This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,6.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 6.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4008 2461334.9008 10.81 08:42:17.66 +18:19:22.0
207.59706 32.42947 galactic Cnc Second-epoch detections are separated by 0.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.27 Euterpe 1 -0 1 11.1 0 -0
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:42:17.66 +18:19:22.0: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:42:17.66 +18:19:22.0: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 10.81CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,7.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 7.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4008 2461334.9008 12.84 08:42:21.93 +13:55:28.8
212.38358 30.77731 galactic Cnc Second-epoch detections are separated by 0.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.202 Chryseis 0 -0 0 13.1 0 -0
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:42:21.93 +13:55:28.8: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:42:21.93 +13:55:28.8: 16.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4008 2461334.9008 12.86 09:09:46.05 +09:00:59.3
221.06023 34.77590 galactic Cnc Second-epoch detections are separated by 1.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.12 Victoria 1 -0 1 12.9 0 0
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 09:09:46.05 +09:00:59.3: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 09:09:46.05 +09:00:59.3: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4008 2461334.9008 13.21 08:27:07.76 +14:29:27.0
210.10667 27.61405 galactic Cnc Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.114 Kassandra 1 -1 1 13.4 -0 0
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:27:07.76 +14:29:27.0: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:27:07.76 +14:29:27.0: 15.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4008 2461334.9008 13.37 08:25:55.54 +18:54:24.5
205.34002 29.02097 galactic Cnc Second-epoch detections are separated by 1.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.779 Nina 1 -1 1 13.6 0 0
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:25:55.54 +18:54:24.5: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:25:55.54 +18:54:24.5: 15.72 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4008 2461334.9008 13.53 08:49:42.86 +10:57:35.1
216.39722 31.18922 galactic Cnc Second-epoch detections are separated by 1.4" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.405 Thia 0 0 0 13.9 -0 0
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:49:42.86 +10:57:35.1: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:49:42.86 +10:57:35.1: 15.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4008 2461334.9008 13.80 08:58:01.77 +12:42:56.8
215.51659 33.77207 galactic Cnc Second-epoch detections are separated by 2.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.305 Gordonia 1 1 1 14.0 -0 0
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:58:01.77 +12:42:56.8: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:58:01.77 +12:42:56.8: 16.08 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4008 2461334.9008 14.20 08:54:30.96 +14:49:03.5
212.78767 33.83332 galactic Cnc Second-epoch detections are separated by 2.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.50 Virginia -0 -1 1 14.5 -0 0
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:54:30.96 +14:49:03.5: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:54:30.96 +14:49:03.5: 16.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4008 2461334.9008 14.34 08:40:59.72 +10:12:18.0
216.12630 28.92965 galactic Cnc Second-epoch detections are separated by 4.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.56 Melete 0 0 0 14.5 0 0
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:40:59.72 +10:12:18.0: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:40:59.72 +10:12:18.0: 15.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4008 2461334.9008 14.31 09:03:52.42 +16:53:38.2
211.48053 36.70322 galactic Cnc Second-epoch detections are separated by 1.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.931 Whittemora 1 -1 2 14.6 0 0
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 09:03:52.42 +16:53:38.2: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 09:03:52.42 +16:53:38.2: 15.71 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.71 +/- 0.28
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461334.9008,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4008 14.31CV 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: 2461093.74344014 22.02.2026 05:50:23.228 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
First image: 2461093.74344014 22.02.2026 05:50:23.228 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Last image: 2461334.90112416 21.10.2026 09:37:27.127 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 10261
Objects passed selection criteria: 10254
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 10044.5
Average stars matched: 9949 (99.0492 %)
Memory usage VmPeak: 236764 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 21 04:40:24 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: 2461093.74344014 22.02.2026 05:50:23.228 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
First image: 2461093.74344014 22.02.2026 05:50:23.228 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Last image: 2461334.90112416 21.10.2026 09:37:27.127 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 54
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.10
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: 21 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 56917
Objects passed selection criteria: 56801
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 51248.5
Average stars matched: 49767.8 (97.1106 %)
Memory usage VmPeak: 278080 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 21 04:41:38 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
SExtractor catalog cache: saved Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.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/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461334.90050887
