This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8
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 07 08.4518 2461229.9518 12.93 20:36:25.19 +06:54:03.9
51.96227 -19.62900 galactic Del Second-epoch detections are separated by 2.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.273 Atropos -1 1 1 13.2 -0 0
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:36:25.19 +06:54:03.9: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:36:25.19 +06:54:03.9: 15.53 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 08.4518* 20 36 25.19 +06 54 03.9 12.9 U Del 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
VARIABLE_NAME,2461229.9518,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260708.4518 12.93CV 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 07 08.4518 2461229.9518 13.16 20:47:40.46 +05:00:16.1
51.83970 -23.00756 galactic Del Second-epoch detections are separated by 1.5" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.456 Abnoba -0 1 1 12.9 -0 -0
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:47:40.46 +05:00:16.1: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:47:40.46 +05:00:16.1: 15.55 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 08.4518* 20 47 40.46 +05 00 16.1 13.2 U Del 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
VARIABLE_NAME,2461229.9518,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260708.4518 13.16CV 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 07 08.4518 2461229.9518 12.22 20:16:42.34 +07:39:00.7
49.95958 -15.06721 galactic Aql Second-epoch detections are separated by 1.4" and 5.4 pix
The object was found in VSX 3" ASAS J201642+0739.0
Type: MISC
# Max. Min./Amp. JD0 Period
13.230 V Y 0.380 V 2452407.90000 63.737850000000
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:16:42.34 +07:39:00.7: 13.19 +/- 0.04 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:16:42.34 +07:39:00.7: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J201642+0739.0,2461229.9518,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J201642+0739.0 20260708.4518 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 07 08.4518 2461229.9518 11.60 20:20:02.35 +08:22:56.5
51.05075 -15.39677 galactic Aql Second-epoch detections are separated by 1.8" and 5.5 pix
The object was found in VSX 4" ASAS J202002+0823.0
Type: MISC
# Max. Min./Amp. JD0 Period
8.770 Ic Y 0.362 Ic 2452719.50000 173.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:20:02.35 +08:22:56.5: 12.59 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:20:02.35 +08:22:56.5: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J202002+0823.0,2461229.9518,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J202002+0823.0 20260708.4518 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 08.4518 2461229.9518 11.55 20:18:38.25 +02:16:19.4
45.36175 -18.19032 galactic Aql Second-epoch detections are separated by 0.7" and 5.1 pix
The object was found in VSX 4" V1284 Aql
Type: SRB
# Max. Min./Amp. JD0 Period
12.600 V 14.000 V 2452393.90000 163.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:18:38.25 +02:16:19.4: 12.52 +/- 0.03 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:18:38.25 +02:16:19.4: 12.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1284 Aql,2461229.9518,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1284 Aql 20260708.4518 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 08.4518 2461229.9518 12.21 20:19:58.21 +09:15:14.5
51.81291 -14.92884 galactic Del Second-epoch detections are separated by 1.0" and 5.4 pix
The object was found in VSX 4" NSVS J2019584+091515
Type: SR
# Max. Min./Amp. JD0 Period
14.701 g Y 0.409 g 2458367.98250 74.335129100000
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:19:58.21 +09:15:14.5: 13.16 +/- 0.05 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:19:58.21 +09:15:14.5: 13.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 08.4518* 20 19 58.21 +09 15 14.5 12.2 U Del 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
NSVS J2019584+091515,2461229.9518,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2019584+091515 20260708.4518 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 07 08.4518 2461229.9518 12.18 20:18:25.05 +07:40:43.7
50.21078 -15.41645 galactic Aql Second-epoch detections are separated by 0.9" and 5.1 pix
The object was found in VSX 2" ASASSN-V J201824.90+074043.7
Type: SR
# Max. Min./Amp. JD0 Period
13.490 V 14.270 V 2458357.29790 93.017010200000
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:18:25.05 +07:40:43.7: 13.31 +/- 0.05 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:18:25.05 +07:40:43.7: 13.27 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201824.90+074043.7,2461229.9518,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201824.90+074043.7 20260708.4518 12.18CV 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 07 08.4518 2461229.9518 11.06 20:24:18.44 +07:34:15.2
50.90040 -16.72125 galactic Del Second-epoch detections are separated by 0.9" and 5.4 pix
The object was found in VSX 3" ASAS J202418+0734.3
Type: MISC
# Max. Min./Amp. JD0 Period
11.910 V Y 0.400 V 2452366.30000 71.341942000000
