This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 15.1386 2461206.6386 12.31 08:36:01.26 +38:01:07.9
184.06466 36.14364 galactic Lyn 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 | 08:36:01.26 +38:01:07.9 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.391+/-0.030 (G)
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:36:01.26 +38:01:07.9: 13.29 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:36:01.26 +38:01:07.9: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6386,12.31,0.05,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 20260615.1386 12.31CV 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 06 15.1386 2461206.6386 12.39 08:38:35.90 +35:37:04.9
187.10386 36.27402 galactic Lyn Second-epoch detections are separated by 0.4" and 9.4 pix
The object was found in VSX 0" Gaia DR3 717569914245367168
Type: ROT
# Max. Min./Amp. JD0 Period
13.300 G 13.320 G G
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:38:35.90 +35:37:04.9: 13.52 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:38:35.90 +35:37:04.9: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 717569914245367168,2461206.6386,12.39,0.05,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 717569914245367168 20260615.1386 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1386 2461206.6386 12.51 08:32:02.63 +40:56:36.8
180.35769 35.76988 galactic Lyn Second-epoch detections are separated by 1.0" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:32:02.63 +40:56:36.8 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5) J-Ks=0.673+/-0.032 (K)
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:32:02.63 +40:56:36.8: 13.49 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:32:02.63 +40:56:36.8: 13.55 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6386,12.51,0.05,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 20260615.1386 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1386 2461206.6386 12.36 08:37:00.93 +36:18:24.5
186.19622 36.07355 galactic Lyn Second-epoch detections are separated by 1.3" 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 | ATO J129.2497+36.3067 | 08:37:00.93 +36:18:24.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: K3 (LAMOST DR5) J-Ks=0.577+/-0.028 (K)
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:37:00.93 +36:18:24.5: 13.47 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:37:00.93 +36:18:24.5: 13.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J129.2497+36.3067,2461206.6386,12.36,0.05,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 J129.2497+36.3067 20260615.1386 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1386 2461206.6386 12.22 08:40:05.28 +34:05:36.2
189.03267 36.30338 galactic Lyn Second-epoch detections are separated by 0.4" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:40:05.28 +34:05:36.2 (user input) | T | P | (position from user input) SpType: G6 (LAMOST DR5) J-Ks=0.465+/-0.033 (K)
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:40:05.28 +34:05:36.2: 13.22 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:40:05.28 +34:05:36.2: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6386,12.22,0.05,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 20260615.1386 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1386 2461206.6386 12.49 08:34:18.83 +35:12:36.2
187.40857 35.34268 galactic Lyn Second-epoch detections are separated by 1.1" and 9.4 pix
The object was found in VSX 1" Gaia DR3 903681979736001664
Type: ROT
# Max. Min./Amp. JD0 Period
13.160 G 13.190 G K
The object was not found in astcheck.
