This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 03.4565 2461255.9565 12.70 05:56:12.51 +05:06:50.0
201.94854 -9.84091 galactic Ori Second-epoch detections are separated by 0.8" and 9.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.185 Eunike -0 1 1 13.0 0 0
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:56:12.51 +05:06:50.0: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:56:12.51 +05:06:50.0: 16.18 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.4565* 05 56 12.51 +05 06 50.0 12.7 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461255.9565,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.4565 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 08 03.4565 2461255.9565 12.68 06:02:49.73 +09:32:13.3
198.83414 -6.26994 galactic Ori Second-epoch detections are separated by 0.8" and 8.8 pix
The object was found in VSX 4" Dauban V274
Type: VAR
# Max. Min./Amp. JD0 Period
10.900 CR < 13.600 CR
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:02:49.73 +09:32:13.3: 14.39 +/- 0.10 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:02:49.73 +09:32:13.3: 14.57 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.07
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.4565* 06 02 49.73 +09 32 13.3 12.7 U Ori 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
Dauban V274,2461255.9565,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Dauban V274 20260803.4565 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4565 2461255.9565 12.61 05:46:42.05 +06:43:48.0
199.34436 -11.12311 galactic Ori Second-epoch detections are separated by 0.9" and 9.4 pix
The object was found in VSX 1" ASAS J054642+0643.7
Type: M
# Max. Min./Amp. JD0 Period
11.480 V 14.600 V 2453849.00000 376.000000000000 C-N5e C2 6-
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:46:42.05 +06:43:48.0: 14.52 +/- 0.09 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:46:42.05 +06:43:48.0: 14.34 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.42 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.4565* 05 46 42.05 +06 43 48.0 12.6 U Ori 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 J054642+0643.7,2461255.9565,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J054642+0643.7 20260803.4565 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4565 2461255.9565 12.16 05:55:09.31 +02:40:55.9
203.99419 -11.23290 galactic Ori Second-epoch detections are separated by 0.6" and 9.3 pix
The object was found in VSX 1" NSVS 12370786
Type: L
# Max. Min./Amp. JD0 Period
10.950 R1 11.250 R1
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:55:09.31 +02:40:55.9: 13.19 +/- 0.03 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:55:09.31 +02:40:55.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.4565* 05 55 09.31 +02 40 55.9 12.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 12370786,2461255.9565,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 12370786 20260803.4565 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4565 2461255.9565 11.49 06:12:59.35 +02:20:46.5
206.41650 -7.45902 galactic Ori Second-epoch detections are separated by 3.8" and 9.2 pix
The object was found in VSX 1" ASAS J061259+0220.8
Type: MISC
# Max. Min./Amp. JD0 Period
9.178 Ic Y 0.490 Ic 2452860.50000 236.400000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:12:59.35 +02:20:46.5: 12.90 +/- 0.03 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:12:59.35 +02:20:46.5: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.4565* 06 12 59.35 +02 20 46.5 11.5 U Ori 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 J061259+0220.8,2461255.9565,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061259+0220.8 20260803.4565 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4565 2461255.9565 11.66 06:06:41.00 +05:44:54.1
202.64358 -7.24739 galactic Ori Second-epoch detections are separated by 1.2" and 9.4 pix
The object was found in VSX 1" ASAS J060641+0544.9
Type: MISC
# Max. Min./Amp. JD0 Period
8.789 Ic Y 0.538 Ic 2453144.60000 269.200000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:06:41.00 +05:44:54.1: 12.66 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:06:41.00 +05:44:54.1: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.4565* 06 06 41.00 +05 44 54.1 11.7 U Ori 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 J060641+0544.9,2461255.9565,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J060641+0544.9 20260803.4565 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4565 2461255.9565 11.35 06:16:06.45 +06:46:37.5
202.84516 -4.69733 galactic Ori Second-epoch detections are separated by 0.3" and 9.4 pix
The object was found in VSX 1" ASAS J061606+0646.6
Type: MISC
# Max. Min./Amp. JD0 Period
12.740 V Y 0.850 V 2452893.70000 191.446735000000 C
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:16:06.45 +06:46:37.5: 12.27 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:16:06.45 +06:46:37.5: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.29 +/- 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 08 03.4565* 06 16 06.45 +06 46 37.5 11.3 U Ori 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 J061606+0646.6,2461255.9565,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061606+0646.6 20260803.4565 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4565 2461255.9565 11.23 06:17:07.44 +02:34:44.8
206.69264 -6.43644 galactic Ori Second-epoch detections are separated by 1.2" and 9.6 pix
The object was found in VSX 0" ASAS J061707+0234.7
Type: MISC
# Max. Min./Amp. JD0 Period
12.740 V Y 0.590 V 2452687.50000 92.384029000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:17:07.44 +02:34:44.8: 12.20 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:17:07.44 +02:34:44.8: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.4565* 06 17 07.44 +02 34 44.8 11.2 U Ori 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 J061707+0234.7,2461255.9565,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061707+0234.7 20260803.4565 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.4565 2461255.9565 12.65 05:57:29.61 +06:06:56.1
