This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 15.1220 2461206.6220 11.41 18:51:02.10 +13:38:34.6
45.07761 6.26192 galactic Her Second-epoch detections are separated by 0.3" and 7.4 pix
The object was found in VSX 5" ASAS J185102+1338.6
Type: MISC
# Max. Min./Amp. JD0 Period
12.202 V Y 0.784 V 93.694409000000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:51:02.10 +13:38:34.6: 12.35 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:51:02.10 +13:38:34.6: 12.37 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 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 06 15.1220* 18 51 02.10 +13 38 34.6 11.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185102+1338.6,2461206.6220,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J185102+1338.6 20260615.1220 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1220 2461206.6220 10.97 18:52:44.24 +15:32:57.1
46.98045 6.74047 galactic Her Second-epoch detections are separated by 0.6" and 7.4 pix
The object was found in VSX 3" ASAS J185244+1533.0
Type: SR
# Max. Min./Amp. JD0 Period
8.307 Ic Y 0.223 Ic 2454969.00000 983.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:52:44.24 +15:32:57.1: 11.92 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:52:44.24 +15:32:57.1: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 15.1220* 18 52 44.24 +15 32 57.1 11.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185244+1533.0,2461206.6220,10.97,0.05,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 J185244+1533.0 20260615.1220 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1220 2461206.6220 11.95 18:33:34.10 +16:06:03.2
45.45154 11.13150 galactic Her Second-epoch detections are separated by 1.7" and 6.8 pix
The object was found in VSX 2" DS Her
Type: M
# Max. Min./Amp. JD0 Period
11.000 pg < 15.500 pg 2440446.00000 263.430000000000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:33:34.10 +16:06:03.2: 13.05 +/- 0.03 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:33:34.10 +16:06:03.2: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 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 06 15.1220* 18 33 34.10 +16 06 03.2 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DS Her,2461206.6220,11.95,0.05,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
DS Her 20260615.1220 11.95CV 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 06 15.1220 2461206.6220 11.01 18:54:15.45 +13:46:57.2
45.55456 5.62395 galactic Her Second-epoch detections are separated by 1.8" and 7.5 pix
The object was found in VSX 7" ASAS J185416+1347.0
Type: MISC
# Max. Min./Amp. JD0 Period
12.013 V Y 0.567 V 93.168282000000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:54:15.45 +13:46:57.2: 12.04 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:54:15.45 +13:46:57.2: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 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 06 15.1220* 18 54 15.45 +13 46 57.2 11.0 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185416+1347.0,2461206.6220,11.01,0.05,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 J185416+1347.0 20260615.1220 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1220 2461206.6220 11.16 18:47:44.47 +11:12:23.8
42.52406 5.89471 galactic Aql Second-epoch detections are separated by 0.9" and 7.6 pix
The object was found in VSX 2" ASAS J184745+1112.4
Type: MISC
# Max. Min./Amp. JD0 Period
8.504 Ic Y 0.266 Ic 2452602.60000 66.890000000000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:47:44.47 +11:12:23.8: 12.08 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:47:44.47 +11:12:23.8: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184745+1112.4,2461206.6220,11.16,0.05,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
ASAS J184745+1112.4 20260615.1220 11.16CV 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 06 15.1220 2461206.6220 10.37 18:42:28.90 +14:01:13.8
44.49387 8.29130 galactic Her Second-epoch detections are separated by 0.7" and 7.2 pix
The object was found in VSX 2" NSV 24558
Type: LB:
# Max. Min./Amp. JD0 Period
12.120 V Y 0.370 V 2452968.40000 103.385292000000 M6III