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:34:18.83 +35:12:36.2: 13.44 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:34:18.83 +35:12:36.2: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 903681979736001664,2461206.6386,12.49,0.05,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 903681979736001664 20260615.1386 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1386 2461206.6386 12.55 08:40:51.81 +35:34:07.5
187.26051 36.71969 galactic Lyn Second-epoch detections are separated by 2.4" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:40:51.81 +35:34:07.5 (user input) | T | P | (position from user input) J-Ks=0.384+/-0.033 (G)
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:40:51.81 +35:34:07.5: 13.70 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:40:51.81 +35:34:07.5: 13.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6386,12.55,0.05,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 20260615.1386 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1386 2461206.6386 12.55 08:38:04.47 +37:10:36.5
185.17265 36.42069 galactic Lyn Second-epoch detections are separated by 1.7" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:38:04.47 +37:10:36.5 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.428+/-0.033 (G)
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:38:04.47 +37:10:36.5: 13.63 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:38:04.47 +37:10:36.5: 13.58 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6386,12.55,0.05,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 20260615.1386 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1386 2461206.6386 12.36 08:36:23.31 +34:58:41.6
187.78408 35.71745 galactic Lyn Second-epoch detections are separated by 0.7" 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 | 08:36:23.31 +34:58:41.6 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5) J-Ks=0.398+/-0.028 (G)
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:36:23.31 +34:58:41.6: 13.35 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:36:23.31 +34:58:41.6: 13.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6386,12.36,0.05,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 20260615.1386 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1386 2461206.6386 12.53 08:35:41.14 +39:20:41.2
182.42599 36.26156 galactic Lyn Second-epoch detections are separated by 1.5" and 9.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:35:41.14 +39:20:41.2 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5) J-Ks=0.330+/-0.033 (G)
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:35:41.14 +39:20:41.2: 13.59 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:35:41.14 +39:20:41.2: 13.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6386,12.53,0.05,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 20260615.1386 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1386 2461206.6386 12.36 08:39:05.38 +35:06:35.0
187.74638 36.28492 galactic Lyn Second-epoch detections are separated by 0.8" 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 | 08:39:05.38 +35:06:35.0 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5) J-Ks=0.392+/-0.025 (G)
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:39:05.38 +35:06:35.0: 13.26 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:39:05.38 +35:06:35.0: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461206.6386,12.36,0.05,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 20260615.1386 12.36CV 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: 2461093.72163340 22.02.2026 05:18:59.126 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
First image: 2461093.72163340 22.02.2026 05:18:59.126 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Last image: 2461206.63883482 15.06.2026 03:19:45.328 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
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: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7886
Objects passed selection criteria: 7814
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 4586
Average stars matched: 4448.75 (97.0072 %)
Memory usage VmPeak: 114192 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 14 23:25:20 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: 2461093.72163340 22.02.2026 05:18:59.126 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
First image: 2461093.72163340 22.02.2026 05:18:59.126 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Last image: 2461206.63883482 15.06.2026 03:19:45.328 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 17
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.17
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: 9 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 45980
Objects passed selection criteria: 45813
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 28565.5
Average stars matched: 27310.2 (95.6057 %)
Memory usage VmPeak: 149840 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 14 23:26:50 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
SExtractor catalog cache: saved Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat to cache
SExtractor catalog cache: saved Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.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: 2461206.63831199
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_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits exists and is non-empty
Saving wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits to local_wcs_cache/
'wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits' -> 'local_wcs_cache/wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits'
wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits exists and is non-empty
Saving wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits to local_wcs_cache/
'wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits' -> 'local_wcs_cache/wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits'
wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits exists and is non-empty
Saving wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits to local_wcs_cache/
'wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits' -> 'local_wcs_cache/wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits'
wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits exists and is non-empty
Saving wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits to local_wcs_cache/
'wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits' -> 'local_wcs_cache/wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits (1st reference image)
verification OK: wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:43:38.069 +38:00:02.87 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_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits (1st new image)
verification OK: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:43:58.893 +38:00:13.94 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:43:38.069 +38:00:02.87
Second-epoch image center 08:43:58.893 +38:00:13.94
Angular distance between the image centers 0.0684 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits (2nd new image)
verification OK: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:43:55.546 +38:00:52.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:43:38.069 +38:00:02.87
Second-epoch image center 08:43:55.546 +38:00:52.60
Angular distance between the image centers 0.0590 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:43:58.893 +38:00:13.94
Second-epoch second image center 08:43:55.546 +38:00:52.60
Angular distance between the image centers 0.01536 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits &> /tmp/tmp.PjYSDRmTGZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits &> /tmp/tmp.ApDXpXBPXu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits &> /tmp/tmp.FJkGCPlAIS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits &> /tmp/tmp.PI8qgsORL2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.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_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.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_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat
Found non-empty wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat
The reference image (wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits) and catalog (wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat) found
'wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat' -> 'wcsmag.cat'
Read 10321 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 119.9860 to 141.1683 deg, Dec +32.0300 to +43.3754 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 119.9860 to 141.1683 deg, Dec 32.0300 to 43.3754 deg
Loaded 6986 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): 4957 out of 5292 total matches.
