This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM
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 09 10.4680 2461293.9680 13.47 05:01:49.10 +46:53:59.6
160.33731 3.04067 galactic Aur Second-epoch detections are separated by 0.5" and 9.0 pix
The object was found in VSX 0" Gaia DR3 206998186513489024
Type: ROT
# Max. Min./Amp. JD0 Period
13.870 G 13.920 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:49.10 +46:53:59.6: 14.35 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:49.10 +46:53:59.6: 14.41 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.05
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 206998186513489024,2461293.9680,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 206998186513489024 20260910.4680 13.47CV 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 09 10.4680 2461293.9680 13.48 04:55:41.02 +46:55:26.5
159.66912 2.23279 galactic Aur Second-epoch detections are separated by 1.6" and 9.1 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 | 04:55:41.02 +46:55:26.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.559+/-0.033 (K)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:41.02 +46:55:26.5: 14.42 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:41.02 +46:55:26.5: 14.46 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.05
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,2461293.9680,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4680 13.48CV 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 09 10.4680 2461293.9680 13.59 04:53:44.82 +44:37:40.3
161.24198 0.52572 galactic Aur Second-epoch detections are separated by 1.4" and 9.3 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 | 04:53:44.82 +44:37:40.3 (user input) | T | P | (position from user input) J-Ks=0.550+/-0.030 (K)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:53:44.82 +44:37:40.3: 14.69 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:53:44.82 +44:37:40.3: 14.48 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461293.9680,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4680 13.59CV 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 09 10.4680 2461293.9680 13.60 04:55:57.90 +46:52:12.6
159.74127 2.23654 galactic Aur Second-epoch detections are separated by 1.3" and 9.0 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 | 04:55:57.90 +46:52:12.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.886+/-0.034 (M)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:57.90 +46:52:12.6: 14.62 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:57.90 +46:52:12.6: 14.52 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461293.9680,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4680 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4680 2461293.9680 13.57 04:55:50.48 +46:51:49.7
159.73299 2.21608 galactic Aur Second-epoch detections are separated by 0.4" and 9.0 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 | 04:55:50.48 +46:51:49.7 (user input) | T | P | (position from user input) J-Ks=0.400+/-0.038 (G)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:50.48 +46:51:49.7: 14.64 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:50.48 +46:51:49.7: 14.49 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461293.9680,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4680 13.57CV 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 09 10.4680 2461293.9680 13.41 04:55:47.62 +47:00:52.9
159.61015 2.30421 galactic Aur Second-epoch detections are separated by 1.7" and 9.1 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 | 04:55:47.62 +47:00:52.9 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.264+/-0.033 (Very red! L if it's a dwarf)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:47.62 +47:00:52.9: 14.48 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:47.62 +47:00:52.9: 14.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.05
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,2461293.9680,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4680 13.41CV 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 09 10.4680 2461293.9680 13.41 05:02:18.01 +47:05:10.0
160.23992 3.21948 galactic Aur Second-epoch detections are separated by 0.4" and 9.0 pix
The object was found in VSX 1" Gaia DR3 207017595469546496
Type: ROT
# Max. Min./Amp. JD0 Period
13.760 G 13.800 G K
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:18.01 +47:05:10.0: 14.43 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:18.01 +47:05:10.0: 14.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.05
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 207017595469546496,2461293.9680,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207017595469546496 20260910.4680 13.41CV 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 09 10.4680 2461293.9680 13.44 05:01:58.27 +47:05:38.1
160.19948 3.17990 galactic Aur Second-epoch detections are separated by 0.5" and 8.9 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 | 05:01:58.27 +47:05:38.1 (user input) | T | P | (position from user input) J-Ks=0.481+/-0.050 (K)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:58.27 +47:05:38.1: 14.34 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:58.27 +47:05:38.1: 14.40 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.05
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,2461293.9680,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4680 13.44CV 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 09 10.4680 2461293.9680 13.35 04:45:15.80 +43:10:19.3
161.37807 -1.58042 galactic Per Second-epoch detections are separated by 1.0" and 9.4 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 | target | 04:45:15.80 +43:10:19.3 (user input) | T | P | (position from user input) J-Ks=0.334+/-0.034 (G)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:45:15.80 +43:10:19.3: 14.29 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:45:15.80 +43:10:19.3: 14.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 10.4680* 04 45 15.80 +43 10 19.3 13.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461293.9680,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4680 13.35CV 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 09 10.4680 2461293.9680 13.29 04:55:55.62 +46:52:25.7
159.73436 2.23375 galactic Aur Second-epoch detections are separated by 1.0" and 9.1 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 | 04:55:55.62 +46:52:25.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.932+/-0.034 (M)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:55.62 +46:52:25.7: 14.29 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:55.62 +46:52:25.7: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.04
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,2461293.9680,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4680 13.29CV 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 09 10.4680 2461293.9680 13.30 04:55:49.33 +46:55:50.7
159.67870 2.25544 galactic Aur Second-epoch detections are separated by 0.2" and 9.0 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 | 04:55:49.33 +46:55:50.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=1.036+/-0.032 (M)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:49.33 +46:55:50.7: 14.23 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:49.33 +46:55:50.7: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.04
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,2461293.9680,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4680 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4680 2461293.9680 13.31 04:56:02.66 +47:02:28.1
159.61626 2.35407 galactic Aur Second-epoch detections are separated by 0.5" and 9.1 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 | 04:56:02.66 +47:02:28.1 (user input) | T | P | (position from user input) J-Ks=0.959+/-0.034 (M)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:02.66 +47:02:28.1: 14.25 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:02.66 +47:02:28.1: 14.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.04
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,2461293.9680,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260910.4680 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 10.4680 2461293.9680 13.29 05:03:56.83 +46:49:54.6
160.61329 3.28786 galactic Aur Second-epoch detections are separated by 1.8" and 8.6 pix
The object was found in VSX 1" Gaia DR3 207042815517191680
Type: ROT
# Max. Min./Amp. JD0 Period
13.840 G 13.860 G G
The object was not found in astcheck.