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:42:28.90 +14:01:13.8: 11.29 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:42:28.90 +14:01:13.8: 11.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.29 +/- 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 06 15.1220* 18 42 28.90 +14 01 13.8 10.4 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 24558,2461206.6220,10.37,0.05,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
NSV 24558 20260615.1220 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1220 2461206.6220 12.32 18:34:22.76 +10:27:20.9
40.37787 8.50144 galactic Oph Second-epoch detections are separated by 3.1" and 8.0 pix
The object was found in VSX 3" V0626 Oph
Type: SR
# Max. Min./Amp. JD0 Period
14.644 g Y 1.265 g 2458273.74320 182.637185500000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:34:22.76 +10:27:20.9: 13.33 +/- 0.04 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:34:22.76 +10:27:20.9: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 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
V0626 Oph,2461206.6220,12.32,0.05,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
V0626 Oph 20260615.1220 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1220 2461206.6220 11.92 18:56:16.43 +14:46:24.1
46.66457 5.63075 galactic Her Second-epoch detections are separated by 0.7" and 7.2 pix
The object was found in VSX 2" ASASSN-V J185616.53+144624.5
Type: SR
# Max. Min./Amp. JD0 Period
14.603 g Y 0.393 g 2458301.02470 198.466020100000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:56:16.43 +14:46:24.1: 12.86 +/- 0.03 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:56:16.43 +14:46:24.1: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 15.1220* 18 56 16.43 +14 46 24.1 11.9 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185616.53+144624.5,2461206.6220,11.92,0.05,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 J185616.53+144624.5 20260615.1220 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1220 2461206.6220 12.43 18:22:47.56 +09:52:05.9
38.57139 10.80434 galactic Oph Second-epoch detections are separated by 1.2" and 7.7 pix
The object was found in VSX 2" V0884 Oph
Type: M
# Max. Min./Amp. JD0 Period
12.500 pg < 17.000 pg 2429450.00000 210.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:22:47.56 +09:52:05.9: 13.59 +/- 0.06 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:22:47.56 +09:52:05.9: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 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
V0884 Oph,2461206.6220,12.43,0.05,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
V0884 Oph 20260615.1220 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1220 2461206.6220 12.70 18:50:05.49 +17:49:14.2
48.75588 8.30983 galactic Her Second-epoch detections are separated by 2.4" and 6.8 pix
The object was found in VSX 1" ASASSN-V J185005.55+174915.5
Type: SR
# Max. Min./Amp. JD0 Period
15.523 g Y 0.801 g 2458358.19500 181.339601300000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:50:05.49 +17:49:14.2: 13.75 +/- 0.06 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:50:05.49 +17:49:14.2: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 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 06 15.1220* 18 50 05.49 +17 49 14.2 12.7 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185005.55+174915.5,2461206.6220,12.70,0.05,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 J185005.55+174915.5 20260615.1220 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1220 2461206.6220 10.94 18:57:47.76 +14:19:08.3
46.42276 5.09766 galactic Aql Second-epoch detections are separated by 0.4" and 7.5 pix
The object was found in VSX 2" ASAS J185748+1419.1
Type: MISC
# Max. Min./Amp. JD0 Period
12.459 V Y 0.877 V 27.729430000000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:57:47.76 +14:19:08.3: 11.93 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:57:47.76 +14:19:08.3: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185748+1419.1,2461206.6220,10.94,0.05,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 J185748+1419.1 20260615.1220 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 15.1220 2461206.6220 11.84 18:28:43.55 +12:17:43.4
41.43991 10.55251 galactic Her Second-epoch detections are separated by 0.9" and 7.4 pix
The object was found in VSX 2" KV Her
Type: SR
# Max. Min./Amp. JD0 Period
12.300 pg 16.000 pg 2425733.00000 203.500000000000
The object was not found in astcheck.
