This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq
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 08 22.3750 2461274.8750 12.16 18:08:56.60 +42:42:17.8
69.80895 25.45681 galactic Her Second-epoch detections are separated by 3.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:08:56.60 +42:42:17.8 (user input) | T | P | (position from user input)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:08:56.60 +42:42:17.8: 13.13 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:08:56.60 +42:42:17.8: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 08 56.60 +42 42 17.8 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8750,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3750 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3750 2461274.8750 12.19 18:10:33.33 +41:37:58.9
68.74719 24.89563 galactic Her Second-epoch detections are separated by 1.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:10:33.33 +41:37:58.9 (user input) | T | P | (position from user input) J-Ks=0.636+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:10:33.33 +41:37:58.9: 13.13 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:10:33.33 +41:37:58.9: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 10 33.33 +41 37 58.9 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8750,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3750 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3750 2461274.8750 12.44 18:11:01.93 +41:27:33.3
68.58804 24.76414 galactic Her Second-epoch detections are separated by 1.4" and 7.3 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 | DocumentRef: VOTx856838 | 18:11:01.93 +41:27:33.3 (user input) | (GCVS) | (GCVS) | (position from user input)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:11:01.93 +41:27:33.3: 13.55 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:11:01.93 +41:27:33.3: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 11 01.93 +41 27 33.3 12.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx856838,2461274.8750,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx856838 20260822.3750 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3750 2461274.8750 12.40 18:12:55.59 +41:29:43.4
68.72965 24.43154 galactic Her Second-epoch detections are separated by 0.8" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:12:55.59 +41:29:43.4 (user input) | T | P | (position from user input) J-Ks=0.545+/-0.028 (K)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:12:55.59 +41:29:43.4: 13.32 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:12:55.59 +41:29:43.4: 13.31 +/- 0.04 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!
TCP 2026 08 22.3750* 18 12 55.59 +41 29 43.4 12.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8750,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3750 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3750 2461274.8750 12.31 18:12:18.00 +41:28:28.5
68.67330 24.53910 galactic Her Second-epoch detections are separated by 1.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:12:18.00 +41:28:28.5 (user input) | T | P | (position from user input) J-Ks=0.319+/-0.028 (F)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:12:18.00 +41:28:28.5: 13.27 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:12:18.00 +41:28:28.5: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 12 18.00 +41 28 28.5 12.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8750,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3750 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 08 22.3750 2461274.8750 12.21 18:11:47.01 +40:28:54.2
67.59390 24.36642 galactic Her Second-epoch detections are separated by 1.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J272.9311+40.4873 | 18:11:47.01 +40:28:54.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.631+/-0.038 (K)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:11:47.01 +40:28:54.2: 13.20 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:11:47.01 +40:28:54.2: 13.24 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 11 47.01 +40 28 54.2 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J272.9311+40.4873,2461274.8750,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J272.9311+40.4873 20260822.3750 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3750 2461274.8750 12.24 18:10:15.25 +42:26:51.5
69.60027 25.15874 galactic Her Second-epoch detections are separated by 0.4" and 7.2 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 | 18:10:15.25 +42:26:51.5 (user input) | T | P | (position from user input) J-Ks=0.393+/-0.026 (G)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:10:15.25 +42:26:51.5: 13.20 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:10:15.25 +42:26:51.5: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 10 15.25 +42 26 51.5 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8750,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3750 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3750 2461274.8750 12.20 18:11:30.33 +42:21:03.2
69.56205 24.91068 galactic Her Second-epoch detections are separated by 1.2" and 7.2 pix
The object was found in VSX 2" ASASSN-V J181130.20+422103.5
Type: VAR
# Max. Min./Amp. JD0 Period
13.260 V 13.520 V
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:11:30.33 +42:21:03.2: 13.18 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:11:30.33 +42:21:03.2: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 11 30.33 +42 21 03.2 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181130.20+422103.5,2461274.8750,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181130.20+422103.5 20260822.3750 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3750 2461274.8750 12.22 18:08:30.47 +42:28:34.3
69.54147 25.47768 galactic Her Second-epoch detections are separated by 3.2" and 7.2 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 | 18:08:30.47 +42:28:34.3 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:08:30.47 +42:28:34.3: 13.15 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:08:30.47 +42:28:34.3: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 08 30.47 +42 28 34.3 12.2 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8750,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3750 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 08 22.3750 2461274.8750 12.08 18:09:30.99 +42:21:15.5
69.46244 25.26693 galactic Her Second-epoch detections are separated by 1.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:09:30.99 +42:21:15.5 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5) J-Ks=0.245+/-0.029 (F)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:09:30.99 +42:21:15.5: 13.04 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:09:30.99 +42:21:15.5: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 09 30.99 +42 21 15.5 12.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8750,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3750 12.08CV 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 08 22.3750 2461274.8750 12.12 18:09:11.11 +42:19:11.7
69.40858 25.31753 galactic Her Second-epoch detections are separated by 2.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 18:09:11.11 +42:19:11.7 (user input) | T | P | (position from user input) J-Ks=0.605+/-0.027 (K)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:09:11.11 +42:19:11.7: 13.02 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:09:11.11 +42:19:11.7: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 09 11.11 +42 19 11.7 12.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8750,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3750 12.12CV 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 08 22.3750 2461274.8750 12.04 18:12:04.08 +39:58:56.6
67.08337 24.17753 galactic Her Second-epoch detections are separated by 2.0" and 7.5 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 | 18:12:04.08 +39:58:56.6 (user input) | T | P | (position from user input) J-Ks=0.272+/-0.029 (F)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:12:04.08 +39:58:56.6: 13.01 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:12:04.08 +39:58:56.6: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 12 04.08 +39 58 56.6 12.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461274.8750,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.3750 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3750 2461274.8750 11.94 18:11:51.11 +41:52:45.1