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:56.83 +46:49:54.6: 14.17 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:56.83 +46:49:54.6: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.04
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 207042815517191680,2461293.9680,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207042815517191680 20260910.4680 13.29CV 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 09 10.4680 2461293.9680 13.23 05:02:02.63 +46:42:23.7
160.51412 2.95304 galactic Aur Second-epoch detections are separated by 0.4" and 8.9 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 J075.4966+46.7009 | 05:02:02.63 +46:42:23.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.981+/-0.031 (M)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:02.63 +46:42:23.7: 14.15 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:02.63 +46:42:23.7: 14.25 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.05
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 J075.4966+46.7009,2461293.9680,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J075.4966+46.7009 20260910.4680 13.23CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
First image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Last image: 2461293.96828023 10.09.2026 11:14:09.412 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.71
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 18788
Objects passed selection criteria: 18702
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 12396
Average stars matched: 11612.2 (93.6774 %)
Memory usage VmPeak: 244252 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Sep 10 02:28:55 CDT 2026
VaST build number 1.0rc89-204-g1bee8b93
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 10 06:16:43 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
First image: 2461093.60953049 22.02.2026 02:37:33.434 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Last image: 2461293.96828023 10.09.2026 11:14:09.412 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 129
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 59 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 160810
Objects passed selection criteria: 160359
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 112606
Average stars matched: 104715 (92.9917 %)
Memory usage VmPeak: 623796 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Sep 10 02:28:55 CDT 2026
VaST build number 1.0rc89-204-g1bee8b93
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Sep 10 06:18:25 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.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/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.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: 2461293.96770466
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits exists and is non-empty
wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (1st reference image)
verification OK: wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:00.727 +45:59:45.06 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_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits (1st new image)
verification OK: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:48:02.316 +46:01:01.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:48:02.316 +46:01:01.93
Angular distance between the image centers 0.0218 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits (2nd new image)
verification OK: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:48:00.240 +46:01:51.97 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:48:00.240 +46:01:51.97
Angular distance between the image centers 0.0353 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 04:48:02.316 +46:01:01.93
Second-epoch second image center 04:48:00.240 +46:01:51.97
Angular distance between the image centers 0.01514 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.HxrxpVYxwu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.SjD9rbys0o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits &> /tmp/tmp.0zLTtGNECF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits &> /tmp/tmp.mSgFLGOeD0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.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_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Found non-empty wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
The reference image (wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits) and catalog (wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat) found
'wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat' -> 'wcsmag.cat'
Read 23847 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9496 to 84.6399 deg, Dec +39.9317 to +51.3292 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 59.9496 to 84.6399 deg, Dec 39.9317 to 51.3292 deg
Loaded 12139 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): 8124 out of 9276 total matches.
Matched with Tycho-2 9276 out of 23847 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.944300
a=0.000000 b=1.000000 c=22.944300
From vast_summary.log: estimated ref. image limiting mag.: -7.71
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23847 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9496 to 84.6399 deg, Dec +39.9317 to +51.3292 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 59.9496 to 84.6399 deg, Dec 39.9317 to 51.3292 deg
Loaded 12139 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): 8124 out of 9276 total matches.
Matched with Tycho-2 9276 out of 23847 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Forced-photometry filter: calibrated wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -> calib.txt_param_ref_wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (aperture=6.0)
Read 23965 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9494 to 84.6297 deg, Dec +39.9321 to +51.3293 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 59.9494 to 84.6297 deg, Dec 39.9321 to 51.3293 deg
Loaded 12131 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): 8135 out of 9280 total matches.