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:24:18.44 +07:34:15.2: 11.99 +/- 0.01 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:24:18.44 +07:34:15.2: 12.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.01 +/- 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 07 08.4518* 20 24 18.44 +07 34 15.2 11.1 U Del 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
ASAS J202418+0734.3,2461229.9518,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J202418+0734.3 20260708.4518 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 08.4518 2461229.9518 12.15 20:19:38.16 +04:35:49.4
47.60783 -17.24676 galactic Aql Second-epoch detections are separated by 1.2" and 5.4 pix
The object was found in VSX 3" ATO J304.9083+04.5968
Type: SRB
# Max. Min./Amp. JD0 Period
12.940 V 13.670 V 2458333.83200 50.580000000000
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:19:38.16 +04:35:49.4: 13.10 +/- 0.04 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:19:38.16 +04:35:49.4: 13.12 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.9083+04.5968,2461229.9518,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.9083+04.5968 20260708.4518 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 08.4518 2461229.9518 12.19 20:49:58.01 +03:19:28.9
50.61703 -24.38415 galactic Del Second-epoch detections are separated by 1.1" and 5.1 pix
The object was found in VSX 1" NSVS J2049581+031916
Type: SR
# Max. Min./Amp. JD0 Period
13.717 g Y 1.107 g 2458345.01150 183.734579600000
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:49:58.01 +03:19:28.9: 13.25 +/- 0.05 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:49:58.01 +03:19:28.9: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 07 08.4518* 20 49 58.01 +03 19 28.9 12.2 U Del 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
NSVS J2049581+031916,2461229.9518,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2049581+031916 20260708.4518 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 07 08.4518 2461229.9518 12.40 20:17:32.52 +03:49:08.8
46.62911 -17.18518 galactic Aql Second-epoch detections are separated by 1.0" and 5.4 pix
The object was found in VSX 3" ASASSN-V J201732.34+034908.2
Type: SR
# Max. Min./Amp. JD0 Period
13.230 V 13.830 V 2458247.79730 54.600799300000
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:17:32.52 +03:49:08.8: 13.28 +/- 0.05 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:17:32.52 +03:49:08.8: 13.39 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201732.34+034908.2,2461229.9518,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J201732.34+034908.2 20260708.4518 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 07 08.4518 2461229.9518 8.95 20:23:15.09 +07:57:21.8
51.10149 -16.29747 galactic Aql Second-epoch detections are separated by 0.2" and 5.3 pix
The object was found in VSX 3" ASAS J202315+0757.4
Type: MISC
# Max. Min./Amp. JD0 Period
10.420 V Y 0.590 V 2452379.20000 110.708389000000 M7
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:23:15.09 +07:57:21.8: 9.93 +/- 0.00 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:23:15.09 +07:57:21.8: 9.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.95 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J202315+0757.4,2461229.9518,8.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J202315+0757.4 20260708.4518 8.95CV 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 07 08.4518 2461229.9518 11.34 20:40:34.80 +09:28:59.8
54.85588 -19.10432 galactic Del Second-epoch detections are separated by 0.5" and 5.3 pix
The object was found in VSX 2" ASAS J204035+0929.1
Type: MISC
# Max. Min./Amp. JD0 Period
12.610 V Y 0.430 V 2452697.70000 146.663483000000 M6/7
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:40:34.80 +09:28:59.8: 12.37 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:40:34.80 +09:28:59.8: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 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 07 08.4518* 20 40 34.80 +09 28 59.8 11.3 U Del 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
ASAS J204035+0929.1,2461229.9518,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J204035+0929.1 20260708.4518 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 08.4518 2461229.9518 12.20 20:24:32.92 +06:12:24.6
49.71182 -17.47867 galactic Del Second-epoch detections are separated by 1.2" and 5.4 pix
The object was found in VSX 3" ASAS J202433+0612.4
Type: MISC
# Max. Min./Amp. JD0 Period
9.330 Ic Y 0.857 Ic 2453146.80000 274.800000000000
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:24:32.92 +06:12:24.6: 13.22 +/- 0.04 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:24:32.92 +06:12:24.6: 13.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 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 07 08.4518* 20 24 32.92 +06 12 24.6 12.2 U Del 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
ASAS J202433+0612.4,2461229.9518,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J202433+0612.4 20260708.4518 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 07 08.4518 2461229.9518 12.06 20:16:20.44 +06:15:35.8
48.67136 -15.69831 galactic Aql Second-epoch detections are separated by 0.7" and 5.2 pix
The object was found in VSX 3" ASAS J201620+0615.6
Type: MISC
# Max. Min./Amp. JD0 Period
12.930 V Y 0.480 V 2452429.10000 71.341217000000
The object was not found in astcheck.