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:28:43.55 +12:17:43.4: 12.76 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:28:43.55 +12:17:43.4: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 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 06 15.1220* 18 28 43.55 +12 17 43.4 11.8 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KV Her,2461206.6220,11.84,0.05,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
KV Her 20260615.1220 11.84CV 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: 2461177.93905348 17.05.2026 10:32:04.221 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
First image: 2461177.93905348 17.05.2026 10:32:04.221 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
Last image: 2461206.62227663 15.06.2026 02:55:54.701 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 19630
Objects passed selection criteria: 19509
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 12028.5
Average stars matched: 11395.5 (94.7375 %)
Memory usage VmPeak: 124352 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jun 14 23:58:19 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: 2461177.93905348 17.05.2026 10:32:04.221 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
First image: 2461177.93905348 17.05.2026 10:32:04.221 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
Last image: 2461206.62227663 15.06.2026 02:55:54.701 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 75
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.40
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: 38 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): 178959
Objects passed selection criteria: 178459
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 116330
Average stars matched: 108057 (92.8887 %)
Memory usage VmPeak: 2001972 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jun 10 15:05:04 CDT 2026
VaST build number 1.0rc89-96-gc6da043e
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 15 00:04:40 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/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
SExtractor catalog cache: saved Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.cat to cache
SExtractor catalog cache: saved Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.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/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461206.62166493
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_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits exists and is non-empty
Saving wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits to local_wcs_cache/
'wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits' -> 'local_wcs_cache/wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits'
wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits exists and is non-empty
Saving wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits to local_wcs_cache/
'wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits' -> 'local_wcs_cache/wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits'
wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits exists and is non-empty
Saving wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits to local_wcs_cache/
'wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits' -> 'local_wcs_cache/wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits'
wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits exists and is non-empty
Saving wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits to local_wcs_cache/
'wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits' -> 'local_wcs_cache/wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits (1st reference image)
verification OK: wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:39:58.501 +14:00:05.66 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits (1st new image)
verification OK: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
Image size: 938.7'x624.2' 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: 18:40:01.320 +13:59:39.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:39:58.501 +14:00:05.66
Second-epoch image center 18:40:01.320 +13:59:39.29
Angular distance between the image centers 0.0135 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits (2nd new image)
verification OK: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
Image size: 938.7'x624.2' 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: 18:39:58.571 +13:59:22.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:39:58.501 +14:00:05.66
Second-epoch image center 18:39:58.571 +13:59:22.73
Angular distance between the image centers 0.0119 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:40:01.320 +13:59:39.29
Second-epoch second image center 18:39:58.571 +13:59:22.73
Angular distance between the image centers 0.01203 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits &> /tmp/tmp.yBvKwbxnSQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits &> /tmp/tmp.Hj4kzZ0975
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits &> /tmp/tmp.UCXuCxfhVt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits &> /tmp/tmp.kg5t3EoS8x
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.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_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits and wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.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_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits and wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat
Found non-empty wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits and wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat
The reference image (wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits) and catalog (wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat) found
'wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat' -> 'wcsmag.cat'
Read 24967 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.7484 to 288.1892 deg, Dec +8.6724 to +19.2637 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 271.7484 to 288.1892 deg, Dec 8.6724 to 19.2637 deg
Loaded 15121 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): 11706 out of 12595 total matches.
Matched with Tycho-2 12595 out of 24967 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.710950
a=0.000000 b=1.000000 c=22.710950
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.98
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.98
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 24967 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.7484 to 288.1892 deg, Dec +8.6724 to +19.2637 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 271.7484 to 288.1892 deg, Dec 8.6724 to 19.2637 deg
Loaded 15121 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): 11706 out of 12595 total matches.
Matched with Tycho-2 12595 out of 24967 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits:
Forced-photometry filter: calibrated wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits -> calib.txt_param_ref_wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits (aperture=6.1)
Read 24705 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.7482 to 288.1895 deg, Dec +8.6738 to +19.2640 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 271.7482 to 288.1895 deg, Dec 8.6738 to 19.2640 deg
Loaded 15118 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): 11686 out of 12596 total matches.
Matched with Tycho-2 12596 out of 24705 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits:
Forced-photometry filter: calibrated wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits -> calib.txt_param_ref_wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
2.3 pix Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
2.6 pix fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
2.6 pix fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
2.3 pix wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
2.3 pix wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
Limiting magnitude estimates:
15.0 mag. Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
15.0 mag. Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
13.3 mag. fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
13.3 mag. fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 10.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.yBvKwbxnSQ (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_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits' -> 'wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
WCS_IMAGE_NAME=wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
WCS-calibrated image found: wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
Checking if the catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat corresponding to the image wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat corresponding to the image wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
WCS catalog name: wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2083, passed=24967
Got 24967 stars (including 22868 good ones) from the SExtractor catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat
util/solve_plate_with_UCAC5 got 24967 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
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: 962 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 24771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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 493 to 548 (Dec 8.7 to 19.3)
