This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 11.56 08:13:32.62 +22:38:05.1
200.22248 27.61426 galactic Cnc Second-epoch detections are separated by 1.6" 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.40 Harmonia -1 -0 1 11.6 -0 0
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:13:32.62 +22:38:05.1: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:13:32.62 +22:38:05.1: 16.26 +/- 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,2461186.6458,11.56,0.05,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 20260526.1458 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.25 08:04:03.65 +23:09:33.6
198.83532 25.74118 galactic Cnc Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:04:03.65 +23:09:33.6 (user input) | T | P | (position from user input) J-Ks=0.753+/-0.028 (K)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:04:03.65 +23:09:33.6: 13.33 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:04:03.65 +23:09:33.6: 13.26 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461186.6458,12.25,0.05,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
target 20260526.1458 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.24 07:50:48.94 +17:54:15.0
202.91659 20.92527 galactic Gem Second-epoch detections are separated by 0.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:50:48.94 +17:54:15.0 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5) J-Ks=0.349+/-0.030 (G)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:48.94 +17:54:15.0: 13.33 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:48.94 +17:54:15.0: 13.28 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461186.6458,12.24,0.05,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
target 20260526.1458 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.27 08:09:36.33 +23:00:13.9
199.48516 26.88617 galactic Cnc Second-epoch detections are separated by 0.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J122.4013+23.0037 | 08:09:36.33 +23:00:13.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.478+/-0.028 (K)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:09:36.33 +23:00:13.9: 13.36 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:09:36.33 +23:00:13.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J122.4013+23.0037,2461186.6458,12.27,0.05,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
ATO J122.4013+23.0037 20260526.1458 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.04 07:51:23.70 +17:22:29.7
203.49574 20.84549 galactic Gem Second-epoch detections are separated by 1.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:51:23.70 +17:22:29.7 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.392+/-0.028 (G)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:51:23.70 +17:22:29.7: 12.97 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:51:23.70 +17:22:29.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461186.6458,12.04,0.05,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
target 20260526.1458 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.06 08:12:43.54 +24:04:44.7
198.61303 27.91962 galactic Cnc Second-epoch detections are separated by 1.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J123.1819+24.0815 | 08:12:43.54 +24:04:44.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G1 (LAMOST DR5) J-Ks=0.314+/-0.028 (F)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:12:43.54 +24:04:44.7: 12.97 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:12:43.54 +24:04:44.7: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
ATO J123.1819+24.0815,2461186.6458,12.06,0.05,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
ATO J123.1819+24.0815 20260526.1458 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.26 08:06:09.45 +23:30:27.9
198.65414 26.31261 galactic Cnc Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:06:09.45 +23:30:27.9 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.239+/-0.027 (F)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:06:09.45 +23:30:27.9: 13.28 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:06:09.45 +23:30:27.9: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461186.6458,12.26,0.05,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
target 20260526.1458 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 11.97 07:50:04.53 +17:37:15.7
203.12178 20.65247 galactic Gem Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:50:04.53 +17:37:15.7 (user input) | T | P | (position from user input) J-Ks=0.637+/-0.029 (K)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:04.53 +17:37:15.7: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:04.53 +17:37:15.7: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461186.6458,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260526.1458 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 11.90 07:50:14.24 +17:21:44.9
203.39207 20.58655 galactic Gem Second-epoch detections are separated by 0.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 667921638492046592 | 07:50:14.19 +17:21:08.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5) J-Ks=0.611+/-0.028 (K)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:14.24 +17:21:44.9: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:14.24 +17:21:44.9: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 667921638492046592,2461186.6458,11.90,0.05,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
Gaia DR3 667921638492046592 20260526.1458 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.23 07:50:00.18 +17:58:46.3
202.76174 20.77661 galactic Gem Second-epoch detections are separated by 1.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:50:00.18 +17:58:46.3 (user input) | T | P | (position from user input) J-Ks=0.710+/-0.029 (K)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:00.18 +17:58:46.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:00.18 +17:58:46.3: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461186.6458,12.23,0.05,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
target 20260526.1458 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 11.91 07:48:35.44 +17:51:41.2
202.73776 20.42122 galactic Gem Second-epoch detections are separated by 1.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 668525373455485568 | 07:48:35.44 +17:51:41.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.614+/-0.029 (K)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:35.44 +17:51:41.2: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:35.44 +17:51:41.2: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 668525373455485568,2461186.6458,11.91,0.05,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
Large-amplitude variable Gaia DR2 668525373455485568 20260526.1458 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.15 07:50:42.68 +17:13:32.9
203.57384 20.63686 galactic Gem Second-epoch detections are separated by 1.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J117.6768+17.2187 | 07:50:42.68 +17:13:32.9 (user input) | NSINE (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.388+/-0.030 (G)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:42.68 +17:13:32.9: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:42.68 +17:13:32.9: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
ATO J117.6768+17.2187,2461186.6458,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J117.6768+17.2187 20260526.1458 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.40 07:47:39.62 +17:29:12.8