201.21401 -9.07891 galactic Ori Second-epoch detections are separated by 0.9" and 9.2 pix
The object was found in VSX 1" ASASSN-V J055729.68+060656.6
Type: L
# Max. Min./Amp. JD0 Period
13.670 V 14.190 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:57:29.61 +06:06:56.1: 13.75 +/- 0.04 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:57:29.61 +06:06:56.1: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 03.4565* 05 57 29.61 +06 06 56.1 12.7 U Ori 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 J055729.68+060656.6,2461255.9565,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J055729.68+060656.6 20260803.4565 12.65CV 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: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
First image: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Last image: 2461255.95685024 03.08.2026 10:57:41.861 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
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: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 22390
Objects passed selection criteria: 22239
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: 13736.8
Average stars matched: 13291.2 (96.7569 %)
Memory usage VmPeak: 247044 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 3 06:00:42 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: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
First image: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Last image: 2461255.95685024 03.08.2026 10:57:41.861 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.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.: -7.46
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 20 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 150689
Objects passed selection criteria: 150204
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: 97411.5
Average stars matched: 93554.5 (96.0405 %)
Memory usage VmPeak: 550228 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Aug 3 06:03:47 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat to cache
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.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/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.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: 2461255.95620251
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'
Plate-solving the images
wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits exists and is non-empty
Saving wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits to local_wcs_cache/
'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits' -> 'local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits'
wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits exists and is non-empty
Saving wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits to local_wcs_cache/
'wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits' -> 'local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits'
wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits exists and is non-empty
Saving wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits to local_wcs_cache/
'wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits' -> 'local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits'
wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits exists and is non-empty
Saving wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits to local_wcs_cache/
'wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits' -> 'local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (1st reference image)
verification OK: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:57.457 +05:59:33.15 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits (1st new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:10.197 +05:57:53.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:57.457 +05:59:33.15
Second-epoch image center 06:00:10.197 +05:57:53.83
Angular distance between the image centers 0.0596 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits (2nd new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:07.209 +05:58:26.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:57.457 +05:59:33.15
Second-epoch image center 06:00:07.209 +05:58:26.61
Angular distance between the image centers 0.0444 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 06:00:10.197 +05:57:53.83
Second-epoch second image center 06:00:07.209 +05:58:26.61
Angular distance between the image centers 0.01537 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits &> /tmp/tmp.YqYQEnXjcm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits &> /tmp/tmp.ebEyOxVxn8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits &> /tmp/tmp.xh82ZZV3zY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits &> /tmp/tmp.qPJp5pNCtB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.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_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
'tns_transients_list.txt' -> '../tns_transients_list.txt'
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_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
The reference image (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits) and catalog (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat) found
'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat' -> 'wcsmag.cat'
Read 23947 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9156 to 97.9251 deg, Dec +0.5852 to +11.3169 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 81.9156 to 97.9251 deg, Dec 0.5852 to 11.3169 deg
Loaded 13838 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): 10471 out of 11616 total matches.
Matched with Tycho-2 11616 out of 23947 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.917600
a=0.000000 b=1.000000 c=22.917600
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23947 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9156 to 97.9251 deg, Dec +0.5852 to +11.3169 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 81.9156 to 97.9251 deg, Dec 0.5852 to 11.3169 deg
Loaded 13838 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): 10471 out of 11616 total matches.