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(), 24771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 24771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits N_match=961 sigma_overall_arcsec=0.617 sigma_q1_arcsec=0.432 sigma_q2_arcsec=0.724 sigma_q3_arcsec=0.566 sigma_q4_arcsec=0.765 n_q1=205 n_q2=270 n_q3=216 n_q4=270 worst_quadrant_to_overall_ratio=1.239
The image catalog is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits -region wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.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.Hj4kzZ0975 (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_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits' -> 'wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
WCS_IMAGE_NAME=wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
WCS-calibrated image found: wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
Checking if the catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat corresponding to the image wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat corresponding to the image wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
WCS catalog name: wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2072, passed=24705
Got 24705 stars (including 22618 good ones) from the SExtractor catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat
util/solve_plate_with_UCAC5 got 24705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
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(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 24456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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 493 to 548 (Dec 8.7 to 19.3)
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(), 24456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 24456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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=Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits N_match=958 sigma_overall_arcsec=0.600 sigma_q1_arcsec=0.467 sigma_q2_arcsec=0.695 sigma_q3_arcsec=0.575 sigma_q4_arcsec=0.722 n_q1=202 n_q2=272 n_q3=211 n_q4=273 worst_quadrant_to_overall_ratio=1.204
The image catalog is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits -region wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.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.UCXuCxfhVt (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
WCS-calibrated image found: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
Checking if the catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
WCS catalog name: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=345, passed=5158
Got 5158 stars (including 4813 good ones) from the SExtractor catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat
util/solve_plate_with_UCAC5 got 5158 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 961 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(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 5044 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits N_match=959 sigma_overall_arcsec=0.718 sigma_q1_arcsec=0.762 sigma_q2_arcsec=0.655 sigma_q3_arcsec=0.602 sigma_q4_arcsec=1.109 n_q1=284 n_q2=157 n_q3=281 n_q4=237 worst_quadrant_to_overall_ratio=1.546
The image catalog is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits -region wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.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.kg5t3EoS8x (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
WCS-calibrated image found: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
Checking if the catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
WCS catalog name: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=336, passed=5520
Got 5520 stars (including 5176 good ones) from the SExtractor catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat
util/solve_plate_with_UCAC5 got 5520 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 5397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits N_match=959 sigma_overall_arcsec=0.760 sigma_q1_arcsec=0.783 sigma_q2_arcsec=0.681 sigma_q3_arcsec=0.626 sigma_q4_arcsec=1.204 n_q1=299 n_q2=165 n_q3=265 n_q4=230 worst_quadrant_to_overall_ratio=1.585
The image catalog is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits -region wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.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=Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits sigma_overall=0.617 worst_q_ratio=1.239
ref2=Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits sigma_overall=0.600 worst_q_ratio=1.204
new1=fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits sigma_overall=0.718 worst_q_ratio=1.546
new2=fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits sigma_overall=0.760 worst_q_ratio=1.585
reference average sigma_overall=0.6085 worst_q_ratio=1.2215
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320_astrometric_residuals.png (961 matched stars from wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.57 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321_astrometric_residuals.png (958 matched stars from wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.54 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008_astrometric_residuals.png (959 matched stars from wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.69 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009_astrometric_residuals.png (959 matched stars from wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.68 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits'
Saving fully-calibrated image wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits'
Preparing the HTML report for the field Her-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20070_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 20070_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:37:19.32 +10:25:46.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Her-10-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/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
SExtractor catalog cache: saved Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.cat to cache
SExtractor catalog cache: saved Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
Creating symlink local_wcs_cache/wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
Creating symlink local_wcs_cache/wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
Creating symlink local_wcs_cache/wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.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_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits exists and is non-empty
wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits exists and is non-empty
wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits exists and is non-empty
wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits (1st reference image)
verification OK: wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 18:39:58.501 +14:00:05.66 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits (1st new image)
verification OK: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 938.7'x624.2' 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: 18:40:01.320 +13:59:39.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:39:58.501 +14:00:05.66
Second-epoch image center 18:40:01.320 +13:59:39.29
Angular distance between the image centers 0.0135 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits (2nd new image)
verification OK: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
Image size: 938.7'x624.2' 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: 18:39:58.571 +13:59:22.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:39:58.501 +14:00:05.66
Second-epoch image center 18:39:58.571 +13:59:22.73
Angular distance between the image centers 0.0119 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:40:01.320 +13:59:39.29
Second-epoch second image center 18:39:58.571 +13:59:22.73
Angular distance between the image centers 0.01203 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits &> /tmp/tmp.mo2krGYZF2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits &> /tmp/tmp.IbMhTkiixi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits &> /tmp/tmp.PvosDHYXUo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits &> /tmp/tmp.mcXxLecO5a
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.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_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits and wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.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_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits and wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat
Found non-empty wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits and wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat
The reference image (wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits) and catalog (wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat) found
'wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat' -> 'wcsmag.cat'
Read 213356 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.7458 to 288.2571 deg, Dec +8.6725 to +19.2659 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 271.7458 to 288.2571 deg, Dec 8.6725 to 19.2659 deg
Loaded 15181 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): 9490 out of 13160 total matches.