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:16:20.44 +06:15:35.8: 13.21 +/- 0.05 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:16:20.44 +06:15:35.8: 13.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J201620+0615.6,2461229.9518,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J201620+0615.6 20260708.4518 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 08.4518 2461229.9518 12.13 20:52:05.37 +04:24:04.2
51.92641 -24.25968 galactic Del Second-epoch detections are separated by 0.7" and 5.1 pix
The object was found in VSX10" Gaia DR3 1734740284448059648
Type: ROT
# Max. Min./Amp. JD0 Period
13.630 G 13.670 G K
The object was found in astcheck.397 Vienna -2 0 2 12.6 0 0
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:52:05.37 +04:24:04.2: 13.49 +/- 0.06 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:52:05.37 +04:24:04.2: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 08.4518* 20 52 05.37 +04 24 04.2 12.1 U Del 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 1734740284448059648,2461229.9518,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1734740284448059648 20260708.4518 12.13CV 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: 2461171.87501223 11.05.2026 08:59:51.057 /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
First image: 2461171.87501223 11.05.2026 08:59:51.057 /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
Last image: 2461229.95206287 08.07.2026 10:50:48.232 /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.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.: -7.84
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: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 12867
Objects passed selection criteria: 12798
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: 8351
Average stars matched: 7858.5 (94.1025 %)
Memory usage VmPeak: 118160 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 7 15:05:04 CDT 2026
VaST build number 1.0rc89-138-g473912fb
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 8 05:58:04 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: 2461171.87501223 11.05.2026 08:59:51.057 /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
First image: 2461171.87501223 11.05.2026 08:59:51.057 /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
Last image: 2461229.95206287 08.07.2026 10:50:48.232 /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 54
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
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: 32 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 98532
Objects passed selection criteria: 98210
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: 65639.5
Average stars matched: 61013 (92.9517 %)
Memory usage VmPeak: 1867268 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 7 15:05:04 CDT 2026
VaST build number 1.0rc89-138-g473912fb
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-07)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jul 8 06:01:40 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
SExtractor catalog cache: saved Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.cat to cache
SExtractor catalog cache: saved Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.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/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.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: 2461229.95159799
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits exists and is non-empty
Saving wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits to local_wcs_cache/
'wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits' -> 'local_wcs_cache/wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits'
wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits exists and is non-empty
Saving wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits to local_wcs_cache/
'wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits' -> 'local_wcs_cache/wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits'
wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits exists and is non-empty
Saving wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits to local_wcs_cache/
'wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits' -> 'local_wcs_cache/wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits'
wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits exists and is non-empty
Saving wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits to local_wcs_cache/
'wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits' -> 'local_wcs_cache/wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits (1st reference image)
verification OK: wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
Image size: 937.8'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 20:34:08.839 +05:59:25.58 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits (1st new image)
verification OK: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 20:34:16.780 +05:59:56.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:34:08.839 +05:59:25.58
Second-epoch image center 20:34:16.780 +05:59:56.85
Angular distance between the image centers 0.0340 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits (2nd new image)
verification OK: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 20:34:14.713 +06:00:01.63 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:34:08.839 +05:59:25.58
Second-epoch image center 20:34:14.713 +06:00:01.63
Angular distance between the image centers 0.0263 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 20:34:16.780 +05:59:56.85
Second-epoch second image center 20:34:14.713 +06:00:01.63
Angular distance between the image centers 0.00867 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/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits &> /tmp/tmp.l3MwXKqACO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits &> /tmp/tmp.3KVW0nEvbW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits &> /tmp/tmp.APqWJzKA2a
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits &> /tmp/tmp.oaBjWowq3H
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
Calibrating the magnitude scale
Found non-empty wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.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_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits and wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.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_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits and wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat
Found non-empty wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits and wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat
The reference image (wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits) and catalog (wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat) found
'wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat' -> 'wcsmag.cat'
Read 15482 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.5401 to 316.4412 deg, Dec +0.6725 to +11.2631 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 300.5401 to 316.4412 deg, Dec 0.6725 to 11.2631 deg
Loaded 14055 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): 10386 out of 10899 total matches.