Matched with Tycho-2 11616 out of 23947 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (aperture=6.3)
Read 23981 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9156 to 97.9135 deg, Dec +0.6076 to +11.3239 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 81.9156 to 97.9135 deg, Dec 0.6076 to 11.3239 deg
Loaded 13821 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): 10495 out of 11630 total matches.
Matched with Tycho-2 11630 out of 23981 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
2.3 pix Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
2.6 pix fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
2.6 pix fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Limiting magnitude estimates:
15.1 mag. Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
15.1 mag. Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
12.7 mag. fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
12.6 mag. fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 10.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.YqYQEnXjcm (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_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2599, bad_region=0, passed=23947
Got 23947 stars (including 21319 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
util/solve_plate_with_UCAC5 got 23947 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4843 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 4781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 23947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4843 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 23947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 23947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4781 stars left (next iteration limit 5259)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits N_match=4781 sigma_overall_arcsec=0.442 sigma_q1_arcsec=0.485 sigma_q2_arcsec=0.402 sigma_q3_arcsec=0.393 sigma_q4_arcsec=0.445 n_q1=820 n_q2=1207 n_q3=1001 n_q4=1753 worst_quadrant_to_overall_ratio=1.098
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.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.ebEyOxVxn8 (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_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2508, bad_region=0, passed=23981
Got 23981 stars (including 21438 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat
util/solve_plate_with_UCAC5 got 23981 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4842 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 4781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4781 matched stars entering correct_measured_positions(), 23981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4842 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4780 matched stars entering correct_measured_positions(), 23981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4780 matched stars entering correct_measured_positions(), 23981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4780 stars left (next iteration limit 5259)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits N_match=4780 sigma_overall_arcsec=0.417 sigma_q1_arcsec=0.462 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.366 sigma_q4_arcsec=0.427 n_q1=829 n_q2=1201 n_q3=1010 n_q4=1740 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.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.xh82ZZV3zY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=347, bad_region=0, passed=3746
Got 3746 stars (including 3394 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat
util/solve_plate_with_UCAC5 got 3746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
Done reading UCAC5 zone files...
Matched 3263 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3205 matched stars entering correct_measured_positions(), 3208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3205 matched stars entering correct_measured_positions(), 3746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
Done reading UCAC5 zone files...
Matched 3259 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3207 matched stars entering correct_measured_positions(), 3746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 3207 matched stars entering correct_measured_positions(), 3746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 3207 stars left (next iteration limit 3525)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3207 robust_rms=10.039 arcsec worst_quadrant_rms=13.936 arcsec
SIP_REFIT: SIP order 3 trial: matched=3207 robust_rms=0.622 arcsec worst_quadrant_rms=1.150 arcsec
SIP_REFIT: SIP order 5 trial: matched=3207 robust_rms=0.454 arcsec worst_quadrant_rms=0.617 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3207 robust_rms_before=1.455 arcsec robust_rms_before_corrected=0.493 arcsec robust_rms_after=0.454 arcsec worst_quadrant_rms_before=0.583 worst_quadrant_rms_after=0.617
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.583 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits N_match=3207 sigma_overall_arcsec=0.489 sigma_q1_arcsec=0.499 sigma_q2_arcsec=0.609 sigma_q3_arcsec=0.370 sigma_q4_arcsec=0.519 n_q1=741 n_q2=597 n_q3=896 n_q4=973 worst_quadrant_to_overall_ratio=1.245
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits -region wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.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.qPJp5pNCtB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=358, bad_region=0, passed=3628
Got 3628 stars (including 3268 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat
util/solve_plate_with_UCAC5 got 3628 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
Done reading UCAC5 zone files...
Matched 3141 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3082 matched stars entering correct_measured_positions(), 3086 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3082 matched stars entering correct_measured_positions(), 3628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
Done reading UCAC5 zone files...