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_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits exists and is non-empty
wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits exists and is non-empty
wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits exists and is non-empty
wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (1st reference image)
verification OK: wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Image size: 937.7'x624.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:53:21.014 +14:00:00.07 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits (1st new image)
verification OK: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
Image size: 941.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:53:12.656 +14:03:11.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:53:21.014 +14:00:00.07
Second-epoch image center 08:53:12.656 +14:03:11.09
Angular distance between the image centers 0.0629 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits (2nd new image)
verification OK: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Image size: 941.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:53:10.145 +14:03:00.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:53:21.014 +14:00:00.07
Second-epoch image center 08:53:10.145 +14:03:00.28
Angular distance between the image centers 0.0666 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 08:53:12.656 +14:03:11.09
Second-epoch second image center 08:53:10.145 +14:03:00.28
Angular distance between the image centers 0.01058 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits &> /tmp/tmp.vN6FqeMdWM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits &> /tmp/tmp.IRE4pPAWVW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits &> /tmp/tmp.FyLYRDrvJz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits &> /tmp/tmp.qvEp4SHYkz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.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_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.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_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
Found non-empty wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
The reference image (wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits) and catalog (wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat) found
'wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat' -> 'wcsmag.cat'
Read 12501 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0576 to 141.9546 deg, Dec +8.1318 to +19.6232 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 125.0576 to 141.9546 deg, Dec 8.1318 to 19.6232 deg
Loaded 7593 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): 5630 out of 5966 total matches.
Matched with Tycho-2 5966 out of 12501 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.982950
a=0.000000 b=1.000000 c=22.982950
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 12501 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0576 to 141.9546 deg, Dec +8.1318 to +19.6232 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 125.0576 to 141.9546 deg, Dec 8.1318 to 19.6232 deg
Loaded 7593 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): 5630 out of 5966 total matches.
Matched with Tycho-2 5966 out of 12501 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Forced-photometry filter: calibrated wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits -> calib.txt_param_ref_wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (aperture=6.6)
Read 9951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0604 to 141.9546 deg, Dec +8.1147 to +19.5889 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 125.0604 to 141.9546 deg, Dec 8.1147 to 19.5889 deg
Loaded 7587 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): 5641 out of 5951 total matches.
Matched with Tycho-2 5951 out of 9951 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Forced-photometry filter: calibrated wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits -> calib.txt_param_ref_wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
2.2 pix Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
3.3 pix fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
3.2 pix fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Limiting magnitude estimates:
15.6 mag. Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
15.4 mag. Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
15.0 mag. fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
15.0 mag. fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.vN6FqeMdWM (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/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.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_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits' -> 'wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Checking if the catalog wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS catalog name: wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=855, bad_region=0, passed=12501
Got 12501 stars (including 11641 good ones) from the SExtractor catalog wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
util/solve_plate_with_UCAC5 got 12501 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 4875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 12501 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 12501 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4875 matched stars entering correct_measured_positions(), 12501 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4875 stars left (next iteration limit 5362)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits N_match=4875 sigma_overall_arcsec=0.400 sigma_q1_arcsec=0.276 sigma_q2_arcsec=0.516 sigma_q3_arcsec=0.342 sigma_q4_arcsec=0.448 n_q1=1004 n_q2=1452 n_q3=945 n_q4=1474 worst_quadrant_to_overall_ratio=1.290
WCS_HEADER_DIAG: file=Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits selection=current_pairs N_selected=4875 N_valid=4875 bias_ra_arcsec=-0.010 bias_dec_arcsec=-0.012 median_sep_arcsec=0.309 p95_sep_arcsec=1.785 n_q1=1004 n_q2=1452 n_q3=945 n_q4=1474 occupied_cells_4x4=16/16