Matched with Tycho-2 9280 out of 23965 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Forced-photometry filter: calibrated wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -> calib.txt_param_ref_wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (aperture=6.0)
____ 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: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
2.1 pix Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
2.2 pix fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
2.2 pix fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
Limiting magnitude estimates:
15.2 mag. Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
15.2 mag. Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
13.6 mag. fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
13.6 mag. fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.HxrxpVYxwu (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/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2564, bad_region=4955, passed=23847
Got 23847 stars (including 16757 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
util/solve_plate_with_UCAC5 got 23847 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 4869 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 19949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 19949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 19949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4869 stars left (next iteration limit 5355)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits N_match=4869 sigma_overall_arcsec=0.469 sigma_q1_arcsec=0.592 sigma_q2_arcsec=0.449 sigma_q3_arcsec=0.450 sigma_q4_arcsec=0.363 n_q1=1401 n_q2=589 n_q3=2033 n_q4=846 worst_quadrant_to_overall_ratio=1.262
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.SjD9rbys0o (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/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2577, bad_region=4981, passed=23965
Got 23965 stars (including 16814 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
util/solve_plate_with_UCAC5 got 23965 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 4866 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 20053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 20053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 20053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4866 stars left (next iteration limit 5352)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits N_match=4866 sigma_overall_arcsec=0.478 sigma_q1_arcsec=0.605 sigma_q2_arcsec=0.469 sigma_q3_arcsec=0.441 sigma_q4_arcsec=0.363 n_q1=1397 n_q2=593 n_q3=2039 n_q4=837 worst_quadrant_to_overall_ratio=1.265
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.0zLTtGNECF (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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=358, bad_region=1627, passed=7809
Got 7809 stars (including 5872 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 7809 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.4 to 51.3)
Done reading UCAC5 zone files...
Matched 4916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 4849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 6647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.4 to 51.3)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 6647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 6647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 4848 stars left (next iteration limit 5332)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4848 robust_rms=7.606 arcsec worst_quadrant_rms=8.474 arcsec
SIP_REFIT: SIP order 3 trial: matched=4848 robust_rms=0.505 arcsec worst_quadrant_rms=0.584 arcsec
SIP_REFIT: SIP order 5 trial: matched=4848 robust_rms=0.454 arcsec worst_quadrant_rms=0.479 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4848 robust_rms_before=0.851 arcsec robust_rms_before_corrected=0.507 arcsec robust_rms_after=0.454 arcsec worst_quadrant_rms_before=0.541 worst_quadrant_rms_after=0.479
verification OK: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
verification OK: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:48:02.308 +46:01:01.21 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 7809 stars ###
'wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/correct_sextractor_wcs_catalog_usingxy2sky3010821.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.851 -> 0.454 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4848 pairs from the initial matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.4 to 51.3)
Done reading UCAC5 zone files...
Matched 4671 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4671 pairs (4848 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4671 robust_rms=7.453 arcsec worst_quadrant_rms=8.327 arcsec
SIP_REFIT: SIP order 3 trial: matched=4671 robust_rms=0.498 arcsec worst_quadrant_rms=0.582 arcsec
SIP_REFIT: SIP order 5 trial: matched=4671 robust_rms=0.449 arcsec worst_quadrant_rms=0.479 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4671 robust_rms_before=0.449 arcsec robust_rms_before_corrected=0.449 arcsec robust_rms_after=0.449 arcsec worst_quadrant_rms_before=0.479 worst_quadrant_rms_after=0.479
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-quadrant 0.479 vs 0.479 arcsec) - keeping the current solution
SIP_REFIT: the second refit on the re-matched pairs was not applied - keeping the first refit solution
Accuracy estimation diagnostic: 4671 matched stars entering correct_measured_positions(), 6647 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4671 matched stars entering correct_measured_positions(), 6645 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
WCS_QUALITY_DIAG: file=fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits N_match=4671 sigma_overall_arcsec=0.514 sigma_q1_arcsec=0.453 sigma_q2_arcsec=0.494 sigma_q3_arcsec=0.538 sigma_q4_arcsec=0.507 n_q1=1362 n_q2=1171 n_q3=1080 n_q4=1058 worst_quadrant_to_overall_ratio=1.046
The image catalog is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits -region wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.mSgFLGOeD0 (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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=323, bad_region=1319, passed=7154
Got 7154 stars (including 5541 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 7154 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.4 to 51.2)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 4838 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 6254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.4 to 51.2)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 6254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 4840 matched stars entering correct_measured_positions(), 6254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 4840 stars left (next iteration limit 5320)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4840 robust_rms=7.351 arcsec worst_quadrant_rms=9.448 arcsec
SIP_REFIT: SIP order 3 trial: matched=4840 robust_rms=0.535 arcsec worst_quadrant_rms=0.642 arcsec
SIP_REFIT: SIP order 5 trial: matched=4840 robust_rms=0.478 arcsec worst_quadrant_rms=0.547 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4840 robust_rms_before=0.826 arcsec robust_rms_before_corrected=0.521 arcsec robust_rms_after=0.478 arcsec worst_quadrant_rms_before=0.546 worst_quadrant_rms_after=0.547
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.546 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits N_match=4840 sigma_overall_arcsec=0.558 sigma_q1_arcsec=0.464 sigma_q2_arcsec=0.572 sigma_q3_arcsec=0.564 sigma_q4_arcsec=0.576 n_q1=1494 n_q2=1496 n_q3=961 n_q4=889 worst_quadrant_to_overall_ratio=1.032
The image catalog is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits -region wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits'
Saving the final (post-refit) wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits to local_wcs_cache/
'wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits' -> 'local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits'
Saving the final (post-refit) wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits to local_wcs_cache/
'wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits'
Saving the final (post-refit) wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits to local_wcs_cache/
'wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits sigma_overall=0.469 worst_q_ratio=1.262
ref2=Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits sigma_overall=0.478 worst_q_ratio=1.265
new1=fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits sigma_overall=0.514 worst_q_ratio=1.046