Matched with Tycho-2 10899 out of 15482 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.526300
a=0.000000 b=1.000000 c=22.526300
From vast_summary.log: estimated ref. image limiting mag.: -7.84
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.69
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.69
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 15482 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.5401 to 316.4412 deg, Dec +0.6725 to +11.2631 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 300.5401 to 316.4412 deg, Dec 0.6725 to 11.2631 deg
Loaded 14055 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): 10386 out of 10899 total matches.
Matched with Tycho-2 10899 out of 15482 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits:
Forced-photometry filter: calibrated wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits -> calib.txt_param_ref_wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits (aperture=6.7)
Read 15515 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.5401 to 316.4504 deg, Dec +0.6664 to +11.2601 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 300.5401 to 316.4504 deg, Dec 0.6664 to 11.2601 deg
Loaded 14063 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): 10350 out of 10865 total matches.
Matched with Tycho-2 10865 out of 15515 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits:
Forced-photometry filter: calibrated wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits -> calib.txt_param_ref_wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.5 pix Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
2.5 pix Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
2.9 pix fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
3.0 pix fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
2.5 pix wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
2.5 pix wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
Limiting magnitude estimates:
14.7 mag. Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
14.7 mag. Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
13.5 mag. fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
13.4 mag. fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 10.8 (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
############ /tmp/tmp.l3MwXKqACO (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits' -> 'wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
WCS_IMAGE_NAME=wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
WCS-calibrated image found: wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
Checking if the catalog wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat corresponding to the image wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits alredy exist and is non-empty...
Catalog wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat corresponding to the image wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
WCS catalog name: wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1114, bad_region=2741, passed=15482
Got 15482 stars (including 11752 good ones) from the SExtractor catalog wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat
util/solve_plate_with_UCAC5 got 15482 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 12917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 12916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 12916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits N_match=958 sigma_overall_arcsec=0.467 sigma_q1_arcsec=0.435 sigma_q2_arcsec=0.434 sigma_q3_arcsec=0.556 sigma_q4_arcsec=0.429 n_q1=308 n_q2=170 n_q3=303 n_q4=177 worst_quadrant_to_overall_ratio=1.190
The image catalog is written to wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits -region wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.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.3KVW0nEvbW (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits' -> 'wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
WCS_IMAGE_NAME=wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
WCS-calibrated image found: wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
Checking if the catalog wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat corresponding to the image wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits alredy exist and is non-empty...
Catalog wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat corresponding to the image wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
WCS catalog name: wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1130, bad_region=2771, passed=15511
Got 15511 stars (including 11747 good ones) from the SExtractor catalog wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat
util/solve_plate_with_UCAC5 got 15511 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 12891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 12890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 12890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits N_match=956 sigma_overall_arcsec=0.494 sigma_q1_arcsec=0.496 sigma_q2_arcsec=0.489 sigma_q3_arcsec=0.566 sigma_q4_arcsec=0.402 n_q1=303 n_q2=171 n_q3=305 n_q4=177 worst_quadrant_to_overall_ratio=1.146
The image catalog is written to wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits -region wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.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.APqWJzKA2a (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_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.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_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
Checking if the catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
WCS catalog name: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=474, bad_region=1062, passed=5206
Got 5206 stars (including 3871 good ones) from the SExtractor catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat
util/solve_plate_with_UCAC5 got 5206 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 4215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 4216 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 4216 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 954 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits N_match=954 sigma_overall_arcsec=0.513 sigma_q1_arcsec=0.391 sigma_q2_arcsec=0.579 sigma_q3_arcsec=0.524 sigma_q4_arcsec=0.799 n_q1=326 n_q2=180 n_q3=274 n_q4=174 worst_quadrant_to_overall_ratio=1.557
The image catalog is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits -region wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.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.oaBjWowq3H (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_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.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_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
WCS_IMAGE_NAME=wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
WCS-calibrated image found: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
Checking if the catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat corresponding to the image wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits alredy exist and is non-empty...
Catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat corresponding to the image wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
WCS catalog name: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=420, bad_region=1004, passed=5000
Got 5000 stars (including 3738 good ones) from the SExtractor catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat
util/solve_plate_with_UCAC5 got 5000 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 4059 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 4058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 4058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 953 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits N_match=953 sigma_overall_arcsec=0.500 sigma_q1_arcsec=0.385 sigma_q2_arcsec=0.633 sigma_q3_arcsec=0.491 sigma_q4_arcsec=0.755 n_q1=328 n_q2=182 n_q3=274 n_q4=169 worst_quadrant_to_overall_ratio=1.511
The image catalog is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits -region wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits sigma_overall=0.467 worst_q_ratio=1.190
ref2=Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits sigma_overall=0.494 worst_q_ratio=1.146
new1=fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits sigma_overall=0.513 worst_q_ratio=1.557
new2=fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits sigma_overall=0.500 worst_q_ratio=1.511
reference average sigma_overall=0.4805 worst_q_ratio=1.168
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435_astrometric_residuals.png (958 matched stars from wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436_astrometric_residuals.png (956 matched stars from wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342_astrometric_residuals.png (954 matched stars from wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343_astrometric_residuals.png (953 matched stars from wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits'
Saving fully-calibrated image wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits'
Preparing the HTML report for the field Del-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21251_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 21251_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:21:26.92 +09:34:20.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21472_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 21472_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:34:14.24 +06:34:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11422_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 11422_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:32:44.07 +08:49:09.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Del-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
SExtractor catalog cache: saved Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.cat to cache
SExtractor catalog cache: saved Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
Creating symlink local_wcs_cache/wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
Creating symlink local_wcs_cache/wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
Creating symlink local_wcs_cache/wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits exists and is non-empty
wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits exists and is non-empty
wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits exists and is non-empty
wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits (1st reference image)
verification OK: wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
Image size: 937.8'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 20:34:08.839 +05:59:25.58 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits (1st new image)
verification OK: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 20:34:16.780 +05:59:56.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:34:08.839 +05:59:25.58
Second-epoch image center 20:34:16.780 +05:59:56.85
Angular distance between the image centers 0.0340 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits (2nd new image)
verification OK: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 20:34:14.713 +06:00:01.63 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:34:08.839 +05:59:25.58
Second-epoch image center 20:34:14.713 +06:00:01.63
Angular distance between the image centers 0.0263 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 20:34:16.780 +05:59:56.85
Second-epoch second image center 20:34:14.713 +06:00:01.63
Angular distance between the image centers 0.00867 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/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits &> /tmp/tmp.WUY6lwmvQ9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits &> /tmp/tmp.UnUzp6s88G
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits &> /tmp/tmp.tLUEZMbs7L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits &> /tmp/tmp.L4ePfztXLI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
Calibrating the magnitude scale
Found non-empty wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.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_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits and wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.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_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits and wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat
Found non-empty wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits and wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat
The reference image (wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits) and catalog (wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat) found
'wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat' -> 'wcsmag.cat'
Read 118300 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.5393 to 316.4572 deg, Dec +0.6692 to +11.2661 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 300.5393 to 316.4572 deg, Dec 0.6692 to 11.2661 deg
Loaded 14078 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): 10115 out of 12436 total matches.
Matched with Tycho-2 12436 out of 118300 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.336000
a=0.000000 b=1.000000 c=22.336000
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 118300 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.5393 to 316.4572 deg, Dec +0.6692 to +11.2661 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 300.5393 to 316.4572 deg, Dec 0.6692 to 11.2661 deg
Loaded 14078 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): 10115 out of 12436 total matches.
Matched with Tycho-2 12436 out of 118300 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits:
Forced-photometry filter: calibrated wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits -> calib.txt_param_ref_wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits (aperture=4.8)
Read 119802 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.5393 to 316.4577 deg, Dec +0.6630 to +11.2602 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 300.5393 to 316.4577 deg, Dec 0.6630 to 11.2602 deg
Loaded 14077 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): 10058 out of 12409 total matches.
Matched with Tycho-2 12409 out of 119802 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits:
Forced-photometry filter: calibrated wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits -> calib.txt_param_ref_wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
2.1 pix Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
2.7 pix fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
2.8 pix fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
2.2 pix wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
2.1 pix wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
Limiting magnitude estimates:
14.9 mag. Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
14.9 mag. Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
13.6 mag. fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
13.5 mag. fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 12.9 (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.WUY6lwmvQ9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits' -> 'wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
WCS_IMAGE_NAME=wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
WCS-calibrated image found: wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
Checking if the catalog wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat corresponding to the image wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits alredy exist and is non-empty...