69.07845 24.72641 galactic Her Second-epoch detections are separated by 1.3" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2113127830939701248 | 18:11:51.12 +41:52:45.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.901+/-0.026 (M)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:11:51.11 +41:52:45.1: 12.92 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:11:51.11 +41:52:45.1: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 11 51.11 +41 52 45.1 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2113127830939701248,2461274.8750,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2113127830939701248 20260822.3750 11.94CV 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 08 22.3750 2461274.8750 11.80 18:10:32.84 +40:38:49.4
67.69935 24.63706 galactic Her Second-epoch detections are separated by 0.9" and 7.1 pix
The object was found in VSX 1" V1522 Her
Type: EW
# Max. Min./Amp. JD0 Period
12.250 V 12.530 V 2456556.79470 0.374352800000
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:10:32.84 +40:38:49.4: 12.77 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:10:32.84 +40:38:49.4: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 10 32.84 +40 38 49.4 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1522 Her,2461274.8750,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1522 Her 20260822.3750 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.3750 2461274.8750 10.97 18:10:27.91 +42:39:23.2
69.83434 25.17388 galactic Her Second-epoch detections are separated by 0.6" and 7.2 pix
The object was found in VSX 4" ROTSE1 J181027.99+423926.0
Type: SR
# Max. Min./Amp. JD0 Period
13.053 g Y 0.280 g 2458227.58950 57.739851800000
The object was not found in astcheck.
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:10:27.91 +42:39:23.2: 11.95 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:10:27.91 +42:39:23.2: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 22.3750* 18 10 27.91 +42 39 23.2 11.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ROTSE1 J181027.99+423926.0,2461274.8750,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ROTSE1 J181027.99+423926.0 20260822.3750 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461176.89547439 16.05.2026 09:29:18.987 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
First image: 2461176.89547439 16.05.2026 09:29:18.987 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Last image: 2461274.87535392 22.08.2026 09:00:20.579 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 23525
Objects passed selection criteria: 23384
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: 14462.5
Average stars matched: 14022.8 (96.9594 %)
Memory usage VmPeak: 248080 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:04:47 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: 2461176.89547439 16.05.2026 09:29:18.987 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
First image: 2461176.89547439 16.05.2026 09:29:18.987 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Last image: 2461274.87535392 22.08.2026 09:00:20.579 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 117
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 21 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 143439
Objects passed selection criteria: 142944
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 96293.5
Average stars matched: 92363.8 (95.919 %)
Memory usage VmPeak: 542936 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:05:44 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
SExtractor catalog cache: saved Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.cat to cache
SExtractor catalog cache: saved Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.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/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.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: 2461274.87472303
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits exists and is non-empty
wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits exists and is non-empty
wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits exists and is non-empty
wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (1st reference image)
verification OK: wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:32:42.750 +37:59:52.55 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits (1st new image)
verification OK: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
Image size: 941.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:32:52.779 +38:00:08.00 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:32:42.750 +37:59:52.55
Second-epoch image center 18:32:52.779 +38:00:08.00
Angular distance between the image centers 0.0332 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits (2nd new image)
verification OK: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Image size: 941.9'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 18:32:53.656 +37:59:27.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:32:42.750 +37:59:52.55
Second-epoch image center 18:32:53.656 +37:59:27.20
Angular distance between the image centers 0.0365 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 18:32:52.779 +38:00:08.00
Second-epoch second image center 18:32:53.656 +37:59:27.20
Angular distance between the image centers 0.01169 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits &> /tmp/tmp.GxCoRCzMsm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits &> /tmp/tmp.zxVQ7ABtFV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits &> /tmp/tmp.aESre5HAtJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits &> /tmp/tmp.Ho2TIDyWBr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.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_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.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_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
Found non-empty wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
The reference image (wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits) and catalog (wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat) found
'wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat' -> 'wcsmag.cat'
Read 25255 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.6061 to 288.8205 deg, Dec +32.4326 to +43.2588 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 267.6061 to 288.8205 deg, Dec 32.4326 to 43.2588 deg
Loaded 16483 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): 11905 out of 12949 total matches.
Matched with Tycho-2 12949 out of 25255 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.754200
a=0.000000 b=1.000000 c=22.754200
From vast_summary.log: estimated ref. image limiting mag.: -7.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 25255 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.6061 to 288.8205 deg, Dec +32.4326 to +43.2588 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 267.6061 to 288.8205 deg, Dec 32.4326 to 43.2588 deg
Loaded 16483 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): 11905 out of 12949 total matches.
Matched with Tycho-2 12949 out of 25255 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Forced-photometry filter: calibrated wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits -> calib.txt_param_ref_wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (aperture=6.4)
Read 25065 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.6033 to 288.8211 deg, Dec +32.4339 to +43.2688 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 267.6033 to 288.8211 deg, Dec 32.4339 to 43.2688 deg
Loaded 16494 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): 11889 out of 12942 total matches.
Matched with Tycho-2 12942 out of 25065 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Forced-photometry filter: calibrated wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
2.3 pix Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
2.2 pix fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
2.2 pix fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Limiting magnitude estimates:
15.3 mag. Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
15.3 mag. Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
12.8 mag. fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
12.9 mag. fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
All-image limiting magnitude estimate: 12.8 (SNR ) 10.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.GxCoRCzMsm (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/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits' -> 'wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS_IMAGE_NAME=wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS-calibrated image found: wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Checking if the catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat corresponding to the image wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits alredy exist and is non-empty...
Catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat corresponding to the image wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS catalog name: wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2241, bad_region=0, passed=25255
Got 25255 stars (including 22995 good ones) from the SExtractor catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
util/solve_plate_with_UCAC5 got 25255 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 4906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 25255 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 25255 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4907 matched stars entering correct_measured_positions(), 25255 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4907 stars left (next iteration limit 5396)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits N_match=4907 sigma_overall_arcsec=0.460 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.555 sigma_q3_arcsec=0.421 sigma_q4_arcsec=0.526 n_q1=1082 n_q2=1527 n_q3=955 n_q4=1343 worst_quadrant_to_overall_ratio=1.205
The image catalog is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits -region wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.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.zxVQ7ABtFV (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/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits' -> 'wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS-calibrated image found: wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Checking if the catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS catalog name: wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2234, bad_region=1, passed=25065
Got 25065 stars (including 22805 good ones) from the SExtractor catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 25065 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 4904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4904 matched stars entering correct_measured_positions(), 25065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 25065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4905 matched stars entering correct_measured_positions(), 25065 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4905 stars left (next iteration limit 5394)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits N_match=4905 sigma_overall_arcsec=0.468 sigma_q1_arcsec=0.354 sigma_q2_arcsec=0.563 sigma_q3_arcsec=0.433 sigma_q4_arcsec=0.544 n_q1=1080 n_q2=1529 n_q3=959 n_q4=1337 worst_quadrant_to_overall_ratio=1.202
The image catalog is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits -region wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.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.aESre5HAtJ (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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
WCS-calibrated image found: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
Checking if the catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
WCS catalog name: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=183, bad_region=0, passed=3996
Got 3996 stars (including 3801 good ones) from the SExtractor catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat
util/solve_plate_with_UCAC5 got 3996 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 3733 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3712 matched stars entering correct_measured_positions(), 3711 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3712 matched stars entering correct_measured_positions(), 3995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 3732 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3711 matched stars entering correct_measured_positions(), 3995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 3711 matched stars entering correct_measured_positions(), 3995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 3711 stars left (next iteration limit 4083)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3711 robust_rms=6.329 arcsec worst_quadrant_rms=65.192 arcsec
SIP_REFIT: SIP order 3 trial: matched=3711 robust_rms=0.426 arcsec worst_quadrant_rms=0.451 arcsec
SIP_REFIT: SIP order 5 trial: matched=3711 robust_rms=0.350 arcsec worst_quadrant_rms=0.389 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3711 robust_rms_before=0.587 arcsec robust_rms_before_corrected=0.382 arcsec robust_rms_after=0.350 arcsec worst_quadrant_rms_before=0.483 worst_quadrant_rms_after=0.389
verification OK: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
verification OK: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
Image size: 942.0'x626.8' 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: 18:32:52.768 +38:00:08.01 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3996 stars ###
'wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/correct_sextractor_wcs_catalog_usingxy2sky1000367.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.587 -> 0.350 arcsec)
WCS_QUALITY_DIAG: file=fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits N_match=3711 sigma_overall_arcsec=0.375 sigma_q1_arcsec=0.386 sigma_q2_arcsec=0.426 sigma_q3_arcsec=0.349 sigma_q4_arcsec=0.391 n_q1=1228 n_q2=585 n_q3=1419 n_q4=479 worst_quadrant_to_overall_ratio=1.137
The image catalog is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits -region wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.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.Ho2TIDyWBr (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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
WCS-calibrated image found: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Checking if the catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
WCS catalog name: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=181, bad_region=0, passed=3954
Got 3954 stars (including 3770 good ones) from the SExtractor catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat
util/solve_plate_with_UCAC5 got 3954 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 3698 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3680 matched stars entering correct_measured_positions(), 3679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3680 matched stars entering correct_measured_positions(), 3953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 3697 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3680 matched stars entering correct_measured_positions(), 3953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 3680 matched stars entering correct_measured_positions(), 3953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 3680 stars left (next iteration limit 4048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3680 robust_rms=6.414 arcsec worst_quadrant_rms=54.897 arcsec
SIP_REFIT: SIP order 3 trial: matched=3680 robust_rms=0.463 arcsec worst_quadrant_rms=0.501 arcsec
SIP_REFIT: SIP order 5 trial: matched=3680 robust_rms=0.341 arcsec worst_quadrant_rms=0.361 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3680 robust_rms_before=0.612 arcsec robust_rms_before_corrected=0.393 arcsec robust_rms_after=0.341 arcsec worst_quadrant_rms_before=0.441 worst_quadrant_rms_after=0.361
verification OK: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
verification OK: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Image size: 942.0'x626.8' 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: 18:32:53.641 +37:59:27.15 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 3954 stars ###
'wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/correct_sextractor_wcs_catalog_usingxy2sky1000384.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.612 -> 0.341 arcsec)
WCS_QUALITY_DIAG: file=fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits N_match=3680 sigma_overall_arcsec=0.368 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.384 n_q1=1211 n_q2=588 n_q3=1396 n_q4=485 worst_quadrant_to_overall_ratio=1.090
The image catalog is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits -region wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits to local_wcs_cache/
'wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits' -> 'local_wcs_cache/wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits'
Saving the final (post-refit) wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits to local_wcs_cache/
'wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits' -> 'local_wcs_cache/wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits'