new2=fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits sigma_overall=0.558 worst_q_ratio=1.032
reference average sigma_overall=0.4735 worst_q_ratio=1.2635
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044_astrometric_residuals.png (4869 matched stars from wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045_astrometric_residuals.png (4866 matched stars from wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138_astrometric_residuals.png (4671 matched stars from wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139_astrometric_residuals.png (4840 matched stars from wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits'
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits'
Preparing the HTML report for the field Per-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Per-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Creating symlink local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
Creating symlink local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
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_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits exists and is non-empty
wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (1st reference image)
verification OK: wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:48:00.727 +45:59:45.06 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_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits (1st new image)
verification OK: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:48:02.308 +46:01:01.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:48:02.308 +46:01:01.21
Angular distance between the image centers 0.0216 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits (2nd new image)
verification OK: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:48:00.240 +46:01:51.97 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:48:00.727 +45:59:45.06
Second-epoch image center 04:48:00.240 +46:01:51.97
Angular distance between the image centers 0.0353 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 04:48:02.308 +46:01:01.21
Second-epoch second image center 04:48:00.240 +46:01:51.97
Angular distance between the image centers 0.01532 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.esy3ZMY7Dv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.oSFhYgHmLM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits &> /tmp/tmp.bkSZNEJQuL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits &> /tmp/tmp.SzsUfOXSd6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.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_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Found non-empty wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits and wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
The reference image (wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits) and catalog (wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat) found
'wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat' -> 'wcsmag.cat'
Read 195814 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9096 to 84.6822 deg, Dec +39.9252 to +51.3404 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 59.9096 to 84.6822 deg, Dec 39.9252 to 51.3404 deg
Loaded 12199 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): 6231 out of 9378 total matches.
Matched with Tycho-2 9378 out of 195814 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.794000
a=0.000000 b=1.000000 c=22.794000
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 195814 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9096 to 84.6822 deg, Dec +39.9252 to +51.3404 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 59.9096 to 84.6822 deg, Dec 39.9252 to 51.3404 deg
Loaded 12199 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): 6231 out of 9378 total matches.
Matched with Tycho-2 9378 out of 195814 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Forced-photometry filter: calibrated wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -> calib.txt_param_ref_wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (aperture=4.4)
Read 196080 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9097 to 84.6518 deg, Dec +39.9253 to +51.3374 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 59.9097 to 84.6518 deg, Dec 39.9253 to 51.3374 deg
Loaded 12186 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): 6203 out of 9379 total matches.
Matched with Tycho-2 9379 out of 196080 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Forced-photometry filter: calibrated wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -> calib.txt_param_ref_wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 109 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
1.9 pix Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
2.0 pix fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
2.0 pix fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
Limiting magnitude estimates:
15.5 mag. Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
15.5 mag. Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
14.0 mag. fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
14.0 mag. fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.esy3ZMY7Dv (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/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=26966, bad_region=31099, passed=195776
Got 195776 stars (including 140771 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat
util/solve_plate_with_UCAC5 got 195776 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 4870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 171776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 171776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 171776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4870 stars left (next iteration limit 5357)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits N_match=4870 sigma_overall_arcsec=0.451 sigma_q1_arcsec=0.539 sigma_q2_arcsec=0.427 sigma_q3_arcsec=0.420 sigma_q4_arcsec=0.341 n_q1=1409 n_q2=639 n_q3=1931 n_q4=891 worst_quadrant_to_overall_ratio=1.196
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.oSFhYgHmLM (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/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=50, blended=27081, bad_region=31072, passed=196030
Got 196030 stars (including 140952 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat
util/solve_plate_with_UCAC5 got 196030 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 4865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 172118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 172118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 172118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 4865 stars left (next iteration limit 5351)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits N_match=4865 sigma_overall_arcsec=0.448 sigma_q1_arcsec=0.569 sigma_q2_arcsec=0.430 sigma_q3_arcsec=0.415 sigma_q4_arcsec=0.337 n_q1=1402 n_q2=638 n_q3=1931 n_q4=894 worst_quadrant_to_overall_ratio=1.270
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.bkSZNEJQuL (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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=4285, bad_region=10544, passed=73845
Got 73845 stars (including 59631 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 73845 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 66871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 66871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 66871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4864 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4864 robust_rms=7.429 arcsec worst_quadrant_rms=8.138 arcsec
SIP_REFIT: SIP order 3 trial: matched=4864 robust_rms=0.507 arcsec worst_quadrant_rms=0.593 arcsec
SIP_REFIT: SIP order 5 trial: matched=4864 robust_rms=0.454 arcsec worst_quadrant_rms=0.480 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4864 robust_rms_before=0.454 arcsec robust_rms_before_corrected=0.509 arcsec robust_rms_after=0.454 arcsec worst_quadrant_rms_before=0.484 worst_quadrant_rms_after=0.480
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.484 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits N_match=4864 sigma_overall_arcsec=0.542 sigma_q1_arcsec=0.489 sigma_q2_arcsec=0.564 sigma_q3_arcsec=0.548 sigma_q4_arcsec=0.540 n_q1=1462 n_q2=1191 n_q3=1135 n_q4=1076 worst_quadrant_to_overall_ratio=1.041
The image catalog is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits -region wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.SzsUfOXSd6 (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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=4034, bad_region=8728, passed=68428