Matched 3139 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3082 matched stars entering correct_measured_positions(), 3628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 3082 matched stars entering correct_measured_positions(), 3628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 3082 stars left (next iteration limit 3390)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3082 robust_rms=10.261 arcsec worst_quadrant_rms=13.679 arcsec
SIP_REFIT: SIP order 3 trial: matched=3082 robust_rms=0.767 arcsec worst_quadrant_rms=1.036 arcsec
SIP_REFIT: SIP order 5 trial: matched=3082 robust_rms=0.497 arcsec worst_quadrant_rms=0.740 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3082 robust_rms_before=1.455 arcsec robust_rms_before_corrected=0.477 arcsec robust_rms_after=0.497 arcsec worst_quadrant_rms_before=0.585 worst_quadrant_rms_after=0.740
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.585 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits N_match=3082 sigma_overall_arcsec=0.476 sigma_q1_arcsec=0.449 sigma_q2_arcsec=0.588 sigma_q3_arcsec=0.372 sigma_q4_arcsec=0.558 n_q1=706 n_q2=569 n_q3=860 n_q4=947 worst_quadrant_to_overall_ratio=1.234
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits -region wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.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=Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits sigma_overall=0.442 worst_q_ratio=1.098
ref2=Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits sigma_overall=0.417 worst_q_ratio=1.108
new1=fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits sigma_overall=0.489 worst_q_ratio=1.245
new2=fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits sigma_overall=0.476 worst_q_ratio=1.234
reference average sigma_overall=0.4295 worst_q_ratio=1.103
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032_astrometric_residuals.png (4781 matched stars from wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033_astrometric_residuals.png (4780 matched stars from wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474_astrometric_residuals.png (3207 matched stars from wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475_astrometric_residuals.png (3082 matched stars from wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits'
Saving fully-calibrated image wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits'
Preparing the HTML report for the field Ori-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31608_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 31608_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:08:59.64 +02:29:47.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31720_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 31720_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:44:28.85 +06:52:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13836_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 13836_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:31:55.96 +07:36:48.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05113_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 05113_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:10:44.95 +03:45:25.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01005_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 01005_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:52:45.13 +01:13:22.3 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 Ori-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat to cache
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Creating symlink local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.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_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits exists and is non-empty
wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits exists and is non-empty
wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits exists and is non-empty
wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (1st reference image)
verification OK: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:59:57.457 +05:59:33.15 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits (1st new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:10.197 +05:57:53.83 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:57.457 +05:59:33.15
Second-epoch image center 06:00:10.197 +05:57:53.83
Angular distance between the image centers 0.0596 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits (2nd new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:00:07.209 +05:58:26.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:57.457 +05:59:33.15
Second-epoch image center 06:00:07.209 +05:58:26.61
Angular distance between the image centers 0.0444 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 06:00:10.197 +05:57:53.83
Second-epoch second image center 06:00:07.209 +05:58:26.61
Angular distance between the image centers 0.01537 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits &> /tmp/tmp.MrVysm7YmF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits &> /tmp/tmp.PgHiniBXVI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits &> /tmp/tmp.elB1xDmbkh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits &> /tmp/tmp.DFQbchbfyl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.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_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.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_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
The reference image (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits) and catalog (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat) found
'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat' -> 'wcsmag.cat'
Read 165923 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9025 to 97.9258 deg, Dec +0.5713 to +11.3193 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 81.9025 to 97.9258 deg, Dec 0.5713 to 11.3193 deg
Loaded 13864 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): 8480 out of 12115 total matches.
Matched with Tycho-2 12115 out of 165923 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.768800
a=0.000000 b=1.000000 c=22.768800
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 165923 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9025 to 97.9258 deg, Dec +0.5713 to +11.3193 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 81.9025 to 97.9258 deg, Dec 0.5713 to 11.3193 deg
Loaded 13864 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): 8480 out of 12115 total matches.
Matched with Tycho-2 12115 out of 165923 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (aperture=4.7)
Read 164824 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.8906 to 97.9164 deg, Dec +0.5830 to +11.3271 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 81.8906 to 97.9164 deg, Dec 0.5830 to 11.3271 deg
Loaded 13866 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): 8525 out of 12126 total matches.