Catalog wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat corresponding to the image wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits
WCS catalog name: wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=62, blended=11186, bad_region=16229, passed=118238
Got 118238 stars (including 91754 good ones) from the SExtractor catalog wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat
util/solve_plate_with_UCAC5 got 118238 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 103454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 103453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 103453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits N_match=961 sigma_overall_arcsec=0.475 sigma_q1_arcsec=0.421 sigma_q2_arcsec=0.438 sigma_q3_arcsec=0.587 sigma_q4_arcsec=0.469 n_q1=313 n_q2=183 n_q3=280 n_q4=185 worst_quadrant_to_overall_ratio=1.235
The image catalog is written to wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits -region wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.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.UnUzp6s88G (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits' -> 'wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
WCS_IMAGE_NAME=wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
WCS-calibrated image found: wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
Checking if the catalog wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat corresponding to the image wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits alredy exist and is non-empty...
Catalog wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat corresponding to the image wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits
WCS catalog name: wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=11329, bad_region=16611, passed=119743
Got 119743 stars (including 92777 good ones) from the SExtractor catalog wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat
util/solve_plate_with_UCAC5 got 119743 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 105132 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 105133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 105133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits N_match=960 sigma_overall_arcsec=0.504 sigma_q1_arcsec=0.494 sigma_q2_arcsec=0.478 sigma_q3_arcsec=0.564 sigma_q4_arcsec=0.465 n_q1=305 n_q2=188 n_q3=278 n_q4=189 worst_quadrant_to_overall_ratio=1.121
The image catalog is written to wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits -region wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.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.tLUEZMbs7L (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_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.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_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
Checking if the catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat corresponding to the image wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
WCS catalog name: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=1, blended=2818, bad_region=5994, passed=36696
Got 36696 stars (including 29459 good ones) from the SExtractor catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat
util/solve_plate_with_UCAC5 got 36696 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 31015 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 31014 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 31015 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 951 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits N_match=951 sigma_overall_arcsec=0.511 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.625 sigma_q3_arcsec=0.528 sigma_q4_arcsec=0.711 n_q1=333 n_q2=176 n_q3=279 n_q4=163 worst_quadrant_to_overall_ratio=1.391
The image catalog is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits -region wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.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.L4ePfztXLI (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_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.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_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
WCS_IMAGE_NAME=wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
WCS-calibrated image found: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
Checking if the catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat corresponding to the image wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits alredy exist and is non-empty...
Catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat corresponding to the image wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
WCS catalog name: wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=2, blended=2505, bad_region=5657, passed=34665
Got 34665 stars (including 27865 good ones) from the SExtractor catalog wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat
util/solve_plate_with_UCAC5 got 34665 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 29377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 29376 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 29377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits N_match=950 sigma_overall_arcsec=0.506 sigma_q1_arcsec=0.419 sigma_q2_arcsec=0.608 sigma_q3_arcsec=0.517 sigma_q4_arcsec=0.696 n_q1=334 n_q2=176 n_q3=279 n_q4=161 worst_quadrant_to_overall_ratio=1.376
The image catalog is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits -region wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.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_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.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_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-08_20.00sec_5.00C_LIGHT_0342.fits
Saving fully-calibrated image wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.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_2026-07-08_CI_Del-02-Q2b1x1_055434_TTUQ2b1x1_4136661_Ttaherk8/wcs_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343.fits
Preparing the HTML report for the field Del-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:27:03.99 +07:23:34.0: 12.18 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:17:04.80 +07:02:38.2: 11.98 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:24:29.73 +05:29:01.9: 12.23 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:17:04.80 +07:02:38.2: 12.01 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.99 +/- 0.01
Forced photometry filter REJECTED candidate at 20:17:04.80 +07:02:38.2: ref_mag=11.99 +/- 0.01 new_mean_mag=11.9230 delta=0.07 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:27:03.99 +07:23:34.0: 12.19 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:24:29.73 +05:29:01.9: 12.22 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter REJECTED candidate at 20:27:03.99 +07:23:34.0: ref_mag=12.18 +/- 0.01 new_mean_mag=12.5279 delta=-0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 20:24:29.73 +05:29:01.9: ref_mag=12.23 +/- 0.01 new_mean_mag=12.2295 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:22:55.68 +03:31:43.8: 12.24 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:25:23.10 +06:39:28.0: 12.28 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:36:59.97 +06:15:52.9: 12.84 +/- 0.04 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:23:21.65 +05:21:00.1: 12.26 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:22:55.68 +03:31:43.8: 12.25 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.24 +/- 0.01