Got 68428 stars (including 56068 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 68428 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4858 matched stars entering correct_measured_positions(), 4858 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4858 matched stars entering correct_measured_positions(), 62877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 4910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4858 matched stars entering correct_measured_positions(), 62877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 4858 matched stars entering correct_measured_positions(), 62877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4858 stars left (next iteration limit 5343)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4858 robust_rms=7.359 arcsec worst_quadrant_rms=9.205 arcsec
SIP_REFIT: SIP order 3 trial: matched=4858 robust_rms=0.536 arcsec worst_quadrant_rms=0.646 arcsec
SIP_REFIT: SIP order 5 trial: matched=4858 robust_rms=0.478 arcsec worst_quadrant_rms=0.535 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4858 robust_rms_before=0.829 arcsec robust_rms_before_corrected=0.514 arcsec robust_rms_after=0.478 arcsec worst_quadrant_rms_before=0.549 worst_quadrant_rms_after=0.535
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.549 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits N_match=4858 sigma_overall_arcsec=0.551 sigma_q1_arcsec=0.464 sigma_q2_arcsec=0.558 sigma_q3_arcsec=0.575 sigma_q4_arcsec=0.532 n_q1=1545 n_q2=1430 n_q3=985 n_q4=898 worst_quadrant_to_overall_ratio=1.042
The image catalog is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits -region wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/wcs_fd_Per-03-Q2b1x1_2026-09-10_06-13-19_20.00sec_-0.00C_LIGHT_0138.fits
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.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_2026-09-10_CI_Per-03-Q2b1x1_061447_TTUQ2b1x1_3000857_rvUalCdM/wcs_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139.fits
Preparing the HTML report for the field Per-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:59:10.47 +44:29:45.0: 14.02 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:23:14.69 +42:16:28.3: 13.63 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:13.60 +46:24:31.4: 14.11 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:52:01.12 +47:00:22.3: 13.74 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:52:42.23 +42:56:24.0: 14.12 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:13:49.61 +50:07:19.6: 12.74 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:22:48.17 +43:57:18.5: 13.20 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:06.64 +44:21:53.1: 13.37 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:59:10.47 +44:29:45.0: 14.02 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:13.60 +46:24:31.4: 14.13 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:52:42.23 +42:56:24.0: 14.09 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:23:14.69 +42:16:28.3: 13.50 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:52:01.12 +47:00:22.3: 13.70 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.12 +/- 0.04
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry reference-image weighted average: 14.02 +/- 0.05
Forced photometry filter REJECTED candidate at 04:23:14.69 +42:16:28.3: ref_mag=13.56 +/- 0.03 new_mean_mag=13.0854 delta=0.47 (need > 0.90)
Forced photometry reference-image weighted average: 13.72 +/- 0.03
Forced photometry filter REJECTED candidate at 04:59:10.47 +44:29:45.0: ref_mag=14.02 +/- 0.05 new_mean_mag=13.7013 delta=0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:52:01.12 +47:00:22.3: ref_mag=13.72 +/- 0.03 new_mean_mag=13.5280 delta=0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:56:13.60 +46:24:31.4: ref_mag=14.12 +/- 0.04 new_mean_mag=13.4366 delta=0.68 (need > 0.90)
Forced photometry reference-image weighted average: 14.10 +/- 0.04
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:00:58.05 +44:45:01.3: 13.28 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:22:48.17 +43:57:18.5: 13.15 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:13:49.61 +50:07:19.6: 12.72 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:06.64 +44:21:53.1: 13.39 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 04:52:42.23 +42:56:24.0: ref_mag=14.10 +/- 0.04 new_mean_mag=13.5910 delta=0.51 (need > 0.90)
Forced photometry reference-image weighted average: 13.38 +/- 0.02
Forced photometry reference-image weighted average: 13.17 +/- 0.02
Forced photometry filter REJECTED candidate at 05:01:06.64 +44:21:53.1: ref_mag=13.38 +/- 0.02 new_mean_mag=13.1379 delta=0.24 (need > 0.90)
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter REJECTED candidate at 04:22:48.17 +43:57:18.5: ref_mag=13.17 +/- 0.02 new_mean_mag=12.9068 delta=0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:13:49.61 +50:07:19.6: ref_mag=12.73 +/- 0.01 new_mean_mag=13.2268 delta=-0.50 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:00:58.05 +44:45:01.3: 13.28 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.02
Forced photometry filter REJECTED candidate at 05:00:58.05 +44:45:01.3: ref_mag=13.28 +/- 0.02 new_mean_mag=12.8776 delta=0.40 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:51:00.71 +48:34:10.5: 12.72 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:51:00.71 +48:34:10.5: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter REJECTED candidate at 04:51:00.71 +48:34:10.5: ref_mag=12.70 +/- 0.01 new_mean_mag=13.0211 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:12:59.65 +44:33:29.7: 12.61 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:04:34.06 +45:59:52.5: 12.98 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:00.68 +42:25:34.2: 12.19 +/- 0.01 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:22.63 +45:52:14.8: 12.52 +/- 0.02 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:12:59.65 +44:33:29.7: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:04:34.06 +45:59:52.5: 12.96 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 05:12:59.65 +44:33:29.7: ref_mag=12.61 +/- 0.01 new_mean_mag=12.8080 delta=-0.20 (need > 0.90)
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter REJECTED candidate at 05:04:34.06 +45:59:52.5: ref_mag=12.97 +/- 0.02 new_mean_mag=12.9746 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:00.68 +42:25:34.2: 12.18 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter REJECTED candidate at 05:03:00.68 +42:25:34.2: ref_mag=12.18 +/- 0.01 new_mean_mag=12.4807 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:54:49.52 +45:43:19.0: 13.20 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:22.63 +45:52:14.8: 12.51 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry filter REJECTED candidate at 05:01:22.63 +45:52:14.8: ref_mag=12.52 +/- 0.01 new_mean_mag=12.4201 delta=0.10 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:54:49.52 +45:43:19.0: 13.18 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter REJECTED candidate at 04:54:49.52 +45:43:19.0: ref_mag=13.19 +/- 0.02 new_mean_mag=12.9439 delta=0.25 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:08:40.72 +42:33:53.2: 12.94 +/- 0.03 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:06:38.90 +47:35:56.0: 13.29 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:08:40.72 +42:33:53.2: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.94 +/- 0.02
Forced photometry filter REJECTED candidate at 05:08:40.72 +42:33:53.2: ref_mag=12.94 +/- 0.02 new_mean_mag=13.1782 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:06:38.90 +47:35:56.0: 13.32 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.03
Forced photometry filter REJECTED candidate at 05:06:38.90 +47:35:56.0: ref_mag=13.31 +/- 0.03 new_mean_mag=13.2242 delta=0.08 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:12:43.10 +47:37:37.8: 13.76 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:38:30.55 +42:57:37.3: 13.43 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:12:43.10 +47:37:37.8: 13.76 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:25:36.52 +43:50:14.6: 13.57 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter REJECTED candidate at 05:12:43.10 +47:37:37.8: ref_mag=13.76 +/- 0.04 new_mean_mag=13.7347 delta=0.03 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:38:30.55 +42:57:37.3: 13.44 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter REJECTED candidate at 04:38:30.55 +42:57:37.3: ref_mag=13.44 +/- 0.03 new_mean_mag=13.3105 delta=0.13 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:08.66 +44:27:33.9: 14.20 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:30.94 +47:03:01.8: 14.37 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:25:36.52 +43:50:14.6: 13.53 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.55 +/- 0.04