203.01221 20.07037 galactic Gem Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J116.9171+17.4862 | 07:47:39.62 +17:29:12.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G2 (LAMOST DR5) J-Ks=0.406+/-0.033 (G)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:39.62 +17:29:12.8: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:39.62 +17:29:12.8: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J116.9171+17.4862,2461186.6458,12.40,0.05,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
ATO J116.9171+17.4862 20260526.1458 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 11.80 07:51:12.49 +17:18:04.2
203.54960 20.77554 galactic Gem Second-epoch detections are separated by 1.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J117.8090+17.2974 | 07:51:12.49 +17:18:04.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G7 (LAMOST DR5) J-Ks=0.606+/-0.027 (K)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:51:12.49 +17:18:04.2: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:51:12.49 +17:18:04.2: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
ATO J117.8090+17.2974,2461186.6458,11.80,0.05,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
ATO J117.8090+17.2974 20260526.1458 11.80CV 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 05 26.1458 2461186.6458 12.11 07:50:14.96 +17:13:52.1
203.52224 20.53754 galactic Gem Second-epoch detections are separated by 0.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J117.5621+17.2309 | 07:50:14.96 +17:13:52.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.353+/-0.030 (G)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:14.96 +17:13:52.1: 13.12 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:14.96 +17:13:52.1: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J117.5621+17.2309,2461186.6458,12.11,0.05,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
ATO J117.5621+17.2309 20260526.1458 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.27 07:51:08.49 +17:14:32.1
203.60085 20.73776 galactic Gem Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:51:08.49 +17:14:32.1 (user input) | T | P | (position from user input) J-Ks=0.237+/-0.042 (F)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:51:08.49 +17:14:32.1: 13.40 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:51:08.49 +17:14:32.1: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461186.6458,12.27,0.05,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
target 20260526.1458 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.09 08:08:29.40 +23:03:29.1
199.33018 26.66332 galactic Cnc Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J122.1243+23.0706 | 08:08:29.40 +23:03:29.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: M2 (LAMOST DR5) J-Ks=0.384+/-0.033 (G)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:08:29.40 +23:03:29.1: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:08:29.40 +23:03:29.1: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
ATO J122.1243+23.0706,2461186.6458,12.09,0.05,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
ATO J122.1243+23.0706 20260526.1458 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 26.1458 2461186.6458 12.27 07:50:17.91 +17:19:39.7
203.43235 20.58631 galactic Gem Second-epoch detections are separated by 2.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:50:17.91 +17:19:39.7 (user input) | T | P | (position from user input) J-Ks=0.433+/-0.032 (G)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:17.91 +17:19:39.7: 13.32 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:17.91 +17:19:39.7: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461186.6458,12.27,0.05,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
target 20260526.1458 12.27CV 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: 2461093.70071369 22.02.2026 04:48:51.663 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
First image: 2461093.70071369 22.02.2026 04:48:51.663 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Last image: 2461186.64604025 26.05.2026 03:30:07.878 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 11602
Objects passed selection criteria: 11559
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 7748.5
Average stars matched: 6847.75 (88.3752 %)
Memory usage VmPeak: 118532 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 22:32:24 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: 2461093.70071369 22.02.2026 04:48:51.663 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
First image: 2461093.70071369 22.02.2026 04:48:51.663 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Last image: 2461186.64604025 26.05.2026 03:30:07.878 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 78
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.25
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 67580
Objects passed selection criteria: 67359
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 47216.2
Average stars matched: 43616.2 (92.3755 %)
Memory usage VmPeak: 174896 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 22:33:49 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461186.64553558
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits exists and is non-empty
Saving wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits to local_wcs_cache/
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits exists and is non-empty
Saving wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits to local_wcs_cache/
'wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits'
wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits'
wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits (1st reference image)
verification OK: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:18:25.645 +22:00:41.67 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits (1st new image)
verification OK: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.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: 08:18:36.652 +21:58:15.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:25.645 +22:00:41.67
Second-epoch image center 08:18:36.652 +21:58:15.17
Angular distance between the image centers 0.0589 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits (2nd new image)
verification OK: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.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: 08:18:39.345 +21:58:28.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:25.645 +22:00:41.67
Second-epoch image center 08:18:39.345 +21:58:28.56
Angular distance between the image centers 0.0646 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 08:18:36.652 +21:58:15.17
Second-epoch second image center 08:18:39.345 +21:58:28.56
Angular distance between the image centers 0.01105 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits &> /tmp/tmp.Q0JoRPoHXZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits &> /tmp/tmp.BWQhjxl9mh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits &> /tmp/tmp.Jm3BiPtTy9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits &> /tmp/tmp.fLNcaosocm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
The reference image (wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits) and catalog (wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat) found
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat' -> 'wcsmag.cat'
Read 13640 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.6697 to 133.2123 deg, Dec +16.3191 to +27.3546 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 115.6697 to 133.2123 deg, Dec 16.3191 to 27.3546 deg
Loaded 8746 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): 6706 out of 7199 total matches.