Forced photometry filter REJECTED candidate at 20:22:55.68 +03:31:43.8: ref_mag=12.24 +/- 0.01 new_mean_mag=12.3335 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:36:59.97 +06:15:52.9: 12.87 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.85 +/- 0.03
Forced photometry filter REJECTED candidate at 20:36:59.97 +06:15:52.9: ref_mag=12.85 +/- 0.03 new_mean_mag=12.7388 delta=0.11 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:25:23.10 +06:39:28.0: 12.32 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.30 +/- 0.02
Forced photometry filter REJECTED candidate at 20:25:23.10 +06:39:28.0: ref_mag=12.30 +/- 0.02 new_mean_mag=12.2848 delta=0.01 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:23:21.65 +05:21:00.1: 12.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.02
Forced photometry filter REJECTED candidate at 20:23:21.65 +05:21:00.1: ref_mag=12.28 +/- 0.02 new_mean_mag=12.3145 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:47:54.40 +09:12:10.8: 13.09 +/- 0.04 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:47:40.46 +05:00:16.1: 15.51 +/- 99.00 upperlimit
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:36:25.19 +06:54:03.9: 15.54 +/- 99.00 upperlimit
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:29:40.83 +03:00:34.7: 12.80 +/- 0.03 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:47:54.40 +09:12:10.8: 13.14 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:36:25.19 +06:54:03.9: 15.53 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 20:47:54.40 +09:12:10.8: ref_mag=13.11 +/- 0.03 new_mean_mag=13.0570 delta=0.05 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:47:40.46 +05:00:16.1: 15.55 +/- 99.00 upperlimit
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:29:40.83 +03:00:34.7: 12.80 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry filter REJECTED candidate at 20:29:40.83 +03:00:34.7: ref_mag=12.80 +/- 0.02 new_mean_mag=12.8395 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:16:42.34 +07:39:00.7: 13.19 +/- 0.04 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:20:02.35 +08:22:56.5: 12.59 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:18:38.25 +02:16:19.4: 12.52 +/- 0.03 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:16:42.34 +07:39:00.7: 13.19 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Forced photometry filter KEPT candidate at 20:16:42.34 +07:39:00.7: ref_mag=13.19 +/- 0.03 new_mean_mag=12.2195 delta=0.97 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:19:58.21 +09:15:14.5: 13.16 +/- 0.05 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:20:02.35 +08:22:56.5: 12.63 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:18:38.25 +02:16:19.4: 12.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Forced photometry filter KEPT candidate at 20:18:38.25 +02:16:19.4: ref_mag=12.53 +/- 0.02 new_mean_mag=11.5531 delta=0.98 (need > 0.90)
Forced photometry reference-image weighted average: 12.61 +/- 0.02
Forced photometry filter KEPT candidate at 20:20:02.35 +08:22:56.5: ref_mag=12.61 +/- 0.02 new_mean_mag=11.5966 delta=1.01 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:24:18.44 +07:34:15.2: 11.99 +/- 0.01 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:18:25.05 +07:40:43.7: 13.31 +/- 0.05 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:19:58.21 +09:15:14.5: 13.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.04
Forced photometry filter KEPT candidate at 20:19:58.21 +09:15:14.5: ref_mag=13.17 +/- 0.04 new_mean_mag=12.2118 delta=0.95 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:24:18.44 +07:34:15.2: 12.02 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.01
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:18:25.05 +07:40:43.7: 13.27 +/- 0.05 detection
Forced photometry filter KEPT candidate at 20:24:18.44 +07:34:15.2: ref_mag=12.01 +/- 0.01 new_mean_mag=11.0561 delta=0.95 (need > 0.90)
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Forced photometry filter KEPT candidate at 20:18:25.05 +07:40:43.7: ref_mag=13.29 +/- 0.03 new_mean_mag=12.1715 delta=1.12 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:19:38.16 +04:35:49.4: 13.10 +/- 0.04 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:19:38.16 +04:35:49.4: 13.12 +/- 0.04 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:49:58.01 +03:19:28.9: 13.25 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.11 +/- 0.03
Forced photometry filter KEPT candidate at 20:19:38.16 +04:35:49.4: ref_mag=13.11 +/- 0.03 new_mean_mag=12.1520 delta=0.96 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:49:58.01 +03:19:28.9: 13.17 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry filter KEPT candidate at 20:49:58.01 +03:19:28.9: ref_mag=13.20 +/- 0.03 new_mean_mag=12.1865 delta=1.02 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:17:32.52 +03:49:08.8: 13.28 +/- 0.05 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:17:32.52 +03:49:08.8: 13.39 +/- 0.06 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:23:15.09 +07:57:21.8: 9.93 +/- 0.00 detection
Forced photometry reference-image weighted average: 13.33 +/- 0.04
Forced photometry filter KEPT candidate at 20:17:32.52 +03:49:08.8: ref_mag=13.33 +/- 0.04 new_mean_mag=12.4006 delta=0.93 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:40:34.80 +09:28:59.8: 12.37 +/- 0.02 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:23:15.09 +07:57:21.8: 9.96 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.95 +/- 0.00
Forced photometry filter KEPT candidate at 20:23:15.09 +07:57:21.8: ref_mag=9.95 +/- 0.00 new_mean_mag=8.9476 delta=1.00 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:24:32.92 +06:12:24.6: 13.22 +/- 0.04 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:40:34.80 +09:28:59.8: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.02
Forced photometry filter KEPT candidate at 20:40:34.80 +09:28:59.8: ref_mag=12.35 +/- 0.02 new_mean_mag=11.3343 delta=1.01 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:24:32.92 +06:12:24.6: 13.18 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.20 +/- 0.03
Forced photometry filter KEPT candidate at 20:24:32.92 +06:12:24.6: ref_mag=13.20 +/- 0.03 new_mean_mag=12.1967 delta=1.00 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:16:20.44 +06:15:35.8: 13.21 +/- 0.05 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_03-59-51_20.00sec_-4.90C_LIGHT_0435.fits at 20:52:05.37 +04:24:04.2: 13.49 +/- 0.06 detection
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:16:20.44 +06:15:35.8: 13.17 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.19 +/- 0.03
Forced photometry filter KEPT candidate at 20:16:20.44 +06:15:35.8: ref_mag=13.19 +/- 0.03 new_mean_mag=12.0613 delta=1.13 (need > 0.90)
Forced photometry on wcs_Del-02-Q2b1x1_2026-05-11_04-00-37_20.00sec_-4.90C_LIGHT_0436.fits at 20:52:05.37 +04:24:04.2: 13.43 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Forced photometry filter KEPT candidate at 20:52:05.37 +04:24:04.2: ref_mag=13.46 +/- 0.04 new_mean_mag=12.1273 delta=1.33 (need > 0.90)