Saving the final (post-refit) wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits to local_wcs_cache/
'wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits' -> 'local_wcs_cache/wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits'
Saving the final (post-refit) wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits to local_wcs_cache/
'wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits' -> 'local_wcs_cache/wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits sigma_overall=0.460 worst_q_ratio=1.205
ref2=Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits sigma_overall=0.468 worst_q_ratio=1.202
new1=fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits sigma_overall=0.375 worst_q_ratio=1.137
new2=fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits sigma_overall=0.368 worst_q_ratio=1.090
reference average sigma_overall=0.464 worst_q_ratio=1.2035
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299_astrometric_residuals.png (4907 matched stars from wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300_astrometric_residuals.png (4905 matched stars from wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100_astrometric_residuals.png (3711 matched stars from wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101_astrometric_residuals.png (3680 matched stars from wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits'
Saving fully-calibrated image wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits'
Preparing the HTML report for the field Lyr-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31545_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 31545_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:44:48.12 +37:35:42.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31546_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 31546_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:50:06.72 +33:21:06.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31644_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 31644_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 17:54:59.15 +33:56:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05599_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 05599_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:44:52.08 +34:40:33.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09830_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 09830_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:45:32.08 +36:18:01.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12539_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 12539_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 17:56:15.33 +37:15:02.9 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Lyr-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
SExtractor catalog cache: saved Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.cat to cache
SExtractor catalog cache: saved Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Creating symlink local_wcs_cache/wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Creating symlink local_wcs_cache/wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
Creating symlink local_wcs_cache/wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits exists and is non-empty
wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits exists and is non-empty
wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits exists and is non-empty
wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (1st reference image)
verification OK: wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:32:42.750 +37:59:52.55 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits (1st new image)
verification OK: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
Image size: 942.0'x626.8' 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: 18:32:52.768 +38:00:08.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:32:42.750 +37:59:52.55
Second-epoch image center 18:32:52.768 +38:00:08.01
Angular distance between the image centers 0.0332 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits (2nd new image)
verification OK: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Image size: 942.0'x626.8' 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: 18:32:53.641 +37:59:27.15 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:32:42.750 +37:59:52.55
Second-epoch image center 18:32:53.641 +37:59:27.15
Angular distance between the image centers 0.0365 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 18:32:52.768 +38:00:08.01
Second-epoch second image center 18:32:53.641 +37:59:27.15
Angular distance between the image centers 0.01171 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits &> /tmp/tmp.HxIPiwjNlc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits &> /tmp/tmp.lbsnM06tZy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits &> /tmp/tmp.ZPyl1zKPLD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits &> /tmp/tmp.nOddEcXX3Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.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_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.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_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
Found non-empty wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits and wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
The reference image (wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits) and catalog (wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat) found
'wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat' -> 'wcsmag.cat'
Read 156217 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.5359 to 288.8250 deg, Dec +32.4126 to +43.2618 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 267.5359 to 288.8250 deg, Dec 32.4126 to 43.2618 deg
Loaded 16557 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): 9794 out of 13149 total matches.
Matched with Tycho-2 13149 out of 156217 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.626300
a=0.000000 b=1.000000 c=22.626300
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 156217 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.5359 to 288.8250 deg, Dec +32.4126 to +43.2618 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 267.5359 to 288.8250 deg, Dec 32.4126 to 43.2618 deg
Loaded 16557 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): 9794 out of 13149 total matches.
Matched with Tycho-2 13149 out of 156217 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Forced-photometry filter: calibrated wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits -> calib.txt_param_ref_wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (aperture=4.9)
Read 156924 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 267.5473 to 288.8404 deg, Dec +32.4215 to +43.2719 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 267.5473 to 288.8404 deg, Dec 32.4215 to 43.2719 deg
Loaded 16566 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): 9829 out of 13152 total matches.
Matched with Tycho-2 13152 out of 156924 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Forced-photometry filter: calibrated wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits -> calib.txt_param_ref_wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 107 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
2.1 pix Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
2.2 pix fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
2.2 pix fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Limiting magnitude estimates:
15.5 mag. Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
15.4 mag. Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
13.2 mag. fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
13.2 mag. fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.HxIPiwjNlc (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/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits' -> 'wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS_IMAGE_NAME=wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS-calibrated image found: wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
Checking if the catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat corresponding to the image wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits alredy exist and is non-empty...
Catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat corresponding to the image wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits
WCS catalog name: wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=81, blended=17837, bad_region=2, passed=156136
Got 156136 stars (including 138093 good ones) from the SExtractor catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat
util/solve_plate_with_UCAC5 got 156136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 4917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 156136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 156136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 156136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4918 stars left (next iteration limit 5408)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits N_match=4918 sigma_overall_arcsec=0.449 sigma_q1_arcsec=0.331 sigma_q2_arcsec=0.559 sigma_q3_arcsec=0.417 sigma_q4_arcsec=0.496 n_q1=1104 n_q2=1524 n_q3=994 n_q4=1296 worst_quadrant_to_overall_ratio=1.244
The image catalog is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits -region wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.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.lbsnM06tZy (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/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits' -> 'wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS-calibrated image found: wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
Checking if the catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits
WCS catalog name: wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=69, blended=17853, bad_region=2, passed=156855
Got 156855 stars (including 138804 good ones) from the SExtractor catalog wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 156855 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 4915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 156855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 612 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 156855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4915 matched stars entering correct_measured_positions(), 156855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4915 stars left (next iteration limit 5406)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits N_match=4915 sigma_overall_arcsec=0.470 sigma_q1_arcsec=0.363 sigma_q2_arcsec=0.570 sigma_q3_arcsec=0.444 sigma_q4_arcsec=0.505 n_q1=1105 n_q2=1524 n_q3=986 n_q4=1300 worst_quadrant_to_overall_ratio=1.212
The image catalog is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits -region wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.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.ZPyl1zKPLD (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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
WCS-calibrated image found: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
Checking if the catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
WCS catalog name: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1077, bad_region=27, passed=37625
Got 37625 stars (including 36436 good ones) from the SExtractor catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat
util/solve_plate_with_UCAC5 got 37625 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 4890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 37624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 4915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 37624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 37624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4891 stars left (next iteration limit 5379)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4891 robust_rms=5.803 arcsec worst_quadrant_rms=72.044 arcsec
SIP_REFIT: SIP order 3 trial: matched=4891 robust_rms=0.432 arcsec worst_quadrant_rms=0.458 arcsec
SIP_REFIT: SIP order 5 trial: matched=4891 robust_rms=0.353 arcsec worst_quadrant_rms=0.398 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4891 robust_rms_before=0.354 arcsec robust_rms_before_corrected=0.383 arcsec robust_rms_after=0.353 arcsec worst_quadrant_rms_before=0.396 worst_quadrant_rms_after=0.398
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.396 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits N_match=4891 sigma_overall_arcsec=0.385 sigma_q1_arcsec=0.394 sigma_q2_arcsec=0.450 sigma_q3_arcsec=0.361 sigma_q4_arcsec=0.392 n_q1=1728 n_q2=713 n_q3=1835 n_q4=615 worst_quadrant_to_overall_ratio=1.170
The image catalog is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits -region wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.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.nOddEcXX3Y (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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
WCS-calibrated image found: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Checking if the catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat corresponding to the image wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
WCS catalog name: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1079, bad_region=28, passed=36944
Got 36944 stars (including 35757 good ones) from the SExtractor catalog wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat
util/solve_plate_with_UCAC5 got 36944 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 4894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 36943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 36943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 36943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4896 stars left (next iteration limit 5383)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4896 robust_rms=5.950 arcsec worst_quadrant_rms=60.758 arcsec
SIP_REFIT: SIP order 3 trial: matched=4896 robust_rms=0.468 arcsec worst_quadrant_rms=0.505 arcsec
SIP_REFIT: SIP order 5 trial: matched=4896 robust_rms=0.350 arcsec worst_quadrant_rms=0.371 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4896 robust_rms_before=0.350 arcsec robust_rms_before_corrected=0.389 arcsec robust_rms_after=0.350 arcsec worst_quadrant_rms_before=0.374 worst_quadrant_rms_after=0.371
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.374 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits N_match=4896 sigma_overall_arcsec=0.396 sigma_q1_arcsec=0.398 sigma_q2_arcsec=0.445 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.385 n_q1=1698 n_q2=735 n_q3=1849 n_q4=614 worst_quadrant_to_overall_ratio=1.123
The image catalog is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits -region wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.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_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/wcs_fd_Lyr-02-Q1b1x1_2026-08-22_03-59-26_20.00sec_-0.00C_LIGHTs_0100.fits
Saving fully-calibrated image wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.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_2026-08-22_CI_Lyr-02-Q1b1x1_040100_TTUQ1b1x1_854494_1VIrCFxq/wcs_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101.fits
Preparing the HTML report for the field Lyr-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:10:07.38 +41:39:47.8: 12.93 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:11:04.42 +41:14:23.0: 12.52 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:12:43.84 +39:52:01.7: 12.48 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:58:09.78 +38:26:18.7: 12.84 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:58:33.84 +32:52:17.2: 12.59 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:04:47.65 +36:54:29.7: 12.55 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:54:53.78 +36:29:51.4: 12.60 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:08:51.53 +37:21:20.4: 12.50 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:02:37.14 +33:17:48.2: 12.56 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:58:33.84 +32:52:17.2: 12.67 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:11:04.42 +41:14:23.0: 12.45 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:04:47.65 +36:54:29.7: 12.54 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:12:43.84 +39:52:01.7: 12.47 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:54:53.78 +36:29:51.4: 12.66 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:10:07.38 +41:39:47.8: 13.03 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:58:09.78 +38:26:18.7: 12.94 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.48 +/- 0.01
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry reference-image weighted average: 12.97 +/- 0.02
Forced photometry filter REJECTED candidate at 19:11:04.42 +41:14:23.0: ref_mag=12.48 +/- 0.01 new_mean_mag=12.5661 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:58:33.84 +32:52:17.2: ref_mag=12.63 +/- 0.01 new_mean_mag=12.5695 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:12:43.84 +39:52:01.7: ref_mag=12.47 +/- 0.01 new_mean_mag=12.6704 delta=-0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:04:47.65 +36:54:29.7: ref_mag=12.55 +/- 0.01 new_mean_mag=12.5567 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:58:09.78 +38:26:18.7: ref_mag=12.88 +/- 0.02 new_mean_mag=12.6621 delta=0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:54:53.78 +36:29:51.4: ref_mag=12.63 +/- 0.01 new_mean_mag=12.4344 delta=0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:10:07.38 +41:39:47.8: ref_mag=12.97 +/- 0.02 new_mean_mag=12.9659 delta=0.01 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:09:45.40 +36:40:17.5: 12.50 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:08:51.53 +37:21:20.4: 12.45 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:02:37.14 +33:17:48.2: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter REJECTED candidate at 19:08:51.53 +37:21:20.4: ref_mag=12.47 +/- 0.01 new_mean_mag=12.5948 delta=-0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:02:37.14 +33:17:48.2: ref_mag=12.59 +/- 0.01 new_mean_mag=12.4396 delta=0.15 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:09:45.40 +36:40:17.5: 12.49 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry filter REJECTED candidate at 19:09:45.40 +36:40:17.5: ref_mag=12.49 +/- 0.01 new_mean_mag=12.6241 delta=-0.13 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:03:08.12 +35:32:54.3: 11.99 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:03:14.56 +41:24:05.4: 12.30 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:12:22.22 +39:57:16.5: 11.92 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:07:24.04 +33:50:52.8: 12.43 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:10:59.77 +37:03:27.9: 12.17 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:04:18.41 +38:26:58.2: 11.24 +/- 0.00 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:56:52.42 +36:42:43.5: 12.06 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:09:29.10 +37:35:55.8: 12.19 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:03:08.12 +35:32:54.3: 12.00 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:12:22.22 +39:57:16.5: 11.92 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:03:14.56 +41:24:05.4: 12.29 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:07:24.04 +33:50:52.8: 12.35 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:10:59.77 +37:03:27.9: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.00 +/- 0.01