The image catalog is written to wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits -region wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.IRE4pPAWVW (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits' -> 'wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS-calibrated image found: wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Checking if the catalog wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat corresponding to the image wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat corresponding to the image wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS catalog name: wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=759, bad_region=0, passed=9951
Got 9951 stars (including 9175 good ones) from the SExtractor catalog wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat
util/solve_plate_with_UCAC5 got 9951 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 4866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 9951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 9951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 9951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4865 stars left (next iteration limit 5352)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits N_match=4865 sigma_overall_arcsec=0.317 sigma_q1_arcsec=0.359 sigma_q2_arcsec=0.330 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.294 n_q1=1014 n_q2=1350 n_q3=1022 n_q4=1479 worst_quadrant_to_overall_ratio=1.132
WCS_HEADER_DIAG: file=Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits selection=current_pairs N_selected=4865 N_valid=4865 bias_ra_arcsec=0.006 bias_dec_arcsec=-0.002 median_sep_arcsec=0.270 p95_sep_arcsec=0.859 n_q1=1014 n_q2=1350 n_q3=1022 n_q4=1479 occupied_cells_4x4=16/16
The image catalog is written to wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits -region wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.FyLYRDrvJz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
Checking if the catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
WCS catalog name: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=455, bad_region=0, passed=8974
Got 8974 stars (including 8512 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat
util/solve_plate_with_UCAC5 got 8974 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 549 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 4870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 8974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 549 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 8974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 8974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 4871 stars left (next iteration limit 5357)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4871 robust_rms=11.949 arcsec worst_region_rms=29.460 arcsec outer_annulus_rms=29.460 arcsec
SIP_REFIT: SIP order 3 trial: matched=4871 robust_rms=0.408 arcsec worst_region_rms=0.743 arcsec outer_annulus_rms=0.743 arcsec
SIP_REFIT: SIP order 5 trial: matched=4871 robust_rms=0.260 arcsec worst_region_rms=0.402 arcsec outer_annulus_rms=0.402 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4871 robust_rms_before=1.000 arcsec robust_rms_before_corrected=0.260 arcsec robust_rms_after=0.260 arcsec worst_region_rms_before=0.435 worst_region_rms_after=0.402 outer_annulus_rms_before=1.214 outer_annulus_rms_after=0.402
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.435 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits worst_region_rms_kept=0.435 arcsec robust_rms_kept=0.260 arcsec matched=4871
WCS_QUALITY_DIAG: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits N_match=4871 sigma_overall_arcsec=0.263 sigma_q1_arcsec=0.302 sigma_q2_arcsec=0.319 sigma_q3_arcsec=0.220 sigma_q4_arcsec=0.235 n_q1=1547 n_q2=909 n_q3=1443 n_q4=972 worst_quadrant_to_overall_ratio=1.215
WCS_HEADER_DIAG: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits selection=current_pairs N_selected=4871 N_valid=4871 bias_ra_arcsec=0.617 bias_dec_arcsec=0.528 median_sep_arcsec=0.933 p95_sep_arcsec=1.896 n_q1=1547 n_q2=909 n_q3=1443 n_q4=972 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits -region wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.qvEp4SHYkz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Checking if the catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
WCS catalog name: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=442, bad_region=0, passed=9000
Got 9000 stars (including 8549 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat
util/solve_plate_with_UCAC5 got 9000 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 549 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 4873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 9000 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 549 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 9000 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 9000 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4873 stars left (next iteration limit 5360)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4873 robust_rms=11.897 arcsec worst_region_rms=29.194 arcsec outer_annulus_rms=29.194 arcsec
SIP_REFIT: SIP order 3 trial: matched=4873 robust_rms=0.397 arcsec worst_region_rms=0.731 arcsec outer_annulus_rms=0.731 arcsec
SIP_REFIT: SIP order 5 trial: matched=4873 robust_rms=0.269 arcsec worst_region_rms=0.406 arcsec outer_annulus_rms=0.406 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4873 robust_rms_before=0.991 arcsec robust_rms_before_corrected=0.257 arcsec robust_rms_after=0.269 arcsec worst_region_rms_before=0.429 worst_region_rms_after=0.406 outer_annulus_rms_before=1.187 outer_annulus_rms_after=0.406
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.429 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits worst_region_rms_kept=0.429 arcsec robust_rms_kept=0.257 arcsec matched=4873
WCS_QUALITY_DIAG: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits N_match=4873 sigma_overall_arcsec=0.264 sigma_q1_arcsec=0.285 sigma_q2_arcsec=0.302 sigma_q3_arcsec=0.228 sigma_q4_arcsec=0.248 n_q1=1544 n_q2=914 n_q3=1438 n_q4=977 worst_quadrant_to_overall_ratio=1.143