Matched with Tycho-2 5292 out of 10321 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.916500
a=0.000000 b=1.000000 c=22.916500
From vast_summary.log: estimated ref. image limiting mag.: -7.46
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 10321 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 119.9860 to 141.1683 deg, Dec +32.0300 to +43.3754 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 119.9860 to 141.1683 deg, Dec 32.0300 to 43.3754 deg
Loaded 6986 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): 4957 out of 5292 total matches.
Matched with Tycho-2 5292 out of 10321 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits:
Forced-photometry filter: calibrated wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits -> calib.txt_param_ref_wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits (aperture=6.3)
Read 10235 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 119.9089 to 141.1680 deg, Dec +32.0509 to +43.3885 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 119.9089 to 141.1680 deg, Dec 32.0509 to 43.3885 deg
Loaded 6999 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): 4924 out of 5290 total matches.
Matched with Tycho-2 5290 out of 10235 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits:
Forced-photometry filter: calibrated wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits -> calib.txt_param_ref_wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
2.1 pix Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
2.4 pix fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
2.4 pix fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
2.1 pix wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
2.1 pix wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Limiting magnitude estimates:
15.5 mag. Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
15.5 mag. Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
12.0 mag. fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
12.2 mag. fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
All-image limiting magnitude estimate: 12.0 (SNR ) 10.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.PjYSDRmTGZ (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/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits' -> 'wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS-calibrated image found: wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Checking if the catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat corresponding to the image wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat corresponding to the image wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS catalog name: wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=776, passed=10321
Got 10321 stars (including 9534 good ones) from the SExtractor catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat
util/solve_plate_with_UCAC5 got 10321 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 10183 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 10184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 10184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits N_match=974 sigma_overall_arcsec=0.394 sigma_q1_arcsec=0.494 sigma_q2_arcsec=0.388 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.347 n_q1=241 n_q2=221 n_q3=281 n_q4=231 worst_quadrant_to_overall_ratio=1.253
The image catalog is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits -region wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ApDXpXBPXu (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/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits' -> 'wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Checking if the catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat corresponding to the image wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat corresponding to the image wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS catalog name: wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=799, passed=10235
Got 10235 stars (including 9422 good ones) from the SExtractor catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat
util/solve_plate_with_UCAC5 got 10235 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 10123 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
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 10123 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 10123 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits N_match=973 sigma_overall_arcsec=0.441 sigma_q1_arcsec=0.540 sigma_q2_arcsec=0.459 sigma_q3_arcsec=0.404 sigma_q4_arcsec=0.415 n_q1=247 n_q2=221 n_q3=275 n_q4=230 worst_quadrant_to_overall_ratio=1.223
The image catalog is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits -region wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FJkGCPlAIS (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
Checking if the catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat corresponding to the image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat corresponding to the image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
WCS catalog name: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=46, passed=1408
Got 1408 stars (including 1361 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat
util/solve_plate_with_UCAC5 got 1408 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 1334 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
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 1335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 1335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits N_match=971 sigma_overall_arcsec=0.493 sigma_q1_arcsec=0.459 sigma_q2_arcsec=0.536 sigma_q3_arcsec=0.496 sigma_q4_arcsec=0.473 n_q1=122 n_q2=388 n_q3=142 n_q4=319 worst_quadrant_to_overall_ratio=1.088
The image catalog is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits -region wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PI8qgsORL2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
Checking if the catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat corresponding to the image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat corresponding to the image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
WCS catalog name: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=48, passed=1495