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter REJECTED candidate at 19:03:08.12 +35:32:54.3: ref_mag=12.00 +/- 0.01 new_mean_mag=12.0274 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 12.38 +/- 0.01
Forced photometry filter REJECTED candidate at 18:12:22.22 +39:57:16.5: ref_mag=11.92 +/- 0.01 new_mean_mag=11.5541 delta=0.37 (need > 0.90)
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry filter REJECTED candidate at 19:03:14.56 +41:24:05.4: ref_mag=12.30 +/- 0.01 new_mean_mag=12.3776 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:07:24.04 +33:50:52.8: ref_mag=12.38 +/- 0.01 new_mean_mag=12.3740 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:10:59.77 +37:03:27.9: ref_mag=12.18 +/- 0.01 new_mean_mag=12.3456 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:04:18.41 +38:26:58.2: 11.25 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.25 +/- 0.00
Forced photometry filter REJECTED candidate at 18:04:18.41 +38:26:58.2: ref_mag=11.25 +/- 0.00 new_mean_mag=11.3929 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:56:52.42 +36:42:43.5: 12.07 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:09:29.10 +37:35:55.8: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter REJECTED candidate at 18:56:52.42 +36:42:43.5: ref_mag=12.07 +/- 0.01 new_mean_mag=12.0110 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter REJECTED candidate at 19:09:29.10 +37:35:55.8: ref_mag=12.20 +/- 0.01 new_mean_mag=12.3733 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:44:45.72 +32:43:00.3: 99.00 +/- 99.00 edge
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:54:43.83 +36:54:20.7: 11.80 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:49:41.54 +38:27:10.7: 11.65 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:08:22.42 +34:39:32.5: 12.45 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:54:37.23 +36:55:50.0: 12.51 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:44:45.72 +32:43:00.3: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 18:44:45.72 +32:43:00.3: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:54:43.83 +36:54:20.7: 11.80 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:49:41.54 +38:27:10.7: 11.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.80 +/- 0.01
Forced photometry reference-image weighted average: 11.63 +/- 0.01
Forced photometry filter REJECTED candidate at 18:54:43.83 +36:54:20.7: ref_mag=11.80 +/- 0.01 new_mean_mag=11.5933 delta=0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:49:41.54 +38:27:10.7: ref_mag=11.63 +/- 0.01 new_mean_mag=11.5739 delta=0.06 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:01:21.16 +42:23:42.2: 13.03 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:05:21.09 +34:18:39.4: 12.74 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:53:11.04 +41:01:13.3: 12.57 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:08:22.42 +34:39:32.5: 12.46 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.46 +/- 0.01
Forced photometry filter REJECTED candidate at 19:08:22.42 +34:39:32.5: ref_mag=12.46 +/- 0.01 new_mean_mag=12.2283 delta=0.23 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:54:37.23 +36:55:50.0: 12.48 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.02
Forced photometry filter REJECTED candidate at 18:54:37.23 +36:55:50.0: ref_mag=12.50 +/- 0.02 new_mean_mag=12.2757 delta=0.22 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:46:08.85 +32:42:39.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:53:11.04 +41:01:13.3: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter REJECTED candidate at 18:53:11.04 +41:01:13.3: ref_mag=12.59 +/- 0.01 new_mean_mag=12.4026 delta=0.19 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:01:21.16 +42:23:42.2: 12.97 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:05:21.09 +34:18:39.4: 12.78 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry reference-image weighted average: 12.76 +/- 0.02
Forced photometry filter REJECTED candidate at 19:01:21.16 +42:23:42.2: ref_mag=13.00 +/- 0.02 new_mean_mag=12.6067 delta=0.39 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:05:21.09 +34:18:39.4: ref_mag=12.76 +/- 0.02 new_mean_mag=12.5571 delta=0.20 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 19:08:09.88 +35:40:56.3: 12.53 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:54:15.45 +36:43:16.5: 12.97 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:46:08.85 +32:42:39.2: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 18:46:08.85 +32:42:39.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 19:08:09.88 +35:40:56.3: 12.57 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter REJECTED candidate at 19:08:09.88 +35:40:56.3: ref_mag=12.55 +/- 0.01 new_mean_mag=12.6074 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:54:15.45 +36:43:16.5: 12.99 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry filter REJECTED candidate at 18:54:15.45 +36:43:16.5: ref_mag=12.98 +/- 0.02 new_mean_mag=12.4614 delta=0.52 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:42:53.29 +36:58:54.2: 12.43 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:58:15.11 +39:38:29.3: 12.90 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:37:51.87 +39:39:45.6: 12.83 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:48:36.33 +33:46:55.8: 12.70 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:44:13.68 +38:32:55.0: 13.13 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:44:36.05 +37:35:17.9: 13.22 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:42:53.29 +36:58:54.2: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.45 +/- 0.01
Forced photometry filter REJECTED candidate at 18:42:53.29 +36:58:54.2: ref_mag=12.45 +/- 0.01 new_mean_mag=12.4302 delta=0.02 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:37:51.87 +39:39:45.6: 12.80 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:58:15.11 +39:38:29.3: 12.89 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.81 +/- 0.02
Forced photometry filter REJECTED candidate at 18:37:51.87 +39:39:45.6: ref_mag=12.81 +/- 0.02 new_mean_mag=12.8330 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:08:56.60 +42:42:17.8: 13.13 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:44:13.68 +38:32:55.0: 13.13 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 18:58:15.11 +39:38:29.3: ref_mag=12.89 +/- 0.02 new_mean_mag=12.7815 delta=0.11 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:48:36.33 +33:46:55.8: 12.73 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter REJECTED candidate at 18:44:13.68 +38:32:55.0: ref_mag=13.13 +/- 0.02 new_mean_mag=12.8373 delta=0.29 (need > 0.90)
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Forced photometry filter REJECTED candidate at 18:48:36.33 +33:46:55.8: ref_mag=12.71 +/- 0.02 new_mean_mag=12.5864 delta=0.13 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:44:36.05 +37:35:17.9: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Forced photometry filter REJECTED candidate at 18:44:36.05 +37:35:17.9: ref_mag=13.19 +/- 0.03 new_mean_mag=12.9274 delta=0.27 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:10:33.33 +41:37:58.9: 13.13 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:08:56.60 +42:42:17.8: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter KEPT candidate at 18:08:56.60 +42:42:17.8: ref_mag=13.13 +/- 0.02 new_mean_mag=12.1567 delta=0.97 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:11:01.93 +41:27:33.3: 13.55 +/- 0.04 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:10:33.33 +41:37:58.9: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.02
Forced photometry filter KEPT candidate at 18:10:33.33 +41:37:58.9: ref_mag=13.10 +/- 0.02 new_mean_mag=12.1875 delta=0.91 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:11:01.93 +41:27:33.3: 13.58 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter KEPT candidate at 18:11:01.93 +41:27:33.3: ref_mag=13.56 +/- 0.03 new_mean_mag=12.4342 delta=1.13 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:12:18.00 +41:28:28.5: 13.27 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:12:55.59 +41:29:43.4: 13.32 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:11:47.01 +40:28:54.2: 13.20 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:10:15.25 +42:26:51.5: 13.20 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:11:30.33 +42:21:03.2: 13.18 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:08:30.47 +42:28:34.3: 13.15 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:12:18.00 +41:28:28.5: 13.27 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.02
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:11:47.01 +40:28:54.2: 13.24 +/- 0.03 detection
Forced photometry filter KEPT candidate at 18:12:18.00 +41:28:28.5: ref_mag=13.27 +/- 0.02 new_mean_mag=12.3143 delta=0.95 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:12:55.59 +41:29:43.4: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter KEPT candidate at 18:11:47.01 +40:28:54.2: ref_mag=13.22 +/- 0.02 new_mean_mag=12.2140 delta=1.00 (need > 0.90)