Matched with Tycho-2 13160 out of 213356 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.524050
a=0.000000 b=1.000000 c=22.524050
From vast_summary.log: estimated ref. image limiting mag.: -7.40
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.12
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.12
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 213356 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.7458 to 288.2571 deg, Dec +8.6725 to +19.2659 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 271.7458 to 288.2571 deg, Dec 8.6725 to 19.2659 deg
Loaded 15181 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): 9490 out of 13160 total matches.
Matched with Tycho-2 13160 out of 213356 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits:
Forced-photometry filter: calibrated wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits -> calib.txt_param_ref_wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits (aperture=4.5)
Read 214485 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.7453 to 288.2569 deg, Dec +8.6738 to +19.2672 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 271.7453 to 288.2569 deg, Dec 8.6738 to 19.2672 deg
Loaded 15177 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): 9535 out of 13195 total matches.
Matched with Tycho-2 13195 out of 214485 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits:
Forced-photometry filter: calibrated wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits -> calib.txt_param_ref_wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 64 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
2.2 pix Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
2.3 pix fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
2.3 pix fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
2.2 pix wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
2.2 pix wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
Limiting magnitude estimates:
15.1 mag. Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
15.1 mag. Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
13.5 mag. fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
13.6 mag. fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 13.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.mo2krGYZF2 (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_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits' -> 'wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
WCS_IMAGE_NAME=wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
WCS-calibrated image found: wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
Checking if the catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat corresponding to the image wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat corresponding to the image wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits
WCS catalog name: wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=30683, passed=213344
Got 213344 stars (including 182454 good ones) from the SExtractor catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat
util/solve_plate_with_UCAC5 got 213344 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 211685 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 211686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 211665 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits N_match=960 sigma_overall_arcsec=0.645 sigma_q1_arcsec=0.501 sigma_q2_arcsec=0.716 sigma_q3_arcsec=0.543 sigma_q4_arcsec=0.799 n_q1=213 n_q2=246 n_q3=239 n_q4=262 worst_quadrant_to_overall_ratio=1.238
The image catalog is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits -region wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.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.IbMhTkiixi (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_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits' -> 'wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
WCS_IMAGE_NAME=wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
WCS-calibrated image found: wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
Checking if the catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat corresponding to the image wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits alredy exist and is non-empty...
Catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat corresponding to the image wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits
WCS catalog name: wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=30949, passed=214466
Got 214466 stars (including 183307 good ones) from the SExtractor catalog wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat
util/solve_plate_with_UCAC5 got 214466 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 961 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(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 212932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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 493 to 548 (Dec 8.7 to 19.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 212930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 212925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits N_match=959 sigma_overall_arcsec=0.625 sigma_q1_arcsec=0.496 sigma_q2_arcsec=0.747 sigma_q3_arcsec=0.507 sigma_q4_arcsec=0.760 n_q1=214 n_q2=252 n_q3=236 n_q4=257 worst_quadrant_to_overall_ratio=1.216
The image catalog is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits -region wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.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.PvosDHYXUo (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
WCS-calibrated image found: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
Checking if the catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
WCS catalog name: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2537, passed=51430
Got 51430 stars (including 48848 good ones) from the SExtractor catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat
util/solve_plate_with_UCAC5 got 51430 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 957 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(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 50349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 957 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(), 50348 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 50349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits N_match=953 sigma_overall_arcsec=0.712 sigma_q1_arcsec=0.810 sigma_q2_arcsec=0.662 sigma_q3_arcsec=0.596 sigma_q4_arcsec=1.026 n_q1=294 n_q2=132 n_q3=311 n_q4=216 worst_quadrant_to_overall_ratio=1.441
The image catalog is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits -region wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.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.mcXxLecO5a (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
WCS_IMAGE_NAME=wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
WCS-calibrated image found: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
Checking if the catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat corresponding to the image wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
WCS catalog name: wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=2686, passed=54530
Got 54530 stars (including 51779 good ones) from the SExtractor catalog wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat
util/solve_plate_with_UCAC5 got 54530 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 957 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(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 53494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 957 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(), 53493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 53494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 954 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits N_match=954 sigma_overall_arcsec=0.743 sigma_q1_arcsec=0.761 sigma_q2_arcsec=0.556 sigma_q3_arcsec=0.650 sigma_q4_arcsec=1.112 n_q1=310 n_q2=146 n_q3=291 n_q4=207 worst_quadrant_to_overall_ratio=1.498
The image catalog is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits -region wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.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_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-01_20.00sec_4.90C_LIGHT_0008.fits
Saving fully-calibrated image wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-06-14_CI_Her-10-Q2b1x1_235308_TTUQ2b1x1_3038625_oGOwOC3D/wcs_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009.fits
Preparing the HTML report for the field Her-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:22:26.19 +15:31:55.5: 13.43 +/- 0.04 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:25:15.42 +16:24:14.6: 12.64 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:23:28.12 +13:45:49.5: 13.01 +/- 0.03 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:36:39.57 +13:24:42.8: 12.64 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:35:18.82 +15:29:03.4: 12.43 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:25:58.26 +16:50:49.7: 13.15 +/- 0.03 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:25:42.36 +14:43:07.7: 12.69 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:30:04.77 +15:50:23.7: 12.09 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:23:57.13 +14:48:28.4: 12.22 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:22:26.19 +15:31:55.5: 13.51 +/- 0.04 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:23:28.12 +13:45:49.5: 13.00 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:36:39.57 +13:24:42.8: 12.65 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 18:22:26.19 +15:31:55.5: ref_mag=13.47 +/- 0.03 new_mean_mag=13.3970 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:25:15.42 +16:24:14.6: 12.63 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:25:58.26 +16:50:49.7: 13.17 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 18:23:28.12 +13:45:49.5: ref_mag=13.00 +/- 0.02 new_mean_mag=13.0260 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:25:42.36 +14:43:07.7: 12.76 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:35:18.82 +15:29:03.4: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter REJECTED candidate at 18:36:39.57 +13:24:42.8: ref_mag=12.65 +/- 0.01 new_mean_mag=12.7308 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:25:15.42 +16:24:14.6: ref_mag=12.63 +/- 0.01 new_mean_mag=12.9120 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:25:58.26 +16:50:49.7: ref_mag=13.16 +/- 0.02 new_mean_mag=13.0863 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 12.72 +/- 0.02
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter REJECTED candidate at 18:25:42.36 +14:43:07.7: ref_mag=12.72 +/- 0.02 new_mean_mag=12.9035 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:35:18.82 +15:29:03.4: ref_mag=12.41 +/- 0.01 new_mean_mag=12.6280 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:30:04.77 +15:50:23.7: 12.13 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:23:57.13 +14:48:28.4: 12.23 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter REJECTED candidate at 18:30:04.77 +15:50:23.7: ref_mag=12.11 +/- 0.01 new_mean_mag=12.3592 delta=-0.25 (need > 0.90)
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter REJECTED candidate at 18:23:57.13 +14:48:28.4: ref_mag=12.23 +/- 0.01 new_mean_mag=12.3119 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:23:23.39 +14:42:28.1: 12.76 +/- 0.03 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:26:10.06 +12:38:37.6: 12.37 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:31:12.91 +14:45:57.7: 11.86 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:49:41.94 +15:54:28.2: 12.51 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:22:45.42 +14:18:05.5: 12.66 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:29:34.25 +12:27:19.0: 12.90 +/- 0.03 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:54:49.02 +09:52:49.9: 12.49 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:27:51.58 +14:41:11.1: 13.15 +/- 0.03 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:23:23.39 +14:42:28.1: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.02
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:31:12.91 +14:45:57.7: 11.89 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 18:23:23.39 +14:42:28.1: ref_mag=12.78 +/- 0.02 new_mean_mag=12.7851 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:26:10.06 +12:38:37.6: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.87 +/- 0.01
Forced photometry filter REJECTED candidate at 18:31:12.91 +14:45:57.7: ref_mag=11.87 +/- 0.01 new_mean_mag=12.1194 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:49:41.94 +15:54:28.2: 12.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter REJECTED candidate at 18:26:10.06 +12:38:37.6: ref_mag=12.37 +/- 0.01 new_mean_mag=12.1965 delta=0.17 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:22:45.42 +14:18:05.5: 12.66 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.51 +/- 0.02
Forced photometry filter REJECTED candidate at 18:49:41.94 +15:54:28.2: ref_mag=12.51 +/- 0.02 new_mean_mag=12.3320 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 12.66 +/- 0.02
Forced photometry filter REJECTED candidate at 18:22:45.42 +14:18:05.5: ref_mag=12.66 +/- 0.02 new_mean_mag=12.6780 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:27:51.58 +14:41:11.1: 13.04 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter REJECTED candidate at 18:27:51.58 +14:41:11.1: ref_mag=13.09 +/- 0.02 new_mean_mag=12.9625 delta=0.13 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:29:34.25 +12:27:19.0: 12.82 +/- 0.03 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:54:49.02 +09:52:49.9: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Forced photometry filter REJECTED candidate at 18:29:34.25 +12:27:19.0: ref_mag=12.86 +/- 0.02 new_mean_mag=12.7294 delta=0.13 (need > 0.90)
Forced photometry reference-image weighted average: 12.40 +/- 0.01
Forced photometry filter REJECTED candidate at 18:54:49.02 +09:52:49.9: ref_mag=12.40 +/- 0.01 new_mean_mag=11.9312 delta=0.47 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:51:31.87 +10:18:54.9: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:51:31.87 +10:18:54.9: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 18:51:31.87 +10:18:54.9: the source is saturated (present but too bright to measure) on at least one reference image -- likely a star-matching failure rather than a new transient
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:51:02.10 +13:38:34.6: 12.35 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:52:44.24 +15:32:57.1: 11.92 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:33:34.10 +16:06:03.2: 13.05 +/- 0.03 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:51:02.10 +13:38:34.6: 12.37 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter KEPT candidate at 18:51:02.10 +13:38:34.6: ref_mag=12.36 +/- 0.01 new_mean_mag=11.4086 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:54:15.45 +13:46:57.2: 12.04 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:52:44.24 +15:32:57.1: 11.93 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.92 +/- 0.01