Forced photometry filter REJECTED candidate at 04:25:36.52 +43:50:14.6: ref_mag=13.55 +/- 0.04 new_mean_mag=13.3601 delta=0.19 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:49.10 +46:53:59.6: 14.35 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:47:40.60 +42:56:59.0: 13.54 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:41.02 +46:55:26.5: 14.42 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:53:44.82 +44:37:40.3: 14.69 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:08.66 +44:27:33.9: 14.20 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:30.94 +47:03:01.8: 14.36 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Forced photometry filter REJECTED candidate at 04:56:08.66 +44:27:33.9: ref_mag=14.20 +/- 0.04 new_mean_mag=13.3032 delta=0.90 (need > 0.90)
Forced photometry reference-image weighted average: 14.36 +/- 0.05
Forced photometry filter REJECTED candidate at 04:56:30.94 +47:03:01.8: ref_mag=14.36 +/- 0.05 new_mean_mag=13.5352 delta=0.83 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:49.10 +46:53:59.6: 14.41 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.38 +/- 0.05
Forced photometry filter KEPT candidate at 05:01:49.10 +46:53:59.6: ref_mag=14.38 +/- 0.05 new_mean_mag=13.4602 delta=0.92 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:47:40.60 +42:56:59.0: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Forced photometry filter REJECTED candidate at 04:47:40.60 +42:56:59.0: ref_mag=13.58 +/- 0.03 new_mean_mag=13.4584 delta=0.12 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:11.87 +46:44:18.7: 14.33 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:41.02 +46:55:26.5: 14.46 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.44 +/- 0.05
Forced photometry filter KEPT candidate at 04:55:41.02 +46:55:26.5: ref_mag=14.44 +/- 0.05 new_mean_mag=13.4602 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:53:44.82 +44:37:40.3: 14.48 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.57 +/- 0.06
Forced photometry filter KEPT candidate at 04:53:44.82 +44:37:40.3: ref_mag=14.57 +/- 0.06 new_mean_mag=13.5727 delta=1.00 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:11.87 +46:44:18.7: 14.52 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.05
Forced photometry filter REJECTED candidate at 04:55:11.87 +46:44:18.7: ref_mag=14.41 +/- 0.05 new_mean_mag=13.5707 delta=0.84 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:00:18.53 +46:13:03.1: 13.72 +/- 0.05 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:50.48 +46:51:49.7: 14.64 +/- 0.09 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:57.90 +46:52:12.6: 14.62 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:00:18.53 +46:13:03.1: 13.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter REJECTED candidate at 05:00:18.53 +46:13:03.1: ref_mag=13.73 +/- 0.03 new_mean_mag=13.4624 delta=0.27 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:47.62 +47:00:52.9: 14.48 +/- 0.08 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:50.48 +46:51:49.7: 14.49 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.06
Forced photometry filter KEPT candidate at 04:55:50.48 +46:51:49.7: ref_mag=14.55 +/- 0.06 new_mean_mag=13.5682 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:57.90 +46:52:12.6: 14.52 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.06
Forced photometry filter KEPT candidate at 04:55:57.90 +46:52:12.6: ref_mag=14.56 +/- 0.06 new_mean_mag=13.5801 delta=0.98 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:18.01 +47:05:10.0: 14.43 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:47.62 +47:00:52.9: 14.35 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.41 +/- 0.05
Forced photometry filter KEPT candidate at 04:55:47.62 +47:00:52.9: ref_mag=14.41 +/- 0.05 new_mean_mag=13.3955 delta=1.01 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:18.01 +47:05:10.0: 14.23 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.31 +/- 0.05
Forced photometry filter KEPT candidate at 05:02:18.01 +47:05:10.0: ref_mag=14.31 +/- 0.05 new_mean_mag=13.3551 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:54:43.69 +44:08:15.9: 13.85 +/- 0.04 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:54:43.69 +44:08:15.9: 13.79 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.03
Forced photometry filter REJECTED candidate at 04:54:43.69 +44:08:15.9: ref_mag=13.82 +/- 0.03 new_mean_mag=13.2483 delta=0.57 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:58.27 +47:05:38.1: 14.34 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:58.27 +47:05:38.1: 14.40 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.37 +/- 0.05
Forced photometry filter KEPT candidate at 05:01:58.27 +47:05:38.1: ref_mag=14.37 +/- 0.05 new_mean_mag=13.4259 delta=0.95 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:53:28.38 +48:35:07.5: 14.02 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:53:28.38 +48:35:07.5: 13.95 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.04
Forced photometry filter REJECTED candidate at 04:53:28.38 +48:35:07.5: ref_mag=13.98 +/- 0.04 new_mean_mag=13.3255 delta=0.66 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:45:15.80 +43:10:19.3: 14.29 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:55.62 +46:52:25.7: 14.29 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:45:15.80 +43:10:19.3: 14.27 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.05
Forced photometry filter KEPT candidate at 04:45:15.80 +43:10:19.3: ref_mag=14.28 +/- 0.05 new_mean_mag=13.3372 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:55.62 +46:52:25.7: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.04
Forced photometry filter KEPT candidate at 04:55:55.62 +46:52:25.7: ref_mag=14.22 +/- 0.04 new_mean_mag=13.2811 delta=0.94 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:01:44.23 +47:26:09.7: 14.24 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:01:44.23 +47:26:09.7: 14.16 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Forced photometry filter REJECTED candidate at 05:01:44.23 +47:26:09.7: ref_mag=14.20 +/- 0.04 new_mean_mag=13.3071 delta=0.89 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:55:49.33 +46:55:50.7: 14.23 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 04:56:02.66 +47:02:28.1: 14.25 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:55:49.33 +46:55:50.7: 14.21 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.04
Forced photometry filter KEPT candidate at 04:55:49.33 +46:55:50.7: ref_mag=14.22 +/- 0.04 new_mean_mag=13.2995 delta=0.92 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 04:56:02.66 +47:02:28.1: 14.22 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.04
Forced photometry filter KEPT candidate at 04:56:02.66 +47:02:28.1: ref_mag=14.24 +/- 0.04 new_mean_mag=13.2729 delta=0.96 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:03:56.83 +46:49:54.6: 14.17 +/- 0.06 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:03:56.83 +46:49:54.6: 14.13 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.15 +/- 0.04
Forced photometry filter KEPT candidate at 05:03:56.83 +46:49:54.6: ref_mag=14.15 +/- 0.04 new_mean_mag=13.2405 delta=0.91 (need > 0.90)
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-37-33_20.00sec_-15.00C_LIGHT_0044.fits at 05:02:02.63 +46:42:23.7: 14.15 +/- 0.07 detection
Forced photometry on wcs_Per-03-Q2b1x1_2026-02-21_20-38-19_20.00sec_-15.00C_LIGHT_0045.fits at 05:02:02.63 +46:42:23.7: 14.25 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.19 +/- 0.05
Forced photometry filter KEPT candidate at 05:02:02.63 +46:42:23.7: ref_mag=14.19 +/- 0.05 new_mean_mag=13.2230 delta=0.97 (need > 0.90)
Adding exclusion_list_local.txt__out112432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72303.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 31s
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: 8s