Matched with Tycho-2 7199 out of 13640 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.927500
a=0.000000 b=1.000000 c=22.927500
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.38
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 13640 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.6697 to 133.2123 deg, Dec +16.3191 to +27.3546 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 115.6697 to 133.2123 deg, Dec 16.3191 to 27.3546 deg
Loaded 8746 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): 6706 out of 7199 total matches.
Matched with Tycho-2 7199 out of 13640 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits:
Forced-photometry filter: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -> calib.txt_param_ref_wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits (aperture=6.2)
Read 15172 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 116.1034 to 133.7296 deg, Dec +16.1403 to +27.5041 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 116.1034 to 133.7296 deg, Dec 16.1403 to 27.5041 deg
Loaded 8883 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): 6662 out of 7094 total matches.
Matched with Tycho-2 7094 out of 15172 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits:
Forced-photometry filter: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits -> calib.txt_param_ref_wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
2.4 pix Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
2.1 pix fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
2.1 pix fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
2.1 pix wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
2.4 pix wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
Limiting magnitude estimates:
15.4 mag. Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
15.4 mag. Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
12.0 mag. fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
12.0 mag. fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
All-image limiting magnitude estimate: 12.0 (SNR ) 9.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Q0JoRPoHXZ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1109, passed=13640
Got 13640 stars (including 12518 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 13640 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
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 13354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 13354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 13355 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits N_match=979 sigma_overall_arcsec=0.358 sigma_q1_arcsec=0.467 sigma_q2_arcsec=0.345 sigma_q3_arcsec=0.331 sigma_q4_arcsec=0.304 n_q1=206 n_q2=300 n_q3=240 n_q4=233 worst_quadrant_to_overall_ratio=1.305
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BWQhjxl9mh (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-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.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-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.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-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1091, passed=15172
Got 15172 stars (including 14062 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat
util/solve_plate_with_UCAC5 got 15172 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 14955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 14957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 14957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits N_match=974 sigma_overall_arcsec=0.490 sigma_q1_arcsec=0.402 sigma_q2_arcsec=0.633 sigma_q3_arcsec=0.420 sigma_q4_arcsec=0.614 n_q1=225 n_q2=266 n_q3=248 n_q4=235 worst_quadrant_to_overall_ratio=1.293
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits -region wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Jm3BiPtTy9 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=85, passed=1109
Got 1109 stars (including 1023 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat
util/solve_plate_with_UCAC5 got 1109 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
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 589 (Dec 16.5 to 27.4)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 1065 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
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 589 (Dec 16.4 to 27.4)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 1066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 1066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits N_match=967 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.422 sigma_q2_arcsec=0.403 sigma_q3_arcsec=0.319 sigma_q4_arcsec=0.378 n_q1=127 n_q2=341 n_q3=132 n_q4=367 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fLNcaosocm (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=87, passed=1261
Got 1261 stars (including 1171 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat
util/solve_plate_with_UCAC5 got 1261 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
Reading UCAC5 zone files...
