52:02:27.6: 11.71 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:07:22.99 +50:57:09.2: 12.41 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:26:19.27 +56:47:27.1: 12.09 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:37:39.04 +52:02:27.6: 11.69 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:07:22.99 +50:57:09.2: 12.42 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.70 +/- 0.01
Forced photometry filter REJECTED candidate at 23:37:39.04 +52:02:27.6: ref_mag=11.70 +/- 0.01 new_mean_mag=12.6234 delta=-0.92 (need > 0.90)
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter REJECTED candidate at 00:07:22.99 +50:57:09.2: ref_mag=12.41 +/- 0.01 new_mean_mag=12.5262 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:06:47.68 +54:28:39.2: 12.74 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:26:19.27 +56:47:27.1: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry filter REJECTED candidate at 00:26:19.27 +56:47:27.1: ref_mag=12.10 +/- 0.01 new_mean_mag=11.8684 delta=0.23 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:14:22.07 +55:17:09.1: 12.53 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:24:18.31 +55:34:12.4: 12.98 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:06:47.68 +54:28:39.2: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.02
Forced photometry filter REJECTED candidate at 00:06:47.68 +54:28:39.2: ref_mag=12.73 +/- 0.02 new_mean_mag=12.4634 delta=0.26 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:22:20.39 +52:13:04.7: 13.29 +/- 0.04 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:03:20.55 +55:39:14.2: 12.62 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:01:09.83 +53:11:47.0: 13.09 +/- 0.05 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:14:22.07 +55:17:09.1: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:24:18.31 +55:34:12.4: 12.95 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 00:14:22.07 +55:17:09.1: ref_mag=12.52 +/- 0.01 new_mean_mag=12.4137 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter REJECTED candidate at 00:24:18.31 +55:34:12.4: ref_mag=12.96 +/- 0.02 new_mean_mag=12.6029 delta=0.36 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:04:40.13 +57:27:45.9: 12.87 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:22:20.39 +52:13:04.7: 13.23 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.03
Forced photometry filter REJECTED candidate at 00:22:20.39 +52:13:04.7: ref_mag=13.26 +/- 0.03 new_mean_mag=12.7439 delta=0.51 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:03:20.55 +55:39:14.2: 12.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Forced photometry filter REJECTED candidate at 00:03:20.55 +55:39:14.2: ref_mag=12.63 +/- 0.02 new_mean_mag=12.4608 delta=0.17 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:01:09.83 +53:11:47.0: 13.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.04
Forced photometry filter REJECTED candidate at 00:01:09.83 +53:11:47.0: ref_mag=13.10 +/- 0.04 new_mean_mag=12.6748 delta=0.42 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:04:40.13 +57:27:45.9: 12.85 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Forced photometry filter REJECTED candidate at 00:04:40.13 +57:27:45.9: ref_mag=12.86 +/- 0.02 new_mean_mag=12.8174 delta=0.04 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:27:59.20 +51:36:52.5: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:32:11.74 +50:01:12.0: 13.12 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:29:58.93 +53:42:32.6: 12.35 +/- 0.01 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:58:59.21 +54:51:07.6: 12.99 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:27:59.20 +51:36:52.5: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 00:27:59.20 +51:36:52.5: ref_mag=13.02 +/- 0.02 new_mean_mag=12.0704 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:19:48.83 +54:03:26.7: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 23:34:44.03 +50:31:11.5: 12.71 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:32:11.74 +50:01:12.0: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 23:32:11.74 +50:01:12.0: ref_mag=13.10 +/- 0.02 new_mean_mag=11.8419 delta=1.26 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:29:58.93 +53:42:32.6: 12.35 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter KEPT candidate at 00:29:58.93 +53:42:32.6: ref_mag=12.35 +/- 0.01 new_mean_mag=11.4439 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:02:03.87 +53:58:57.9: 13.30 +/- 0.03 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:58:59.21 +54:51:07.6: 13.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter KEPT candidate at 23:58:59.21 +54:51:07.6: ref_mag=13.01 +/- 0.02 new_mean_mag=12.0691 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:19:48.83 +54:03:26.7: 13.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.02
Forced photometry filter KEPT candidate at 00:19:48.83 +54:03:26.7: ref_mag=13.45 +/- 0.02 new_mean_mag=12.4895 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 23:34:44.03 +50:31:11.5: 12.66 +/- 0.02 detection
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-20-38_20.00sec_-14.90C_LIGHT_0006.fits at 00:18:42.86 +54:02:20.7: 14.30 +/- 0.08 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter KEPT candidate at 23:34:44.03 +50:31:11.5: ref_mag=12.68 +/- 0.01 new_mean_mag=11.5565 delta=1.12 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:02:03.87 +53:58:57.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter KEPT candidate at 00:02:03.87 +53:58:57.9: ref_mag=13.30 +/- 0.02 new_mean_mag=12.1701 delta=1.13 (need > 0.90)
Forced photometry on wcs_Cas-04-Q2b1x1_2026-02-10_20-21-47_20.00sec_-15.00C_LIGHT_0007.fits at 00:18:42.86 +54:02:20.7: 14.37 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.06
Forced photometry filter KEPT candidate at 00:18:42.86 +54:02:20.7: ref_mag=14.33 +/- 0.06 new_mean_mag=13.0767 delta=1.25 (need > 0.90)
Adding exclusion_list_local.txt__out109046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98268.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: 4s
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Considering the candidate 243661_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 243661_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:01:22.80 +56:07:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243667_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 243667_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
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Considering the candidate 243670_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 243670_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
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Considering the candidate 243675_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 243675_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:21:25.92 +52:06:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243678_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 243678_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:23:29.19 +54:55:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243680_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 243680_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:23:09.38 +54:34:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243907_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 243907_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 243919_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 243919_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 244966_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 244966_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 245166_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 245166_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:06:03.00 +55:12:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247070_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 247070_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