WCS_HEADER_DIAG: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits selection=current_pairs N_selected=4873 N_valid=4873 bias_ra_arcsec=0.608 bias_dec_arcsec=0.549 median_sep_arcsec=0.930 p95_sep_arcsec=1.847 n_q1=1544 n_q2=914 n_q3=1438 n_q4=977 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits -region wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits to local_wcs_cache/
'wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits'
Saving the final (post-refit) wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits to local_wcs_cache/
'wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits'
Saving the final (post-refit) wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits'
Saving the final (post-refit) wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits sigma_overall=0.400 worst_q_ratio=1.290
ref2=Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits sigma_overall=0.317 worst_q_ratio=1.132
new1=fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits sigma_overall=0.263 worst_q_ratio=1.215
new2=fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits sigma_overall=0.264 worst_q_ratio=1.143
reference average sigma_overall=0.3585 worst_q_ratio=1.211
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187_astrometric_residuals.png (4875 matched stars from wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114_astrometric_residuals.png (4865 matched stars from wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398_astrometric_residuals.png (4871 matched stars from wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399_astrometric_residuals.png (4873 matched stars from wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits'
Saving fully-calibrated image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits'
Preparing the HTML report for the field Cnc-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:42:17.66 +18:19:22.0: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:45:35.48 +15:50:44.3: 12.13 +/- 0.01 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:42:17.66 +18:19:22.0: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:45:35.48 +15:50:44.3: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter REJECTED candidate at 08:45:35.48 +15:50:44.3: ref_mag=12.17 +/- 0.01 new_mean_mag=12.4205 delta=-0.25 (need > 0.90)
Adding exclusion_list_local.txt__out20245.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20185_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 20185_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20187_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 20187_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:32:49.04 +10:16:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20188_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 20188_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20245_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 20245_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20276_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 20276_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:31:45.94 +18:59:43.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Cnc-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:42:17.66 +18:19:22.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
SExtractor catalog cache: saved Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Creating symlink local_wcs_cache/wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits exists and is non-empty
wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits exists and is non-empty
wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits exists and is non-empty
wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (1st reference image)
verification OK: wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Image size: 937.7'x624.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:53:21.014 +14:00:00.07 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits (1st new image)
verification OK: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
Image size: 941.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:53:12.656 +14:03:11.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:53:21.014 +14:00:00.07
Second-epoch image center 08:53:12.656 +14:03:11.09
Angular distance between the image centers 0.0629 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits (2nd new image)
verification OK: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Image size: 941.6'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:53:10.145 +14:03:00.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:53:21.014 +14:00:00.07
Second-epoch image center 08:53:10.145 +14:03:00.28
Angular distance between the image centers 0.0666 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 08:53:12.656 +14:03:11.09
Second-epoch second image center 08:53:10.145 +14:03:00.28
Angular distance between the image centers 0.01058 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits &> /tmp/tmp.w9P5KjpZOE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits &> /tmp/tmp.HKBGGI950V
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits &> /tmp/tmp.S8HkotTAU6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits &> /tmp/tmp.LEtPjIsZGY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.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_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.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_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
Found non-empty wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
The reference image (wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits) and catalog (wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat) found
'wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat' -> 'wcsmag.cat'
Read 63179 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0577 to 141.9546 deg, Dec +8.1206 to +19.6320 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 125.0577 to 141.9546 deg, Dec 8.1206 to 19.6320 deg
Loaded 7608 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): 5179 out of 5984 total matches.