Adding exclusion_list_local.txt__out101018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99226.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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: 10s
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Considering the candidate 138734_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 138734_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 140076_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 140076_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:18:54.06 +07:34:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140869_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 140869_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:30:38.54 +06:10:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140982_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 140982_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:29:19.31 +09:54:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141290_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 141290_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:17:27.61 +10:10:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141515_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 141515_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 141815_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 141815_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:30:14.81 +10:16:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141961_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 141961_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:25:39.87 +10:04:22.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 142033_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 142033_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 142069_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 142069_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:29:03.24 +06:58:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142422_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 142422_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 142527_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 142527_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 142584_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 142584_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 142827_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 142827_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:23:19.14 +05:20:48.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 142860_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 142860_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:48:26.70 +01:44:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143866_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 143866_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 143911_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 143911_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:33:51.53 +10:04:52.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 144248_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 144248_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 144289_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 144289_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 144327_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 144327_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
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Considering the candidate 144469_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 144469_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 97841_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 97841_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:21:26.93 +09:34:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115892_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 115892_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 109319_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 109319_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 14523_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 14523_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 112248_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 112248_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:25:38.48 +08:05:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62492_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 62492_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:19:09.71 +06:26:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101018_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 101018_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 114806_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 114806_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:23:35.23 +07:50:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115742_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 115742_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 116477_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 116477_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 105537_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 105537_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:32:44.08 +08:49:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40141_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 40141_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 24719_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 24719_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 31118_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 31118_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 50026_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 50026_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:22:40.16 +05:26:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113162_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 113162_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 99226_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 99226_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 63043_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 63043_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:34:14.24 +06:34:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59466_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 59466_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 29831_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 29831_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
**** FOUND 20:22:18.57 +03:43:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60572_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 60572_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 37105_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
Preparing report for the candidate 37105_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
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Considering the candidate 62709_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343
The candidate 62709_fd_Del-02-Q2b1x1_2026-07-08_05-50-48_20.00sec_5.00C_LIGHT_0343 did not pass the final checks