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 18:12:55.59 +41:29:43.4: ref_mag=13.32 +/- 0.02 new_mean_mag=12.3602 delta=0.96 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:10:15.25 +42:26:51.5: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter KEPT candidate at 18:10:15.25 +42:26:51.5: ref_mag=13.16 +/- 0.02 new_mean_mag=12.2223 delta=0.93 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:11:30.33 +42:21:03.2: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 18:11:30.33 +42:21:03.2: ref_mag=13.15 +/- 0.02 new_mean_mag=12.1979 delta=0.95 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:08:30.47 +42:28:34.3: 13.16 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter KEPT candidate at 18:08:30.47 +42:28:34.3: ref_mag=13.15 +/- 0.02 new_mean_mag=12.2032 delta=0.95 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:09:30.99 +42:21:15.5: 13.04 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:09:30.99 +42:21:15.5: 13.02 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry filter KEPT candidate at 18:09:30.99 +42:21:15.5: ref_mag=13.03 +/- 0.02 new_mean_mag=12.0699 delta=0.96 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:09:11.11 +42:19:11.7: 13.02 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:09:11.11 +42:19:11.7: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.04 +/- 0.02
Forced photometry filter KEPT candidate at 18:09:11.11 +42:19:11.7: ref_mag=13.04 +/- 0.02 new_mean_mag=12.1269 delta=0.91 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:12:04.08 +39:58:56.6: 13.01 +/- 0.03 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:12:04.08 +39:58:56.6: 12.96 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter KEPT candidate at 18:12:04.08 +39:58:56.6: ref_mag=12.99 +/- 0.02 new_mean_mag=12.0409 delta=0.95 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:11:51.11 +41:52:45.1: 12.92 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:10:32.84 +40:38:49.4: 12.77 +/- 0.02 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:11:51.11 +41:52:45.1: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.02
Forced photometry filter KEPT candidate at 18:11:51.11 +41:52:45.1: ref_mag=12.93 +/- 0.02 new_mean_mag=11.9366 delta=1.00 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:10:32.84 +40:38:49.4: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter KEPT candidate at 18:10:32.84 +40:38:49.4: ref_mag=12.76 +/- 0.01 new_mean_mag=11.8046 delta=0.95 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:10:27.91 +42:39:23.2: 11.95 +/- 0.01 detection
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:10:27.91 +42:39:23.2: 11.92 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.93 +/- 0.01
Forced photometry filter KEPT candidate at 18:10:27.91 +42:39:23.2: ref_mag=11.93 +/- 0.01 new_mean_mag=10.9665 delta=0.97 (need > 0.90)
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-29-18_20.00sec_-0.00C_LIGHT_0299.fits at 18:07:59.20 +42:13:19.8: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Lyr-02-Q1b1x1_2026-05-16_04-30-03_20.00sec_0.00C_LIGHT_0300.fits at 18:07:59.20 +42:13:19.8: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 18:07:59.20 +42:13:19.8: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Adding exclusion_list_local.txt__out106452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154710.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 359s
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: 6s
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Considering the candidate 180047_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180047_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:21:52.17 +42:16:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180048_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180048_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180052_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180052_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:11:04.14 +42:03:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180056_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180056_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180057_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180057_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180062_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180062_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180064_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180064_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180066_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180066_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:06:29.29 +37:49:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180067_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180067_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180068_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180068_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180069_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180069_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180072_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180072_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:17:17.11 +34:41:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180074_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180074_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180075_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180075_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180076_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180076_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180078_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180078_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180079_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180079_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180080_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180080_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:07:11.44 +35:48:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180082_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180082_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180084_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180084_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180085_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180085_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180086_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180086_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180087_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180087_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:53:01.77 +33:07:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180090_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180090_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180091_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180091_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:13:19.84 +40:31:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180093_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180093_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:08:45.37 +36:23:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180094_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180094_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:06:21.05 +41:35:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180096_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180096_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:06:16.79 +33:12:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180097_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180097_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:56:03.36 +33:47:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180101_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180101_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:44:48.11 +37:35:41.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 180207_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180207_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 17:54:59.13 +33:56:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180293_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180293_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180393_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180393_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:54:10.05 +32:49:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180470_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180470_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:03:12.62 +33:58:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180492_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180492_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180516_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180516_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180539_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180539_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:56:00.50 +39:29:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180604_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180604_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:07:18.38 +36:04:41.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 180704_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180704_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180726_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180726_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:11:28.56 +40:25:44.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 180736_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180736_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:57:08.28 +32:54:20.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 180830_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180830_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:51:35.97 +36:33:49.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 180831_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180831_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180877_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180877_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:08:10.55 +36:23:02.