Matched with Tycho-2 5984 out of 63179 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.869500
a=0.000000 b=1.000000 c=22.869500
From vast_summary.log: estimated ref. image limiting mag.: -7.10
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.77
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.77
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 63179 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0577 to 141.9546 deg, Dec +8.1206 to +19.6320 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 125.0577 to 141.9546 deg, Dec 8.1206 to 19.6320 deg
Loaded 7608 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): 5179 out of 5984 total matches.
Matched with Tycho-2 5984 out of 63179 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Forced-photometry filter: calibrated wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits -> calib.txt_param_ref_wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (aperture=5.2)
Read 59553 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0604 to 141.9546 deg, Dec +8.1147 to +19.5889 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 125.0604 to 141.9546 deg, Dec 8.1147 to 19.5889 deg
Loaded 7587 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): 5243 out of 6043 total matches.
Matched with Tycho-2 6043 out of 59553 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Forced-photometry filter: calibrated wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits -> calib.txt_param_ref_wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 50 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
2.0 pix Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
3.1 pix fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
3.0 pix fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Limiting magnitude estimates:
15.8 mag. Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
15.6 mag. Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
15.0 mag. fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
15.0 mag. fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.w9P5KjpZOE (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/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.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_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits' -> 'wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Checking if the catalog wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS catalog name: wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=4250, bad_region=0, passed=63153
Got 63153 stars (including 58843 good ones) from the SExtractor catalog wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
util/solve_plate_with_UCAC5 got 63153 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 4874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 63153 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 63153 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 63153 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4874 stars left (next iteration limit 5361)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits N_match=4874 sigma_overall_arcsec=0.386 sigma_q1_arcsec=0.271 sigma_q2_arcsec=0.492 sigma_q3_arcsec=0.336 sigma_q4_arcsec=0.441 n_q1=1027 n_q2=1432 n_q3=938 n_q4=1477 worst_quadrant_to_overall_ratio=1.275
WCS_HEADER_DIAG: file=Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits selection=current_pairs N_selected=4874 N_valid=4874 bias_ra_arcsec=-0.016 bias_dec_arcsec=-0.002 median_sep_arcsec=0.300 p95_sep_arcsec=1.720 n_q1=1027 n_q2=1432 n_q3=938 n_q4=1477 occupied_cells_4x4=16/16
The image catalog is written to wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits -region wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.HKBGGI950V (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits' -> 'wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS-calibrated image found: wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Checking if the catalog wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat corresponding to the image wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat corresponding to the image wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS catalog name: wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=3477, bad_region=30, passed=59531
Got 59531 stars (including 55925 good ones) from the SExtractor catalog wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat
util/solve_plate_with_UCAC5 got 59531 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4871 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 4862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 59531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 59531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 59531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4861 stars left (next iteration limit 5348)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits N_match=4861 sigma_overall_arcsec=0.306 sigma_q1_arcsec=0.331 sigma_q2_arcsec=0.322 sigma_q3_arcsec=0.277 sigma_q4_arcsec=0.282 n_q1=1010 n_q2=1336 n_q3=1044 n_q4=1471 worst_quadrant_to_overall_ratio=1.084
WCS_HEADER_DIAG: file=Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits selection=current_pairs N_selected=4861 N_valid=4861 bias_ra_arcsec=-0.011 bias_dec_arcsec=0.008 median_sep_arcsec=0.262 p95_sep_arcsec=0.853 n_q1=1010 n_q2=1336 n_q3=1044 n_q4=1471 occupied_cells_4x4=16/16
The image catalog is written to wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits -region wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.S8HkotTAU6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
Checking if the catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
WCS catalog name: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1918, bad_region=47, passed=41876
Got 41876 stars (including 39859 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat
util/solve_plate_with_UCAC5 got 41876 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 549 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 4863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 41876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 549 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4875 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 41876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 41876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4863 stars left (next iteration limit 5349)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4863 robust_rms=11.896 arcsec worst_region_rms=29.508 arcsec outer_annulus_rms=29.508 arcsec