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Considering the candidate 221433_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221433_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:58:25.30 +46:42:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221434_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221434_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221436_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221436_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221447_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221447_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:28:55.30 +45:49:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221451_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221451_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221466_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221466_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:51:17.65 +43:39:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221467_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221467_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221468_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221468_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 05:02:30.69 +44:40:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221470_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221470_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221471_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221471_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:35:23.05 +42:22:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221472_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221472_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221484_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221484_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:29:40.39 +42:26:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221485_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221485_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221489_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221489_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221491_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221491_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:50:51.96 +42:58:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221492_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221492_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221495_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221495_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:24:23.85 +42:39:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221497_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221497_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221499_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221499_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:56:51.06 +42:50:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221500_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221500_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:28:50.89 +41:45:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221501_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221501_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:30:19.01 +45:56:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221503_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221503_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221504_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221504_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:30:26.69 +41:49:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221506_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221506_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:25:01.83 +44:15:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 221510_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221510_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 221513_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 221513_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 223979_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 223979_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:55:46.89 +43:10:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 224409_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 224409_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 05:00:41.04 +43:33:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 225522_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 225522_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 225750_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 225750_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:47:24.60 +46:00:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226194_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 226194_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:23:59.83 +41:56:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226423_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 226423_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:43:32.00 +49:59:18.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 226861_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 226861_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:24:24.67 +41:42:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 226915_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 226915_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 05:06:36.75 +46:13:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227454_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 227454_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
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Considering the candidate 227479_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 227479_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 05:12:14.35 +45:35:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227696_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 227696_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:46:53.66 +43:00:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227800_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 227800_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:48:56.31 +43:15:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 227973_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 227973_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:52:57.40 +42:34:51.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 228033_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 228033_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:55:24.15 +43:25:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228502_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 228502_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:46:20.88 +42:21:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228579_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 228579_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:51:41.73 +42:03:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228801_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 228801_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:35:36.66 +45:11:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228873_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 228873_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 05:01:52.92 +43:51:44.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 228907_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 228907_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:55:20.30 +43:23:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229073_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 229073_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:49:32.98 +46:30:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229084_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 229084_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:58:01.71 +49:10:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229335_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 229335_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:36:40.80 +45:00:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229347_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 229347_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:54:55.06 +42:57:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229379_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 229379_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:56:55.86 +43:08:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229578_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 229578_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 229776_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 229776_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:40:04.81 +43:16:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 229824_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 229824_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 05:02:06.96 +44:00:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230190_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 230190_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:27:48.21 +46:15:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230207_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 230207_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:48:26.07 +43:18:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230221_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 230221_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:57:58.14 +49:13:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230427_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 230427_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 230496_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 230496_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:55:50.62 +43:08:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230498_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 230498_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 05:11:12.06 +42:54:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230632_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 230632_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 05:02:06.58 +43:47:07.