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 180921_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180921_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180933_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180933_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180936_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180936_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 180941_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 180941_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:44:22.74 +39:38:18.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181004_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181004_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 181039_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181039_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:38:16.51 +39:42:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181041_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181041_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 181048_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181048_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:04:46.45 +38:43:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181053_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181053_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 181079_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181079_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:02:52.38 +38:30:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181085_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181085_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:11:13.58 +40:25:18.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181106_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181106_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:53:43.60 +40:18:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181123_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181123_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:37:58.34 +39:41:09.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181159_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181159_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:12:59.53 +38:45:03.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181223_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181223_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 181243_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181243_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 181474_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181474_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 181513_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181513_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 181521_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181521_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 181561_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 181561_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 154710_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 154710_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 114559_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 114559_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 117553_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 117553_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 126432_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 126432_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:51:26.16 +40:54:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69646_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 69646_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
Rejecting candidate due to large distance (41.9") between the two second-epoch detections
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Considering the candidate 117042_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 117042_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 117373_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 117373_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 77309_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 77309_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:30:13.34 +37:29:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133116_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 133116_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 109069_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 109069_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 110412_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 110412_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 108400_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 108400_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 114937_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 114937_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 17:58:09.23 +41:25:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128873_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 128873_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:43:26.03 +40:50:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110061_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 110061_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 110414_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 110414_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 139675_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 139675_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 111621_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 111621_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 130415_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 130415_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 150091_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 150091_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:05:47.25 +39:09:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155141_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 155141_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:37:14.66 +42:49:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58883_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 58883_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:45:32.09 +36:18:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03313_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 03313_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:40:25.69 +32:54:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106452_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
Preparing report for the candidate 106452_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
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Considering the candidate 31971_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 31971_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:44:52.09 +34:40:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146398_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 146398_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 19:05:33.78 +39:20:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111142_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 111142_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
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Considering the candidate 11802_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 11802_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:12:11.10 +33:17:29.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 88473_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 88473_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:36:56.78 +38:47:09.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 74705_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 74705_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:44:46.21 +37:36:20.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 147526_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 147526_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:24:13.91 +39:30:25.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54863_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 54863_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:19:51.82 +36:03:55.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 65952_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 65952_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:54:29.95 +36:53:55.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 14207_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 14207_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:01:35.94 +33:18:40.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 13024_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 13024_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:36:37.31 +33:28:09.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 14069_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 14069_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:11:45.15 +33:26:49.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 13073_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 13073_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:00:36.35 +33:12:47.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 62475_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 62475_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:09:59.07 +36:27:58.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129148_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 129148_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:15:38.84 +42:09:32.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 62001_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 62001_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 18:08:02.11 +36:23:59.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 135031_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 135031_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 17:53:18.14 +40:00:29.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75378_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 75378_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
**** FOUND 17:56:15.31 +37:15:02.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 12284_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101
The candidate 12284_fd_Lyr-02-Q1b1x1_2026-08-22_04-00-20_20.00sec_-0.00C_LIGHTs_0101 did not pass the final checks