Matched with Tycho-2 12126 out of 164824 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 67 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
2.1 pix Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
2.5 pix fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
2.4 pix fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Limiting magnitude estimates:
15.3 mag. Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
15.3 mag. Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
13.0 mag. fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
13.0 mag. fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
All-image limiting magnitude estimate: 13.0 (SNR ) 12.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.MrVysm7YmF (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_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=50, blended=21856, bad_region=0, passed=165873
Got 165873 stars (including 143783 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat
util/solve_plate_with_UCAC5 got 165873 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4836 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 4785 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4784 matched stars entering correct_measured_positions(), 165873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4836 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4786 matched stars entering correct_measured_positions(), 165873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4786 matched stars entering correct_measured_positions(), 165873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4786 stars left (next iteration limit 5262)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits N_match=4786 sigma_overall_arcsec=0.403 sigma_q1_arcsec=0.436 sigma_q2_arcsec=0.383 sigma_q3_arcsec=0.361 sigma_q4_arcsec=0.418 n_q1=899 n_q2=1223 n_q3=1055 n_q4=1609 worst_quadrant_to_overall_ratio=1.083
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.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.PgHiniBXVI (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_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=53, blended=21523, bad_region=1, passed=164771
Got 164771 stars (including 143000 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat
util/solve_plate_with_UCAC5 got 164771 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4841 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4795 matched stars entering correct_measured_positions(), 4795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4795 matched stars entering correct_measured_positions(), 164771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4841 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4794 matched stars entering correct_measured_positions(), 164771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4794 matched stars entering correct_measured_positions(), 164771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4794 stars left (next iteration limit 5274)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits N_match=4794 sigma_overall_arcsec=0.399 sigma_q1_arcsec=0.413 sigma_q2_arcsec=0.375 sigma_q3_arcsec=0.348 sigma_q4_arcsec=0.422 n_q1=916 n_q2=1211 n_q3=1057 n_q4=1610 worst_quadrant_to_overall_ratio=1.056
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.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.elB1xDmbkh (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=941, bad_region=2, passed=30990
Got 30990 stars (including 30008 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat
util/solve_plate_with_UCAC5 got 30990 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4812 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4735 matched stars entering correct_measured_positions(), 4739 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4735 matched stars entering correct_measured_positions(), 30990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4808 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4734 matched stars entering correct_measured_positions(), 30990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4734 matched stars entering correct_measured_positions(), 30990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 4734 stars left (next iteration limit 5208)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits N_match=4734 sigma_overall_arcsec=0.478 sigma_q1_arcsec=0.497 sigma_q2_arcsec=0.596 sigma_q3_arcsec=0.398 sigma_q4_arcsec=0.511 n_q1=1037 n_q2=811 n_q3=1385 n_q4=1501 worst_quadrant_to_overall_ratio=1.245
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits -region wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.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.DFQbchbfyl (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=912, bad_region=2, passed=30287
Got 30287 stars (including 29314 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat
util/solve_plate_with_UCAC5 got 30287 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4812 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4735 matched stars entering correct_measured_positions(), 4741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4735 matched stars entering correct_measured_positions(), 30287 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4808 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4736 matched stars entering correct_measured_positions(), 30287 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 4736 matched stars entering correct_measured_positions(), 30287 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4736 stars left (next iteration limit 5208)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits N_match=4736 sigma_overall_arcsec=0.465 sigma_q1_arcsec=0.464 sigma_q2_arcsec=0.561 sigma_q3_arcsec=0.379 sigma_q4_arcsec=0.520 n_q1=1021 n_q2=810 n_q3=1379 n_q4=1526 worst_quadrant_to_overall_ratio=1.206
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits -region wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.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_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-56-45_20.00sec_-0.00C_LIGHTs_0474.fits
Saving fully-calibrated image wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-03_CI_Ori-04-Q1b1x1_055814_TTUQ1b1x1_1576959_pPXWv07w/wcs_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475.fits
Preparing the HTML report for the field Ori-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:30:30.16 +02:47:06.7: 10.70 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:34:52.49 +01:59:05.0: 11.80 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:29:54.10 +01:23:12.4: 9.70 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:29:51.35 +01:37:28.2: 9.59 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:29:41.04 +01:23:08.7: 10.11 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:29:55.59 +01:27:28.6: 99.00 +/- 99.00 saturated
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:34:52.49 +01:59:05.0: 11.81 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:30:30.16 +02:47:06.7: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.01