Forced photometry filter KEPT candidate at 18:52:44.24 +15:32:57.1: ref_mag=11.92 +/- 0.01 new_mean_mag=10.9742 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:33:34.10 +16:06:03.2: 13.06 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry filter KEPT candidate at 18:33:34.10 +16:06:03.2: ref_mag=13.06 +/- 0.02 new_mean_mag=11.9456 delta=1.11 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:54:15.45 +13:46:57.2: 12.07 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.06 +/- 0.01
Forced photometry filter KEPT candidate at 18:54:15.45 +13:46:57.2: ref_mag=12.06 +/- 0.01 new_mean_mag=10.9937 delta=1.06 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:47:44.47 +11:12:23.8: 12.08 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:42:28.90 +14:01:13.8: 11.29 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:47:44.47 +11:12:23.8: 12.08 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:42:28.90 +14:01:13.8: 11.29 +/- 0.01 detection
Forced photometry filter KEPT candidate at 18:47:44.47 +11:12:23.8: ref_mag=12.08 +/- 0.01 new_mean_mag=11.1492 delta=0.93 (need > 0.90)
Forced photometry reference-image weighted average: 11.29 +/- 0.01
Forced photometry filter KEPT candidate at 18:42:28.90 +14:01:13.8: ref_mag=11.29 +/- 0.01 new_mean_mag=10.3653 delta=0.93 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:34:22.76 +10:27:20.9: 13.33 +/- 0.04 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:56:16.43 +14:46:24.1: 12.86 +/- 0.03 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:34:22.76 +10:27:20.9: 13.31 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry filter KEPT candidate at 18:34:22.76 +10:27:20.9: ref_mag=13.32 +/- 0.03 new_mean_mag=12.3099 delta=1.01 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:56:16.43 +14:46:24.1: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.87 +/- 0.02
Forced photometry filter KEPT candidate at 18:56:16.43 +14:46:24.1: ref_mag=12.87 +/- 0.02 new_mean_mag=11.9194 delta=0.95 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:22:47.56 +09:52:05.9: 13.59 +/- 0.06 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:56:36.93 +11:17:34.7: 13.43 +/- 0.06 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:22:47.56 +09:52:05.9: 13.45 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.04
Forced photometry filter KEPT candidate at 18:22:47.56 +09:52:05.9: ref_mag=13.52 +/- 0.04 new_mean_mag=12.4258 delta=1.09 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:56:36.93 +11:17:34.7: 13.45 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.04
Forced photometry filter KEPT candidate at 18:56:36.93 +11:17:34.7: ref_mag=13.44 +/- 0.04 new_mean_mag=12.3050 delta=1.14 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:50:05.49 +17:49:14.2: 13.75 +/- 0.06 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:50:05.49 +17:49:14.2: 13.72 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.04
Forced photometry filter KEPT candidate at 18:50:05.49 +17:49:14.2: ref_mag=13.74 +/- 0.04 new_mean_mag=12.6824 delta=1.05 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:57:47.76 +14:19:08.3: 11.93 +/- 0.01 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:57:47.76 +14:19:08.3: 11.96 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.94 +/- 0.01
Forced photometry filter KEPT candidate at 18:57:47.76 +14:19:08.3: ref_mag=11.94 +/- 0.01 new_mean_mag=10.9173 delta=1.03 (need > 0.90)
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-04_20.00sec_0.00C_LIGHT_1320.fits at 18:28:43.55 +12:17:43.4: 12.76 +/- 0.02 detection
Forced photometry on wcs_Her-10-Q2b1x1_2026-05-17_05-32-29_20.00sec_-0.00C_LIGHT_1321.fits at 18:28:43.55 +12:17:43.4: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Forced photometry filter KEPT candidate at 18:28:43.55 +12:17:43.4: ref_mag=12.77 +/- 0.02 new_mean_mag=11.8390 delta=0.93 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out160076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out102296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93966.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
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: 7s
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Considering the candidate 241902_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241902_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 241915_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241915_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 241920_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241920_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 241921_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241921_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:23:34.09 +17:03:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 241922_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241922_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:23:52.92 +17:24:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 241923_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241923_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 241925_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241925_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 241928_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241928_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 241932_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241932_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 241933_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241933_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:32:52.45 +17:29:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 241935_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241935_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:22:27.58 +17:11:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 241938_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241938_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 241939_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241939_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 241941_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 241941_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:49:11.07 +17:13:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244530_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 244530_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:51:45.01 +12:13:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246344_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 246344_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 246549_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 246549_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:37:41.57 +09:45:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246611_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 246611_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 247252_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 247252_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:47:20.84 +16:53:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247454_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 