Searching UCAC5 zones 534 to 589 (Dec 16.8 to 27.4)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 1219 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 534 to 589 (Dec 16.8 to 27.4)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 1220 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 1220 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 970 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits N_match=970 sigma_overall_arcsec=0.384 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.392 sigma_q3_arcsec=0.348 sigma_q4_arcsec=0.396 n_q1=153 n_q2=322 n_q3=149 n_q4=346 worst_quadrant_to_overall_ratio=1.031
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits sigma_overall=0.358 worst_q_ratio=1.305
ref2=Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits sigma_overall=0.490 worst_q_ratio=1.293
new1=fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits sigma_overall=0.378 worst_q_ratio=1.116
new2=fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits sigma_overall=0.384 worst_q_ratio=1.031
reference average sigma_overall=0.424 worst_q_ratio=1.299
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174_astrometric_residuals.png (979 matched stars from wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177_astrometric_residuals.png (974 matched stars from wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042_astrometric_residuals.png (967 matched stars from wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043_astrometric_residuals.png (970 matched stars from wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits'
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits'
Preparing the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Creating symlink local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits exists and is non-empty
wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits exists and is non-empty
wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits exists and is non-empty
wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits (1st reference image)
verification OK: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:18:25.645 +22:00:41.67 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits (1st new image)
verification OK: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.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: 08:18:36.652 +21:58:15.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:25.645 +22:00:41.67
Second-epoch image center 08:18:36.652 +21:58:15.17
Angular distance between the image centers 0.0589 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits (2nd new image)
verification OK: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.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: 08:18:39.345 +21:58:28.56 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:25.645 +22:00:41.67
Second-epoch image center 08:18:39.345 +21:58:28.56
Angular distance between the image centers 0.0646 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 08:18:36.652 +21:58:15.17
Second-epoch second image center 08:18:39.345 +21:58:28.56
Angular distance between the image centers 0.01105 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits &> /tmp/tmp.buuUIeM0qz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits &> /tmp/tmp.8BFfkA51IN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits &> /tmp/tmp.DWaEOU1WmJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits &> /tmp/tmp.hNM10qffjh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
The reference image (wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits) and catalog (wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat) found
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat' -> 'wcsmag.cat'
Read 84357 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.6159 to 133.2123 deg, Dec +16.3191 to +27.3632 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 115.6159 to 133.2123 deg, Dec 16.3191 to 27.3632 deg
Loaded 8799 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): 5958 out of 7250 total matches.
Matched with Tycho-2 7250 out of 84357 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.798800
a=0.000000 b=1.000000 c=22.798800
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.55
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.55
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 84357 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.6159 to 133.2123 deg, Dec +16.3191 to +27.3632 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 115.6159 to 133.2123 deg, Dec 16.3191 to 27.3632 deg
Loaded 8799 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): 5958 out of 7250 total matches.
Matched with Tycho-2 7250 out of 84357 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits:
Forced-photometry filter: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -> calib.txt_param_ref_wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits (aperture=4.7)
Read 81224 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 116.0970 to 133.7295 deg, Dec +16.1151 to +27.5040 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 116.0970 to 133.7295 deg, Dec 16.1151 to 27.5040 deg
Loaded 8913 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): 5998 out of 7116 total matches.
Matched with Tycho-2 7116 out of 81224 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits:
Forced-photometry filter: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits -> calib.txt_param_ref_wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 58 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
2.2 pix Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
1.9 pix fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
1.9 pix fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
1.9 pix wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
2.2 pix wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
Limiting magnitude estimates:
15.6 mag. Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
15.6 mag. Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
12.6 mag. fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
12.6 mag. fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.buuUIeM0qz (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=6314, passed=84327
Got 84327 stars (including 77873 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 84327 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
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 83173 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 83174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 83174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits N_match=976 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.519 sigma_q2_arcsec=0.317 sigma_q3_arcsec=0.302 sigma_q4_arcsec=0.292 n_q1=212 n_q2=285 n_q3=252 n_q4=227 worst_quadrant_to_overall_ratio=1.486
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8BFfkA51IN (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-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.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-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.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-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=6417, passed=81182
Got 81182 stars (including 74651 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat
util/solve_plate_with_UCAC5 got 81182 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 79765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 79766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 79767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits N_match=971 sigma_overall_arcsec=0.525 sigma_q1_arcsec=0.415 sigma_q2_arcsec=0.651 sigma_q3_arcsec=0.464 sigma_q4_arcsec=0.624 n_q1=225 n_q2=275 n_q3=240 n_q4=231 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits -region wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DWaEOU1WmJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=206, passed=11917