SIP_REFIT: SIP order 3 trial: matched=4863 robust_rms=0.413 arcsec worst_region_rms=0.713 arcsec outer_annulus_rms=0.713 arcsec
SIP_REFIT: SIP order 5 trial: matched=4863 robust_rms=0.260 arcsec worst_region_rms=0.395 arcsec outer_annulus_rms=0.395 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4863 robust_rms_before=1.000 arcsec robust_rms_before_corrected=0.254 arcsec robust_rms_after=0.260 arcsec worst_region_rms_before=0.427 worst_region_rms_after=0.395 outer_annulus_rms_before=1.207 outer_annulus_rms_after=0.395
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.427 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits worst_region_rms_kept=0.427 arcsec robust_rms_kept=0.254 arcsec matched=4863
WCS_QUALITY_DIAG: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits N_match=4863 sigma_overall_arcsec=0.258 sigma_q1_arcsec=0.283 sigma_q2_arcsec=0.313 sigma_q3_arcsec=0.219 sigma_q4_arcsec=0.237 n_q1=1520 n_q2=897 n_q3=1464 n_q4=982 worst_quadrant_to_overall_ratio=1.212
WCS_HEADER_DIAG: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits selection=current_pairs N_selected=4863 N_valid=4863 bias_ra_arcsec=0.626 bias_dec_arcsec=0.517 median_sep_arcsec=0.933 p95_sep_arcsec=1.873 n_q1=1520 n_q2=897 n_q3=1464 n_q4=982 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits -region wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.LEtPjIsZGY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Checking if the catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
WCS catalog name: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=2005, bad_region=48, passed=42020
Got 42020 stars (including 39915 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat
util/solve_plate_with_UCAC5 got 42020 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 549 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 4863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 42020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 549 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 42020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4863 matched stars entering correct_measured_positions(), 42020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4863 stars left (next iteration limit 5349)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4863 robust_rms=11.941 arcsec worst_region_rms=29.276 arcsec outer_annulus_rms=29.276 arcsec
SIP_REFIT: SIP order 3 trial: matched=4863 robust_rms=0.405 arcsec worst_region_rms=0.687 arcsec outer_annulus_rms=0.687 arcsec
SIP_REFIT: SIP order 5 trial: matched=4863 robust_rms=0.269 arcsec worst_region_rms=0.397 arcsec outer_annulus_rms=0.397 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4863 robust_rms_before=0.993 arcsec robust_rms_before_corrected=0.255 arcsec robust_rms_after=0.269 arcsec worst_region_rms_before=0.417 worst_region_rms_after=0.397 outer_annulus_rms_before=1.178 outer_annulus_rms_after=0.397
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.417 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits worst_region_rms_kept=0.417 arcsec robust_rms_kept=0.255 arcsec matched=4863
WCS_QUALITY_DIAG: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits N_match=4863 sigma_overall_arcsec=0.262 sigma_q1_arcsec=0.284 sigma_q2_arcsec=0.298 sigma_q3_arcsec=0.225 sigma_q4_arcsec=0.252 n_q1=1515 n_q2=906 n_q3=1464 n_q4=978 worst_quadrant_to_overall_ratio=1.135
WCS_HEADER_DIAG: file=fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits selection=current_pairs N_selected=4863 N_valid=4863 bias_ra_arcsec=0.614 bias_dec_arcsec=0.531 median_sep_arcsec=0.925 p95_sep_arcsec=1.832 n_q1=1515 n_q2=906 n_q3=1464 n_q4=978 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits -region wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-36-33_20.00sec_-0.00C_LIGHTs_0398.fits
Saving fully-calibrated image wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Cnc-05-Q1b1x1_043812_TTUQ1b1x1_780982_RySMzr0t/wcs_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399.fits
Preparing the HTML report for the field Cnc-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:41:05.73 +17:05:05.6: 14.82 +/- 0.11 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:29:09.16 +12:23:07.4: 14.74 +/- 0.11 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:27:07.76 +14:29:27.0: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 09:09:46.05 +09:00:59.3: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:42:21.93 +13:55:28.8: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 09:13:21.67 +11:57:11.3: 13.16 +/- 0.03 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:29:09.16 +12:23:07.4: 14.85 +/- 0.15 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:25:55.54 +18:54:24.5: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:41:05.73 +17:05:05.6: 14.69 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.09
Forced photometry filter REJECTED candidate at 08:29:09.16 +12:23:07.4: ref_mag=14.78 +/- 0.09 new_mean_mag=14.5865 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 14.76 +/- 0.08
Forced photometry filter REJECTED candidate at 08:41:05.73 +17:05:05.6: ref_mag=14.76 +/- 0.08 new_mean_mag=14.6838 delta=0.07 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:27:07.76 +14:29:27.0: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 09:09:46.05 +09:00:59.3: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:42:21.93 +13:55:28.8: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:49:42.86 +10:57:35.1: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:25:27.89 +14:25:46.8: 13.76 +/- 0.05 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:25:55.54 +18:54:24.5: 15.72 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 09:13:21.67 +11:57:11.3: 12.98 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter REJECTED candidate at 09:13:21.67 +11:57:11.3: ref_mag=13.07 +/- 0.02 new_mean_mag=13.2519 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:25:27.89 +14:25:46.8: 13.77 +/- 0.06 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:49:42.86 +10:57:35.1: 15.99 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter REJECTED candidate at 08:25:27.89 +14:25:46.8: ref_mag=13.76 +/- 0.04 new_mean_mag=13.7326 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:58:01.77 +12:42:56.8: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:28:08.18 +11:41:41.5: 13.59 +/- 0.05 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:29:49.53 +15:32:55.6: 13.85 +/- 0.05 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:58:01.77 +12:42:56.8: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:28:08.18 +11:41:41.5: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.65 +/- 0.04