Forced photometry reference-image weighted average: 10.71 +/- 0.00
Forced photometry filter REJECTED candidate at 05:34:52.49 +01:59:05.0: ref_mag=11.81 +/- 0.01 new_mean_mag=11.9832 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:30:30.16 +02:47:06.7: ref_mag=10.71 +/- 0.00 new_mean_mag=10.8853 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:28:21.72 +01:04:45.1: 10.24 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:29:42.91 +01:27:51.9: 9.95 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:28:22.05 +01:08:15.7: 10.18 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:27:39.05 +00:59:03.5: 10.17 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:29:54.10 +01:23:12.4: 9.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.70 +/- 0.00
Forced photometry filter REJECTED candidate at 06:29:54.10 +01:23:12.4: ref_mag=9.70 +/- 0.00 new_mean_mag=10.1708 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:29:51.35 +01:37:28.2: 9.56 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:29:41.04 +01:23:08.7: 10.10 +/- 0.00 detection
Forced photometry reference-image weighted average: 9.58 +/- 0.00
Forced photometry reference-image weighted average: 10.11 +/- 0.00
Forced photometry filter REJECTED candidate at 06:29:51.35 +01:37:28.2: ref_mag=9.58 +/- 0.00 new_mean_mag=9.9337 delta=-0.36 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:29:55.59 +01:27:28.6: 99.00 +/- 99.00 saturated
Forced photometry filter REJECTED candidate at 06:29:55.59 +01:27:28.6: 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 filter REJECTED candidate at 06:29:41.04 +01:23:08.7: ref_mag=10.11 +/- 0.00 new_mean_mag=10.5476 delta=-0.44 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:28:21.72 +01:04:45.1: 10.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.25 +/- 0.00
Forced photometry filter REJECTED candidate at 06:28:21.72 +01:04:45.1: ref_mag=10.25 +/- 0.00 new_mean_mag=10.5972 delta=-0.35 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:28:22.05 +01:08:15.7: 10.20 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:29:42.91 +01:27:51.9: 9.94 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.19 +/- 0.00
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:27:39.05 +00:59:03.5: 10.18 +/- 0.00 detection
Forced photometry filter REJECTED candidate at 06:28:22.05 +01:08:15.7: ref_mag=10.19 +/- 0.00 new_mean_mag=10.7772 delta=-0.59 (need > 0.90)
Forced photometry reference-image weighted average: 9.94 +/- 0.00
Forced photometry filter REJECTED candidate at 06:29:42.91 +01:27:51.9: ref_mag=9.94 +/- 0.00 new_mean_mag=10.6224 delta=-0.68 (need > 0.90)
Forced photometry reference-image weighted average: 10.18 +/- 0.00
Forced photometry filter REJECTED candidate at 06:27:39.05 +00:59:03.5: ref_mag=10.18 +/- 0.00 new_mean_mag=10.8005 delta=-0.62 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:55:17.06 +07:28:22.5: 12.25 +/- 0.11 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:28:53.55 +01:15:53.6: 10.48 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:28:52.58 +01:12:42.2: 10.78 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:29:29.76 +01:20:08.9: 10.92 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:55:17.06 +07:28:22.5: 12.19 +/- 0.09 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:28:53.55 +01:15:53.6: 10.49 +/- 0.00 detection
Forced photometry reference-image weighted average: 12.21 +/- 0.07
Forced photometry filter REJECTED candidate at 05:55:17.06 +07:28:22.5: ref_mag=12.21 +/- 0.07 new_mean_mag=11.5396 delta=0.68 (need > 0.90)
Forced photometry reference-image weighted average: 10.49 +/- 0.00
Forced photometry filter REJECTED candidate at 06:28:53.55 +01:15:53.6: ref_mag=10.49 +/- 0.00 new_mean_mag=10.9715 delta=-0.49 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:28:44.61 +01:22:06.1: 11.22 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:20:46.47 +00:49:01.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:28:38.46 +01:04:32.3: 10.71 +/- 0.00 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:29:29.76 +01:20:08.9: 10.93 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:28:52.58 +01:12:42.2: 10.77 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.92 +/- 0.00
Forced photometry reference-image weighted average: 10.78 +/- 0.00
Forced photometry filter REJECTED candidate at 06:29:29.76 +01:20:08.9: ref_mag=10.92 +/- 0.00 new_mean_mag=11.2936 delta=-0.37 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:28:52.58 +01:12:42.2: ref_mag=10.78 +/- 0.00 new_mean_mag=11.1829 delta=-0.41 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:28:07.95 +01:06:30.2: 10.83 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:28:44.61 +01:22:06.1: 11.24 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:20:46.47 +00:49:01.4: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 06:20:46.47 +00:49:01.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:28:38.46 +01:04:32.3: 10.71 +/- 0.00 detection
Forced photometry reference-image weighted average: 11.23 +/- 0.00
Forced photometry filter REJECTED candidate at 06:28:44.61 +01:22:06.1: ref_mag=11.23 +/- 0.00 new_mean_mag=11.3529 delta=-0.12 (need > 0.90)
Forced photometry reference-image weighted average: 10.71 +/- 0.00
Forced photometry filter REJECTED candidate at 06:28:38.46 +01:04:32.3: ref_mag=10.71 +/- 0.00 new_mean_mag=11.2663 delta=-0.56 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:28:23.49 +00:57:37.8: 11.04 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:28:07.95 +01:06:30.2: 10.85 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.84 +/- 0.00
Forced photometry filter REJECTED candidate at 06:28:07.95 +01:06:30.2: ref_mag=10.84 +/- 0.00 new_mean_mag=11.3807 delta=-0.54 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:08:35.45 +07:18:33.8: 12.43 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:56:12.51 +05:06:50.0: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:28:23.49 +00:57:37.8: 11.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.04 +/- 0.00
Forced photometry filter REJECTED candidate at 06:28:23.49 +00:57:37.8: ref_mag=11.04 +/- 0.00 new_mean_mag=11.5270 delta=-0.49 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:08:35.45 +07:18:33.8: 12.43 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.43 +/- 0.01
Forced photometry filter REJECTED candidate at 06:08:35.45 +07:18:33.8: ref_mag=12.43 +/- 0.01 new_mean_mag=12.2054 delta=0.23 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:56:12.51 +05:06:50.0: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:02:49.73 +09:32:13.3: 14.39 +/- 0.10 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:46:42.05 +06:43:48.0: 14.52 +/- 0.09 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:55:09.31 +02:40:55.9: 13.19 +/- 0.03 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:02:49.73 +09:32:13.3: 14.57 +/- 0.11 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:46:42.05 +06:43:48.0: 14.34 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.07