Got 11917 stars (including 11693 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat
util/solve_plate_with_UCAC5 got 11917 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
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 11331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 11332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 11332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits N_match=967 sigma_overall_arcsec=0.372 sigma_q1_arcsec=0.393 sigma_q2_arcsec=0.384 sigma_q3_arcsec=0.297 sigma_q4_arcsec=0.374 n_q1=146 n_q2=353 n_q3=125 n_q4=343 worst_quadrant_to_overall_ratio=1.057
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.hNM10qffjh (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=246, passed=12767
Got 12767 stars (including 12490 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat
util/solve_plate_with_UCAC5 got 12767 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
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 12314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 12314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 12314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits N_match=969 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.368 sigma_q3_arcsec=0.319 sigma_q4_arcsec=0.376 n_q1=157 n_q2=329 n_q3=147 n_q4=336 worst_quadrant_to_overall_ratio=1.047
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-29-24_20.00sec_0.00C_LIGHTs_0042.fits
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Cnc-02-Q1b1x1_223044_TTUQ1b1x1_1065996_MFG7Y6C4/wcs_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043.fits
Preparing the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:13:32.62 +22:38:05.1: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:46:13.27 +21:34:21.1: 12.83 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:09:36.33 +23:00:13.9: 13.36 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:48.94 +17:54:15.0: 13.33 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:04:03.65 +23:09:33.6: 13.33 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:49:26.95 +17:08:55.9: 13.43 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:49:57.49 +17:09:18.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:46:55.46 +17:14:26.4: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:40.65 +17:23:34.8: 13.06 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:21.49 +17:31:06.6: 13.13 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:46:13.27 +21:34:21.1: 12.83 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter REJECTED candidate at 07:46:13.27 +21:34:21.1: ref_mag=12.83 +/- 0.01 new_mean_mag=12.4724 delta=0.36 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:13:32.62 +22:38:05.1: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:04:03.65 +23:09:33.6: 13.26 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:48.94 +17:54:15.0: 13.28 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:09:36.33 +23:00:13.9: 13.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 08:04:03.65 +23:09:33.6: ref_mag=13.29 +/- 0.02 new_mean_mag=12.2503 delta=1.04 (need > 0.90)
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 07:50:48.94 +17:54:15.0: ref_mag=13.31 +/- 0.02 new_mean_mag=12.2432 delta=1.06 (need > 0.90)
Forced photometry filter KEPT candidate at 08:09:36.33 +23:00:13.9: ref_mag=13.28 +/- 0.02 new_mean_mag=12.2528 delta=1.02 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:40.65 +17:23:34.8: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter REJECTED candidate at 07:47:40.65 +17:23:34.8: ref_mag=13.02 +/- 0.02 new_mean_mag=12.1338 delta=0.89 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:21.49 +17:31:06.6: 13.13 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:49:57.49 +17:09:18.8: 13.33 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:46:55.46 +17:14:26.4: 13.09 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:49:26.95 +17:08:55.9: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry reference-image weighted average: 13.42 +/- 0.03
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 07:47:21.49 +17:31:06.6: ref_mag=13.13 +/- 0.02 new_mean_mag=12.2174 delta=0.91 (need > 0.90)
Forced photometry reference-image weighted average: 13.39 +/- 0.03
Forced photometry filter KEPT candidate at 07:49:57.49 +17:09:18.8: ref_mag=13.42 +/- 0.03 new_mean_mag=12.3627 delta=1.05 (need > 0.90)
Forced photometry filter KEPT candidate at 07:46:55.46 +17:14:26.4: ref_mag=13.13 +/- 0.02 new_mean_mag=12.2029 delta=0.93 (need > 0.90)
Forced photometry filter KEPT candidate at 07:49:26.95 +17:08:55.9: ref_mag=13.39 +/- 0.03 new_mean_mag=12.2858 delta=1.10 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:58.30 +17:19:05.2: 13.22 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:56.60 +18:12:26.3: 12.88 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:58.30 +17:19:05.2: 13.22 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 07:47:58.30 +17:19:05.2: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2603 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:56.60 +18:12:26.3: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter REJECTED candidate at 07:47:56.60 +18:12:26.3: ref_mag=12.84 +/- 0.02 new_mean_mag=11.9745 delta=0.86 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:26.12 +17:30:23.5: 12.91 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:43.88 +17:27:20.4: 13.00 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:43.11 +17:10:13.3: 12.96 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:51:23.70 +17:22:29.7: 12.97 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:12:43.54 +24:04:44.7: 12.97 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:26.12 +17:30:23.5: 12.88 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry filter KEPT candidate at 07:47:26.12 +17:30:23.5: ref_mag=12.89 +/- 0.02 new_mean_mag=11.9118 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:43.88 +17:27:20.4: 12.88 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:43.11 +17:10:13.3: 12.93 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter KEPT candidate at 07:48:43.88 +17:27:20.4: ref_mag=12.94 +/- 0.02 new_mean_mag=12.0001 delta=0.94 (need > 0.90)
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 07:47:43.11 +17:10:13.3: ref_mag=12.95 +/- 0.02 new_mean_mag=11.9809 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:51:23.70 +17:22:29.7: 12.92 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.95 +/- 0.02
Forced photometry filter KEPT candidate at 07:51:23.70 +17:22:29.7: ref_mag=12.95 +/- 0.02 new_mean_mag=12.0418 delta=0.91 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:12:43.54 +24:04:44.7: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.92 +/- 0.01
Forced photometry filter KEPT candidate at 08:12:43.54 +24:04:44.7: ref_mag=12.92 +/- 0.01 new_mean_mag=12.0004 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:38.20 +17:15:25.9: 12.97 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:38.20 +17:15:25.9: 12.95 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.96 +/- 0.02
Forced photometry filter KEPT candidate at 07:48:38.20 +17:15:25.9: ref_mag=12.96 +/- 0.02 new_mean_mag=12.0258 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:11.33 +17:44:06.5: 12.93 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:11.33 +17:44:06.5: 12.86 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.02
Forced photometry filter REJECTED candidate at 07:48:11.33 +17:44:06.5: ref_mag=12.90 +/- 0.02 new_mean_mag=12.0416 delta=0.85 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:06:09.45 +23:30:27.9: 13.28 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:06:09.45 +23:30:27.9: 13.19 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter KEPT candidate at 08:06:09.45 +23:30:27.9: ref_mag=13.24 +/- 0.02 new_mean_mag=12.2507 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:27.73 +18:08:53.2: 13.26 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:04.53 +17:37:15.7: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:27.73 +18:08:53.2: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.26 +/- 0.02