Got 1495 stars (including 1446 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat
util/solve_plate_with_UCAC5 got 1495 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 1450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.2)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 1448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 1448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits N_match=969 sigma_overall_arcsec=0.531 sigma_q1_arcsec=0.509 sigma_q2_arcsec=0.555 sigma_q3_arcsec=0.527 sigma_q4_arcsec=0.508 n_q1=145 n_q2=342 n_q3=173 n_q4=309 worst_quadrant_to_overall_ratio=1.046
The image catalog is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits -region wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits sigma_overall=0.394 worst_q_ratio=1.253
ref2=Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits sigma_overall=0.441 worst_q_ratio=1.223
new1=fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits sigma_overall=0.493 worst_q_ratio=1.088
new2=fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits sigma_overall=0.531 worst_q_ratio=1.046
reference average sigma_overall=0.4175 worst_q_ratio=1.238
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207_astrometric_residuals.png (974 matched stars from wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208_astrometric_residuals.png (973 matched stars from wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034_astrometric_residuals.png (971 matched stars from wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035_astrometric_residuals.png (969 matched stars from wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits'
Saving fully-calibrated image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits'
Preparing the HTML report for the field Lyn-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20459_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
The candidate 20459_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035 did not pass the final checks
**** FOUND 08:25:31.41 +35:24:14.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Lyn-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
SExtractor catalog cache: saved Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat to cache
SExtractor catalog cache: saved Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Creating symlink local_wcs_cache/wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits exists and is non-empty
wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits exists and is non-empty
wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits exists and is non-empty
wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits (1st reference image)
verification OK: wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:43:38.069 +38:00:02.87 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_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits (1st new image)
verification OK: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:43:58.893 +38:00:13.94 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:43:38.069 +38:00:02.87
Second-epoch image center 08:43:58.893 +38:00:13.94
Angular distance between the image centers 0.0684 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits (2nd new image)
verification OK: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
Image size: 937.8'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:43:55.546 +38:00:52.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:43:38.069 +38:00:02.87
Second-epoch image center 08:43:55.546 +38:00:52.60
Angular distance between the image centers 0.0590 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:43:58.893 +38:00:13.94
Second-epoch second image center 08:43:55.546 +38:00:52.60
Angular distance between the image centers 0.01536 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits &> /tmp/tmp.RVvanXMl0B
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits &> /tmp/tmp.t6J4XYzOmO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits &> /tmp/tmp.5nPbynpk63
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits &> /tmp/tmp.qbbMYKm7LQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.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_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.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_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat
Found non-empty wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits and wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat
The reference image (wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits) and catalog (wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat) found
'wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat' -> 'wcsmag.cat'
Read 58327 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 119.9105 to 141.2591 deg, Dec +31.9813 to +43.3876 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 119.9105 to 141.2591 deg, Dec 31.9813 to 43.3876 deg
Loaded 7080 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): 4555 out of 5331 total matches.
Matched with Tycho-2 5331 out of 58327 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.797900
a=0.000000 b=1.000000 c=22.797900
From vast_summary.log: estimated ref. image limiting mag.: -7.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.63
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.63
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 58327 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 119.9105 to 141.2591 deg, Dec +31.9813 to +43.3876 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 119.9105 to 141.2591 deg, Dec 31.9813 to 43.3876 deg
Loaded 7080 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): 4555 out of 5331 total matches.
Matched with Tycho-2 5331 out of 58327 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits:
Forced-photometry filter: calibrated wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits -> calib.txt_param_ref_wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits (aperture=4.8)
Read 58690 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 119.9089 to 141.2531 deg, Dec +32.0019 to +43.3962 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 119.9089 to 141.2531 deg, Dec 32.0019 to 43.3962 deg
Loaded 7068 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): 4517 out of 5330 total matches.