Forced photometry filter KEPT candidate at 06:02:49.73 +09:32:13.3: ref_mag=14.47 +/- 0.07 new_mean_mag=12.6722 delta=1.80 (need > 0.90)
Forced photometry reference-image weighted average: 14.42 +/- 0.06
Forced photometry filter KEPT candidate at 05:46:42.05 +06:43:48.0: ref_mag=14.42 +/- 0.06 new_mean_mag=12.6059 delta=1.82 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:55:09.31 +02:40:55.9: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.02
Forced photometry filter KEPT candidate at 05:55:09.31 +02:40:55.9: ref_mag=13.23 +/- 0.02 new_mean_mag=12.1685 delta=1.07 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:12:59.35 +02:20:46.5: 12.90 +/- 0.03 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:06:41.00 +05:44:54.1: 12.66 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:12:59.35 +02:20:46.5: 12.89 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.02
Forced photometry filter KEPT candidate at 06:12:59.35 +02:20:46.5: ref_mag=12.89 +/- 0.02 new_mean_mag=11.4800 delta=1.41 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:06:41.00 +05:44:54.1: 12.69 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.67 +/- 0.01
Forced photometry filter KEPT candidate at 06:06:41.00 +05:44:54.1: ref_mag=12.67 +/- 0.01 new_mean_mag=11.6628 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:16:06.45 +06:46:37.5: 12.27 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:17:07.44 +02:34:44.8: 12.20 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:17:07.44 +02:34:44.8: 12.19 +/- 0.01 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:16:06.45 +06:46:37.5: 12.31 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry filter KEPT candidate at 06:17:07.44 +02:34:44.8: ref_mag=12.19 +/- 0.01 new_mean_mag=11.2267 delta=0.97 (need > 0.90)
Forced photometry filter KEPT candidate at 06:16:06.45 +06:46:37.5: ref_mag=12.29 +/- 0.01 new_mean_mag=11.3448 delta=0.94 (need > 0.90)
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:57:29.61 +06:06:56.1: 13.75 +/- 0.04 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:57:29.61 +06:06:56.1: 13.72 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.03
Forced photometry filter KEPT candidate at 05:57:29.61 +06:06:56.1: ref_mag=13.73 +/- 0.03 new_mean_mag=12.6539 delta=1.08 (need > 0.90)
Adding exclusion_list_local.txt__out132306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81101.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 4s
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Considering the candidate 190093_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190093_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:12:06.92 +06:14:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190095_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190095_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:52:13.83 +09:13:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190097_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190097_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:52:20.63 +07:17:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190101_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190101_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:22:12.94 +09:54:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190104_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190104_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190105_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190105_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 190106_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190106_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190108_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190108_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:37:15.41 +08:11:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190109_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190109_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:08:59.69 +02:29:46.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190134_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190134_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:31:30.96 +09:13:03.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 190167_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190167_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:30:04.42 +01:19:40.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 190174_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190174_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:29:09.33 +01:21:26.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 190199_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190199_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190272_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190272_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190315_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190315_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190347_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190347_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:54:55.59 +07:26:01.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 190382_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190382_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:48:01.26 +06:28:46.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190404_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190404_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190410_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190410_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190457_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190457_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190461_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190461_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190472_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190472_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190475_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190475_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190527_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190527_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190578_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190578_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:30:24.51 +04:10:59.