Forced photometry filter KEPT candidate at 07:47:27.73 +18:08:53.2: ref_mag=13.26 +/- 0.02 new_mean_mag=12.2278 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:04.53 +17:37:15.7: 12.84 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:19.04 +17:29:53.0: 12.87 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 07:50:04.53 +17:37:15.7: ref_mag=12.87 +/- 0.02 new_mean_mag=11.9009 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:19.04 +17:29:53.0: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter REJECTED candidate at 07:47:19.04 +17:29:53.0: ref_mag=12.82 +/- 0.02 new_mean_mag=12.0296 delta=0.79 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:49:07.84 +17:18:10.1: 13.24 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:49:07.84 +17:18:10.1: 13.20 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 07:49:07.84 +17:18:10.1: ref_mag=13.22 +/- 0.02 new_mean_mag=12.1655 delta=1.06 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:14.24 +17:21:44.9: 12.86 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:14.24 +17:21:44.9: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry filter KEPT candidate at 07:50:14.24 +17:21:44.9: ref_mag=12.83 +/- 0.02 new_mean_mag=11.9015 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:53.91 +17:12:30.8: 13.22 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:53.91 +17:12:30.8: 13.22 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 07:48:53.91 +17:12:30.8: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2004 delta=1.02 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:00.18 +17:58:46.3: 13.21 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:00.18 +17:58:46.3: 13.17 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter KEPT candidate at 07:50:00.18 +17:58:46.3: ref_mag=13.19 +/- 0.02 new_mean_mag=12.2133 delta=0.98 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:31.98 +17:51:50.8: 13.52 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:31.98 +17:51:50.8: 13.35 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter KEPT candidate at 07:48:31.98 +17:51:50.8: ref_mag=13.43 +/- 0.03 new_mean_mag=12.4302 delta=1.00 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:39.78 +17:25:58.6: 12.51 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:39.78 +17:25:58.6: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 07:48:39.78 +17:25:58.6: ref_mag=12.49 +/- 0.01 new_mean_mag=11.6163 delta=0.88 (need > 0.90)
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:32.43 +17:26:35.5: 12.51 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:32.43 +17:26:35.5: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 07:48:32.43 +17:26:35.5: ref_mag=12.49 +/- 0.01 new_mean_mag=11.6251 delta=0.86 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:29.69 +17:20:15.2: 13.19 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:29.69 +17:20:15.2: 13.07 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter REJECTED candidate at 07:48:29.69 +17:20:15.2: ref_mag=13.13 +/- 0.02 new_mean_mag=12.2803 delta=0.85 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:35.44 +17:51:41.2: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:35.44 +17:51:41.2: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter KEPT candidate at 07:48:35.44 +17:51:41.2: ref_mag=12.81 +/- 0.02 new_mean_mag=11.8957 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:27.66 +18:10:40.3: 13.18 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:27.66 +18:10:40.3: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter REJECTED candidate at 07:48:27.66 +18:10:40.3: ref_mag=13.10 +/- 0.02 new_mean_mag=12.2088 delta=0.89 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:22.14 +17:25:04.9: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:42.68 +17:13:32.9: 13.17 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:22.14 +17:25:04.9: 13.09 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 07:48:22.14 +17:25:04.9: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1383 delta=0.99 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:42.68 +17:13:32.9: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 07:50:42.68 +17:13:32.9: ref_mag=13.10 +/- 0.02 new_mean_mag=12.1491 delta=0.95 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:39.62 +17:29:12.8: 13.46 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:51:12.49 +17:18:04.2: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:39.62 +17:29:12.8: 13.48 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry filter KEPT candidate at 07:47:39.62 +17:29:12.8: ref_mag=13.47 +/- 0.03 new_mean_mag=12.3936 delta=1.08 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:51:12.49 +17:18:04.2: 12.78 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter KEPT candidate at 07:51:12.49 +17:18:04.2: ref_mag=12.80 +/- 0.01 new_mean_mag=11.7779 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:14.96 +17:13:52.1: 13.12 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:51.62 +17:15:12.0: 13.12 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:14.96 +17:13:52.1: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 07:50:14.96 +17:13:52.1: ref_mag=13.14 +/- 0.02 new_mean_mag=12.1090 delta=1.03 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:51.62 +17:15:12.0: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.14 +/- 0.02
Forced photometry filter KEPT candidate at 07:47:51.62 +17:15:12.0: ref_mag=13.14 +/- 0.02 new_mean_mag=12.2073 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:28.93 +17:37:15.6: 13.41 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:51:08.49 +17:14:32.1: 13.40 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:28.93 +17:37:15.6: 13.40 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter KEPT candidate at 07:48:28.93 +17:37:15.6: ref_mag=13.41 +/- 0.03 new_mean_mag=12.2568 delta=1.15 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:51:08.49 +17:14:32.1: 13.33 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.02
Forced photometry filter KEPT candidate at 07:51:08.49 +17:14:32.1: ref_mag=13.36 +/- 0.02 new_mean_mag=12.2559 delta=1.11 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:46:56.67 +17:52:26.4: 13.40 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:46:56.67 +17:52:26.4: 13.29 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.03
Forced photometry filter KEPT candidate at 07:46:56.67 +17:52:26.4: ref_mag=13.35 +/- 0.03 new_mean_mag=12.2791 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:22.51 +17:46:05.7: 13.09 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:09.36 +17:22:29.6: 13.08 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:22.51 +17:46:05.7: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 07:48:22.51 +17:46:05.7: ref_mag=13.07 +/- 0.02 new_mean_mag=12.0694 delta=1.00 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:09.36 +17:22:29.6: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 07:48:09.36 +17:22:29.6: ref_mag=13.06 +/- 0.02 new_mean_mag=11.9989 delta=1.07 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:29.09 +17:12:22.9: 13.56 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:29.09 +17:12:22.9: 13.37 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter KEPT candidate at 07:48:29.09 +17:12:22.9: ref_mag=13.45 +/- 0.03 new_mean_mag=12.3679 delta=1.09 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:58.95 +17:19:20.4: 13.06 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:05.82 +17:16:14.9: 13.05 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:49:09.38 +17:23:53.1: 12.70 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:58.95 +17:19:20.4: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 07:48:58.95 +17:19:20.4: ref_mag=13.03 +/- 0.02 new_mean_mag=12.0698 delta=0.96 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:05.82 +17:16:14.9: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter KEPT candidate at 07:48:05.82 +17:16:14.9: ref_mag=13.02 +/- 0.02 new_mean_mag=12.0809 delta=0.94 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:49:09.38 +17:23:53.1: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter KEPT candidate at 07:49:09.38 +17:23:53.1: ref_mag=12.66 +/- 0.01 new_mean_mag=11.7358 delta=0.93 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:48:14.69 +17:17:56.3: 13.36 +/- 0.04 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:48:14.69 +17:17:56.3: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry filter KEPT candidate at 07:48:14.69 +17:17:56.3: ref_mag=13.32 +/- 0.03 new_mean_mag=12.3523 delta=0.97 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:47:48.92 +17:17:45.5: 12.66 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:08:29.40 +23:03:29.1: 13.01 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:50:17.91 +17:19:39.7: 13.32 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:47:48.92 +17:17:45.5: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.68 +/- 0.01
Forced photometry filter REJECTED candidate at 07:47:48.92 +17:17:45.5: ref_mag=12.68 +/- 0.01 new_mean_mag=11.7817 delta=0.90 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 08:08:29.40 +23:03:29.1: 12.93 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.97 +/- 0.01
Forced photometry filter KEPT candidate at 08:08:29.40 +23:03:29.1: ref_mag=12.97 +/- 0.01 new_mean_mag=12.0523 delta=0.92 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_23-40-53_20.00sec_-15.00C_LIGHT_0177.fits at 07:50:17.91 +17:19:39.7: 13.23 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter KEPT candidate at 07:50:17.91 +17:19:39.7: ref_mag=13.28 +/- 0.02 new_mean_mag=12.2639 delta=1.01 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out06392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out06465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out06953.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out06970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out07387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out07479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out07508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out07575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out07589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out07725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out07828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out07996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out08399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out08408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out08767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out08976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out09584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out09706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out10457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out11578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out12407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out12654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out14877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out06774.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out06881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82770.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 32s
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 108504_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 108504_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 108587_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 108587_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:46:15.06 +18:30:22.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 108600_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 108600_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:10:23.12 +25:29:16.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 108629_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 108629_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 108678_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 108678_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:53:37.14 +26:45:21.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 108687_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 108687_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:13:43.92 +23:09:18.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 108698_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 108698_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:01:27.18 +23:56:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70571_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 70571_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 12419_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 12419_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 59797_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 59797_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 08584_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 08584_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 09706_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 09706_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:47:21.49 +17:31:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.731 668135214328885632 116.83969259397 +17.51835682896 12.9355 12.4626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 06465_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 06465_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:49:26.95 +17:08:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.937 667911158771910272 117.36242985093 +17.14863679588 13.2050 12.6691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07508_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 07508_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:46:55.46 +17:14:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.166 668089348375046144 116.73112080547 +17.24063766758 12.8827 12.3742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 06392_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 06392_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:49:57.49 +17:09:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.413 667909165907062272 117.48960999411 +17.15512787809 13.2276 12.7098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07996_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 07996_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:47:58.30 +17:19:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.861 668093712061768192 116.99314817689 +17.31801981793 12.9522 12.3294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 15189_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 15189_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 09584_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 09584_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:47:26.12 +17:30:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 1.614 668134943747797120 116.85928866529 +17.50641637273 12.7434 12.3308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07995_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 07995_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 78829_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 78829_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 08976_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 08976_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:43.88 +17:27:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 1.015 668120031621313280 117.18256338897 +17.45578128009 12.6274 11.9360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 06774_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 06774_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:47:43.11 +17:10:13.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)