Matched with Tycho-2 5330 out of 58690 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits:
Forced-photometry filter: calibrated wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits -> calib.txt_param_ref_wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
2.0 pix Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
2.2 pix fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
2.0 pix fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
2.0 pix wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
2.0 pix wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Limiting magnitude estimates:
15.6 mag. Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
15.6 mag. Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
12.7 mag. fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
12.9 mag. fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 12.6 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.RVvanXMl0B (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/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits' -> 'wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS-calibrated image found: wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Checking if the catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat corresponding to the image wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat corresponding to the image wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS catalog name: wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=3509, passed=58308
Got 58308 stars (including 54702 good ones) from the SExtractor catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat
util/solve_plate_with_UCAC5 got 58308 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 57676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 57676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 57676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits N_match=974 sigma_overall_arcsec=0.416 sigma_q1_arcsec=0.501 sigma_q2_arcsec=0.420 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.357 n_q1=241 n_q2=220 n_q3=283 n_q4=230 worst_quadrant_to_overall_ratio=1.206
The image catalog is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits -region wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.t6J4XYzOmO (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/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits' -> 'wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Checking if the catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat corresponding to the image wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat corresponding to the image wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS catalog name: wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=3533, passed=58663
Got 58663 stars (including 55036 good ones) from the SExtractor catalog wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat
util/solve_plate_with_UCAC5 got 58663 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 58156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 58156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 58156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits N_match=974 sigma_overall_arcsec=0.466 sigma_q1_arcsec=0.560 sigma_q2_arcsec=0.451 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.420 n_q1=244 n_q2=222 n_q3=280 n_q4=228 worst_quadrant_to_overall_ratio=1.201
The image catalog is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits -region wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5nPbynpk63 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
Checking if the catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat corresponding to the image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat corresponding to the image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
WCS catalog name: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=190, passed=9993
Got 9993 stars (including 9792 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat
util/solve_plate_with_UCAC5 got 9993 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 9402 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 9398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 9398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 966 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits N_match=966 sigma_overall_arcsec=0.491 sigma_q1_arcsec=0.486 sigma_q2_arcsec=0.525 sigma_q3_arcsec=0.469 sigma_q4_arcsec=0.484 n_q1=124 n_q2=384 n_q3=142 n_q4=316 worst_quadrant_to_overall_ratio=1.070
The image catalog is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits -region wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qbbMYKm7LQ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
Checking if the catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat corresponding to the image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat corresponding to the image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
WCS catalog name: wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=353, passed=11285
Got 11285 stars (including 10915 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat
util/solve_plate_with_UCAC5 got 11285 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 10947 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
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 10950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 10950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 960 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits N_match=960 sigma_overall_arcsec=0.518 sigma_q1_arcsec=0.553 sigma_q2_arcsec=0.540 sigma_q3_arcsec=0.512 sigma_q4_arcsec=0.475 n_q1=150 n_q2=338 n_q3=173 n_q4=299 worst_quadrant_to_overall_ratio=1.067
The image catalog is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits -region wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-00_20.00sec_5.00C_LIGHT_0034.fits
Saving fully-calibrated image wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Lyn-06-Q2b1x1_232106_TTUQ2b1x1_1612118_dASUT4pM/wcs_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035.fits