247454_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:39:50.45 +09:58:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248768_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 248768_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 248950_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 248950_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 249090_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 249090_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 249347_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 249347_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 250047_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 250047_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 250249_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 250249_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:38:37.55 +15:05:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251266_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 251266_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:37:16.62 +11:20:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251712_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 251712_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 254184_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 254184_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:53:01.88 +09:46:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 225754_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 225754_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
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Considering the candidate 109184_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 109184_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 54364_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 54364_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:58:10.75 +16:18:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70026_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 70026_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 94500_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 94500_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:55:18.43 +14:18:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59363_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 59363_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 115895_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 115895_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:55:45.90 +13:16:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185537_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 185537_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:44:20.56 +10:33:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105952_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 105952_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 162257_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 162257_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:22:27.18 +11:12:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88808_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 88808_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:49:40.65 +14:34:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163170_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 163170_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 102296_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 102296_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 123279_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 123279_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:57:05.96 +12:58:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197478_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 197478_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:38:43.55 +11:02:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143867_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 143867_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:44:23.05 +12:00:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80865_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 80865_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:30:08.28 +14:57:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183510_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 183510_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 130734_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 130734_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:55:53.08 +12:34:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84207_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 84207_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 80950_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 80950_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:50:19.11 +14:56:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171267_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 171267_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 160076_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 160076_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:56:36.93 +11:17:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 2.834 4312086245377317504 284.15467117617 +11.29307178777 10.4376 8.8320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 36186_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 36186_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:33:20.66 +17:15:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27519_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 27519_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:35:43.02 +17:43:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25299_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 25299_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 74726_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 74726_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:29:11.22 +15:16:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129383_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 129383_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:25:07.90 +12:43:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93966_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 93966_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 137602_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
Preparing report for the candidate 137602_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
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Considering the candidate 227366_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 227366_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:38:29.56 +11:11:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163365_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 163365_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:37:19.31 +10:25:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189338_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 189338_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:55:12.59 +10:41:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 225698_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 225698_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
**** FOUND 18:52:02.03 +09:53:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83948_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009
The candidate 83948_fd_Her-10-Q2b1x1_2026-06-14_21-55-54_20.00sec_5.00C_LIGHT_0009 did not pass the final checks