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Considering the candidate 07387_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 07387_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:38.20 +17:15:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 1.010 667927445287786368 117.15888872285 +17.25710384238 12.7630 12.2075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 11285_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 11285_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 03951_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 03951_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 08:21:42.81 +17:17:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82770_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 82770_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 10164_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 10164_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 14877_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 14877_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:47:27.73 +18:08:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.328 668592581103410432 116.86552000692 +18.14774287547 13.1513 12.7396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 09536_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 09536_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 07725_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 07725_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:49:07.84 +17:18:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.110 667929296417091968 117.28264273323 +17.30278513563 12.9961 12.3827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 08012_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 08012_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 06953_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 06953_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:53.91 +17:12:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.506 667923871875116800 117.22449583387 +17.20848839832 13.0827 12.8016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 13144_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 13144_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 12407_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 12407_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:31.98 +17:51:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.056 668525442174785152 117.13348736699 +17.86392423302 13.3402 12.8586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 08749_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 08749_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 08859_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 08859_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 08010_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 08010_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 12310_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 12310_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 14943_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 14943_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
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Considering the candidate 08767_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 08767_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:22.14 +17:25:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.739 668119619304465408 117.09243770771 +17.41812796691 12.9343 12.4790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 06881_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 06881_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 09437_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 09437_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 07298_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 07298_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 06920_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 06920_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 07479_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 07479_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:47:51.62 +17:15:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.779 668092337672249344 116.96530282842 +17.25338697269 12.9356 12.4534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 06964_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 06964_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 10457_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 10457_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:28.93 +17:37:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.797 668131232896005760 117.12077110843 +17.62103441348 13.2483 12.8222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 12654_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 12654_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:46:56.67 +17:52:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.547 668195107649455616 116.73616956377 +17.87385422462 13.1709 12.5133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 11578_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 11578_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:22.51 +17:46:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.738 668149168679417600 117.09400010525 +17.76830105486 12.9272 12.5012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 08399_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 08399_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:09.36 +17:22:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.398 668117592079916800 117.03904339099 +17.37499140941 12.9043 12.3633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 06970_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 06970_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:29.09 +17:12:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.685 667903737068316544 117.12111563984 +17.20652939708 13.1753 12.4779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07589_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 07589_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:58.95 +17:19:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.582 667929536935259776 117.24576801150 +17.32224665761 12.7932 12.1336 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07575_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 07575_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:05.82 +17:16:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.337 668092715629358208 117.02433979978 +17.27084339044 12.8806 12.4498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 08408_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 08408_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:49:09.38 +17:23:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 0.635 667936821199790336 117.28893046304 +17.39798394768 12.5331 12.0859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07828_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 07828_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
**** FOUND 07:48:14.69 +17:17:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.506 668116148970914688 117.06126886693 +17.29910031180 13.1281 12.6337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 59100_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
Preparing report for the candidate 59100_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
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Considering the candidate 07746_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043
The candidate 07746_fd_Cnc-02-Q1b1x1_2026-05-25_22-30-07_20.00sec_-0.00C_LIGHTs_0043 did not pass the final checks