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Considering the candidate 247103_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 247103_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:14:58.21 +53:15:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247745_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 247745_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 248315_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 248315_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:24:15.01 +51:59:53.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248330_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 248330_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 23:59:16.08 +55:57:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248420_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 248420_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:04:19.32 +54:17:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248658_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 248658_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 23:55:26.71 +58:05:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248713_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 248713_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:26:03.96 +56:47:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248829_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 248829_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:31:47.08 +56:53:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249202_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 249202_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:24:12.83 +57:39:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249367_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 249367_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:23:03.54 +55:45:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249639_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 249639_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 249779_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 249779_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
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Considering the candidate 249795_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 249795_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:22:44.32 +57:06:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250207_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 250207_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 23:57:10.91 +55:44:00.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 250372_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 250372_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:24:36.81 +56:59:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 250599_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 250599_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
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Considering the candidate 250892_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 250892_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
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Considering the candidate 250990_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 250990_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 23:38:48.27 +52:15:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251029_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 251029_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:16:30.35 +53:57:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251068_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 251068_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 251608_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 251608_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
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Considering the candidate 251797_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 251797_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 23:54:36.42 +57:28:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251812_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 251812_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:22:38.40 +54:16:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251822_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 251822_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
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Considering the candidate 252238_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 252238_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:24:57.64 +53:01:58.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 252865_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 252865_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
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Considering the candidate 252889_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 252889_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:02:36.55 +55:35:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 252952_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 252952_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
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Considering the candidate 253163_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 253163_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 23:55:17.47 +58:06:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253599_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 253599_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:18:54.41 +53:18:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254305_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 254305_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:05:04.57 +56:02:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254322_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 254322_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:27:21.96 +54:05:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166100_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 166100_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:21:20.39 +51:21:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157793_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
Preparing report for the candidate 157793_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
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Considering the candidate 79234_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 79234_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:04:40.65 +55:32:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168527_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
Preparing report for the candidate 168527_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
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Considering the candidate 111591_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
Preparing report for the candidate 111591_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
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Considering the candidate 179137_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 179137_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:20:53.26 +50:09:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98268_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
Preparing report for the candidate 98268_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
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Considering the candidate 109046_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
Preparing report for the candidate 109046_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
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Considering the candidate 177194_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
Preparing report for the candidate 177194_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
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Considering the candidate 117774_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
Preparing report for the candidate 117774_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
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Considering the candidate 119320_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 119320_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
**** FOUND 00:18:33.33 +53:39:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143637_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203
The candidate 143637_fd_Cas-04-Q2b1x1_2026-06-20_01-04-49_20.00sec_5.00C_LIGHT_0203 did not pass the final checks