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190587_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190587_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190639_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190639_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190669_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190669_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:56:33.22 +11:01:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190677_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190677_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:29:12.63 +00:51:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190710_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190710_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:35:55.99 +09:31:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190727_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190727_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190747_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190747_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190779_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190779_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190795_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190795_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:54:40.12 +00:56:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190816_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190816_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:34:40.76 +05:38:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190826_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190826_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190838_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190838_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:42:19.74 +02:19:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190892_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190892_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 190912_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190912_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:07:10.17 +09:11:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190968_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 190968_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:36:59.98 +09:15:23.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 191032_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 191032_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 191046_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 191046_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
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Considering the candidate 191076_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 191076_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:39:33.35 +09:52:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191083_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 191083_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:54:16.50 +10:33:28.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191099_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 191099_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:37:19.60 +08:11:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191155_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
Preparing report for the candidate 191155_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
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Considering the candidate 132306_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
Preparing report for the candidate 132306_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
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Considering the candidate 111548_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 111548_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:12:45.91 +08:27:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81101_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
Preparing report for the candidate 81101_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
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Considering the candidate 45229_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 45229_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:47:51.54 +04:25:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135524_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 135524_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:18:56.07 +09:18:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23194_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
Preparing report for the candidate 23194_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
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Considering the candidate 155457_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 155457_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:18:03.47 +10:31:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18414_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
Preparing report for the candidate 18414_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
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Considering the candidate 84127_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 84127_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:44:28.85 +06:52:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157497_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 157497_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:26:52.61 +10:23:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64338_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
Preparing report for the candidate 64338_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
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Considering the candidate 108481_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 108481_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:13:52.23 +08:15:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46740_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 46740_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:06:06.70 +04:35:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79997_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
Preparing report for the candidate 79997_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
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Considering the candidate 20875_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
Preparing report for the candidate 20875_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
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Considering the candidate 143663_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 143663_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:02:43.46 +08:42:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102420_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 102420_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:31:56.05 +07:36:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33592_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 33592_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 06:10:44.93 +03:45:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18787_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 18787_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
**** FOUND 05:46:27.36 +02:18:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05061_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475
The candidate 05061_fd_Ori-04-Q1b1x1_2026-08-03_05-57-41_20.00sec_-0.00C_LIGHTs_0475 did not pass the final checks