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 230759_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 230759_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:46:55.07 +43:00:58.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 231062_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 231062_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 05:11:47.44 +45:38:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231288_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 231288_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:34:50.79 +43:27:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231417_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 231417_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:28:17.78 +44:43:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231547_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 231547_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:53:16.29 +42:56:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231704_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 231704_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 05:04:16.11 +45:48:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 231893_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 231893_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:34:09.86 +45:55:33.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232015_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 232015_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 05:10:58.74 +43:36:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 232057_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 232057_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:57:13.74 +46:34:35.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232060_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 232060_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232185_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 232185_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:48:56.65 +43:59:05.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233443_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 233443_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:48:15.84 +42:48:54.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233692_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 233692_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:56:13.99 +47:27:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233941_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 233941_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:46:20.23 +43:34:19.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234006_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 234006_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:46:35.14 +42:20:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234251_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 234251_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234615_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 234615_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234657_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 234657_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:41:35.56 +42:05:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235162_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 235162_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:53:35.58 +46:33:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115045_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 115045_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68798_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 68798_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70176_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 70176_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208602_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 208602_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73213_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 73213_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:58:46.28 +46:41:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112432_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 112432_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209625_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 209625_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209464_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 209464_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81676_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 81676_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70856_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 70856_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70914_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 70914_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25749_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 25749_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:21:35.37 +49:37:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68281_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 68281_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65274_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 65274_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138372_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 138372_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:39:20.27 +43:29:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93325_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 93325_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:52:33.40 +45:41:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121836_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 121836_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65237_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 65237_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41591_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 41591_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170083_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 170083_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:27:32.51 +41:47:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144553_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 144553_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70798_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 70798_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59336_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 59336_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69724_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 69724_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67814_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 67814_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69382_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 69382_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72303_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
Preparing report for the candidate 72303_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193050_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 193050_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:23:13.89 +42:49:37.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51769_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 51769_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
**** FOUND 04:33:43.83 +48:06:53.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95776_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139
The candidate 95776_fd_Per-03-Q2b1x1_2026-09-10_06-14-09_20.00sec_0.00C_LIGHT_0139 did not pass the final checks