Forced photometry filter REJECTED candidate at 08:28:08.18 +11:41:41.5: ref_mag=13.65 +/- 0.04 new_mean_mag=13.7176 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:26:38.45 +19:02:41.6: 14.43 +/- 0.10 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:29:49.53 +15:32:55.6: 13.86 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Forced photometry filter REJECTED candidate at 08:29:49.53 +15:32:55.6: ref_mag=13.85 +/- 0.04 new_mean_mag=13.7447 delta=0.11 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:26:38.45 +19:02:41.6: 14.16 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.07
Forced photometry filter REJECTED candidate at 08:26:38.45 +19:02:41.6: ref_mag=14.28 +/- 0.07 new_mean_mag=13.9893 delta=0.29 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:22:07.27 +17:58:36.7: 14.64 +/- 0.13 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:54:30.96 +14:49:03.5: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:22:07.27 +17:58:36.7: 14.55 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.09
Forced photometry filter REJECTED candidate at 08:22:07.27 +17:58:36.7: ref_mag=14.59 +/- 0.09 new_mean_mag=14.2663 delta=0.32 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:40:59.72 +10:12:18.0: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:30:22.20 +19:11:45.2: 14.90 +/- 0.14 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:54:30.96 +14:49:03.5: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:40:59.72 +10:12:18.0: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:30:22.20 +19:11:45.2: 15.02 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.95 +/- 0.11
Forced photometry filter REJECTED candidate at 08:30:22.20 +19:11:45.2: ref_mag=14.95 +/- 0.11 new_mean_mag=14.6012 delta=0.35 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:22:53.16 +15:05:29.3: 15.07 +/- 0.17 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:22:53.16 +15:05:29.3: 14.95 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.12
Forced photometry filter REJECTED candidate at 08:22:53.16 +15:05:29.3: ref_mag=15.01 +/- 0.12 new_mean_mag=14.5858 delta=0.42 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 09:03:52.42 +16:53:38.2: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 09:03:52.42 +16:53:38.2: 15.71 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.71 +/- 0.28
Forced photometry filter KEPT candidate at 09:03:52.42 +16:53:38.2: ref_mag=15.71 +/- 0.28 new_mean_mag=14.3091 delta=1.40 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:22:49.01 +18:31:40.2: 15.17 +/- 0.20 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:22:49.01 +18:31:40.2: 15.00 +/- 0.18 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.14
Forced photometry filter REJECTED candidate at 08:22:49.01 +18:31:40.2: ref_mag=15.08 +/- 0.14 new_mean_mag=14.6542 delta=0.42 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:22:10.46 +15:53:40.0: 15.16 +/- 0.20 detection
Forced photometry on wcs_Cnc-05-Q1b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:22:10.46 +15:53:40.0: 15.06 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.10 +/- 0.14
Forced photometry filter REJECTED candidate at 08:22:10.46 +15:53:40.0: ref_mag=15.10 +/- 0.14 new_mean_mag=14.7168 delta=0.39 (need > 0.90)
Adding exclusion_list_local.txt__out77433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78227.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
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: 9s
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Considering the candidate 77107_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77107_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 77110_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77110_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 77126_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77126_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:48:14.07 +11:33:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77129_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77129_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:23:56.06 +18:30:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77136_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77136_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:22:56.27 +16:47:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77138_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77138_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 09:15:09.28 +13:50:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77139_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 77139_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
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Considering the candidate 77196_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77196_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:42:17.66 +18:19:22.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 77232_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77232_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:31:45.95 +18:59:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77369_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77369_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:25:14.01 +11:55:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77382_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77382_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 09:08:21.07 +13:11:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77413_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77413_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:44:40.02 +10:06:15.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 77433_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 77433_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
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Considering the candidate 77490_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 77490_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