Preparing the HTML report for the field Lyn-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:40:05.28 +34:05:36.2: 13.22 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:37:00.93 +36:18:24.5: 13.47 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:36:23.31 +34:58:41.6: 13.35 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:38:04.47 +37:10:36.5: 13.63 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:36:01.26 +38:01:07.9: 13.29 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:32:02.63 +40:56:36.8: 13.49 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:40:51.81 +35:34:07.5: 13.70 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:38:35.90 +35:37:04.9: 13.52 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:34:18.83 +35:12:36.2: 13.44 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:35:41.14 +39:20:41.2: 13.59 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:40:51.81 +35:34:07.5: 13.64 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:37:00.93 +36:18:24.5: 13.36 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:32:02.63 +40:56:36.8: 13.55 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:36:23.31 +34:58:41.6: 13.29 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:36:01.26 +38:01:07.9: 13.29 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:34:18.83 +35:12:36.2: 13.48 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:40:05.28 +34:05:36.2: 13.17 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:38:04.47 +37:10:36.5: 13.58 +/- 0.03 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:38:35.90 +35:37:04.9: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.02
Forced photometry reference-image weighted average: 13.67 +/- 0.02
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry reference-image weighted average: 13.41 +/- 0.02
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry filter KEPT candidate at 08:40:51.81 +35:34:07.5: ref_mag=13.67 +/- 0.02 new_mean_mag=12.5185 delta=1.15 (need > 0.90)
Forced photometry reference-image weighted average: 13.46 +/- 0.02
Forced photometry filter KEPT candidate at 08:32:02.63 +40:56:36.8: ref_mag=13.52 +/- 0.02 new_mean_mag=12.4429 delta=1.07 (need > 0.90)
Forced photometry filter KEPT candidate at 08:36:23.31 +34:58:41.6: ref_mag=13.32 +/- 0.02 new_mean_mag=12.3620 delta=0.96 (need > 0.90)
Forced photometry reference-image weighted average: 13.50 +/- 0.02
Forced photometry filter KEPT candidate at 08:36:01.26 +38:01:07.9: ref_mag=13.29 +/- 0.02 new_mean_mag=12.3091 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 13.19 +/- 0.01
Forced photometry filter KEPT candidate at 08:37:00.93 +36:18:24.5: ref_mag=13.41 +/- 0.02 new_mean_mag=12.3463 delta=1.06 (need > 0.90)
Forced photometry reference-image weighted average: 13.61 +/- 0.02
Forced photometry filter KEPT candidate at 08:34:18.83 +35:12:36.2: ref_mag=13.46 +/- 0.02 new_mean_mag=12.4653 delta=0.99 (need > 0.90)
Forced photometry filter KEPT candidate at 08:40:05.28 +34:05:36.2: ref_mag=13.19 +/- 0.01 new_mean_mag=12.2353 delta=0.96 (need > 0.90)
Forced photometry filter KEPT candidate at 08:38:35.90 +35:37:04.9: ref_mag=13.50 +/- 0.02 new_mean_mag=12.3749 delta=1.13 (need > 0.90)
Forced photometry filter KEPT candidate at 08:38:04.47 +37:10:36.5: ref_mag=13.61 +/- 0.02 new_mean_mag=12.5594 delta=1.05 (need > 0.90)
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:35:41.14 +39:20:41.2: 13.66 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.02
Forced photometry filter KEPT candidate at 08:35:41.14 +39:20:41.2: ref_mag=13.62 +/- 0.02 new_mean_mag=12.5071 delta=1.11 (need > 0.90)
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits at 08:39:05.38 +35:06:35.0: 13.26 +/- 0.02 detection
Forced photometry on wcs_Lyn-06-Q2b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits at 08:39:05.38 +35:06:35.0: 13.24 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.25 +/- 0.02
Forced photometry filter KEPT candidate at 08:39:05.38 +35:06:35.0: ref_mag=13.25 +/- 0.02 new_mean_mag=12.2986 delta=0.95 (need > 0.90)
Adding exclusion_list_local.txt__out07247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58221.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 72367_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
The candidate 72367_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035 did not pass the final checks
**** FOUND 08:33:30.87 +36:26:18.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 29400_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
Preparing report for the candidate 29400_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
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Considering the candidate 15630_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
Preparing report for the candidate 15630_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
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Considering the candidate 49954_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
Preparing report for the candidate 49954_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
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Considering the candidate 19619_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
Preparing report for the candidate 19619_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
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Considering the candidate 07247_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
Preparing report for the candidate 07247_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
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Considering the candidate 13677_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
Preparing report for the candidate 13677_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
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Considering the candidate 15189_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
Preparing report for the candidate 15189_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
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Considering the candidate 24426_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
Preparing report for the candidate 24426_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
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Considering the candidate 12220_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
Preparing report for the candidate 12220_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
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Considering the candidate 58221_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
Preparing report for the candidate 58221_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
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Considering the candidate 15712_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
The candidate 15712_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035 did not pass the final checks
**** FOUND 08:25:31.43 +35:24:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12761_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
Preparing report for the candidate 12761_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
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Considering the candidate 46611_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035
The candidate 46611_fd_Lyn-06-Q2b1x1_2026-06-14_22-19-45_20.00sec_5.00C_LIGHT_0035 did not pass the final checks