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Considering the candidate 77517_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77517_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:49:32.74 +12:08:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77530_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 77530_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
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Considering the candidate 77573_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77573_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 09:12:51.68 +17:27:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77596_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 77596_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
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Considering the candidate 77615_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77615_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 77654_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77654_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:43:08.98 +14:05:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77677_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77677_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:22:30.29 +13:09:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77683_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 77683_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
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Considering the candidate 77751_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77751_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 77832_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77832_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:49:56.35 +14:48:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77850_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77850_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:36:13.22 +15:18:03.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 77857_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 77857_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
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Considering the candidate 77873_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77873_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 09:05:14.13 +14:15:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77880_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77880_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 77883_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77883_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 77901_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77901_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 09:09:49.97 +10:12:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77922_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77922_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 77941_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77941_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:37:49.43 +09:09:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77966_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77966_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:42:55.49 +14:05:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77978_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 77978_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:50:06.03 +17:51:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78014_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 78014_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 09:01:31.11 +15:10:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78027_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 78027_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 78059_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 78059_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:55:12.59 +16:14:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78063_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 78063_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:37:49.91 +17:15:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78142_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 78142_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:57:41.48 +16:32:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78148_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 78148_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
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Considering the candidate 78157_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 78157_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 08:52:30.08 +18:02:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78178_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 78178_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
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Considering the candidate 78222_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 78222_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 78226_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 78226_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 78227_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
Preparing report for the candidate 78227_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
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Considering the candidate 78241_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 78241_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 78342_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 78342_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
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Considering the candidate 50284_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 50284_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
**** FOUND 09:09:52.05 +09:48:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46719_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 46719_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
Rejecting candidate due to large distance (39.2") between the two second-epoch detections
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Considering the candidate 02505_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399
The candidate 02505_fd_Cnc-05-Q1b1x1_2026-10-21_04-37-27_20.00sec_-0.00C_LIGHTs_0399 did not pass the final checks
