This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ
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 10 04.2974 2461317.7974 12.34 06:29:45.82 +13:05:51.1
198.82840 1.23047 galactic Gem Second-epoch detections are separated by 1.0" and 5.8 pix
The object was found in VSX 1" NSVS J0629459+130550
Type: M
# Max. Min./Amp. JD0 Period
17.593 g Y 2.119 g 2458484.53460 343.700000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:29:45.82 +13:05:51.1: 13.22 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:29:45.82 +13:05:51.1: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0629459+130550,2461317.7974,12.34,0.05,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 J0629459+130550 20261004.2974 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.2974 2461317.7974 12.30 06:30:25.99 +09:22:59.5
202.19625 -0.34503 galactic Mon Second-epoch detections are separated by 1.3" and 6.1 pix
The object was found in VSX 5" NSVS J0630261+092255
Type: L:
# Max. Min./Amp. JD0 Period
11.421 R1 Y 0.683 R1 48.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:30:25.99 +09:22:59.5: 13.13 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:30:25.99 +09:22:59.5: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0630261+092255,2461317.7974,12.30,0.05,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 J0630261+092255 20261004.2974 12.30CV 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 10 04.2974 2461317.7974 12.03 06:21:12.30 +12:29:12.7
198.39410 -0.89978 galactic Ori Second-epoch detections are separated by 0.3" and 5.8 pix
The object was found in VSX 0" ASASSN-V J062112.31+122913.1
Type: SR
# Max. Min./Amp. JD0 Period
14.650 g Y 0.230 g 2459115.00600 33.370000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:12.30 +12:29:12.7: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:12.30 +12:29:12.7: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 04.2974* 06 21 12.30 +12 29 12.7 12.0 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 J062112.31+122913.1,2461317.7974,12.03,0.05,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 J062112.31+122913.1 20261004.2974 12.03CV 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 10 04.2974 2461317.7974 11.50 06:41:58.62 +14:42:19.9
198.75506 4.60155 galactic Gem Second-epoch detections are separated by 0.6" and 5.8 pix
The object was found in VSX 2" ASASSN-V J064158.75+144221.1
Type: SR
# Max. Min./Amp. JD0 Period
15.051 g Y 1.376 g 2458603.65900 291.244880400000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:41:58.62 +14:42:19.9: 12.96 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:41:58.62 +14:42:19.9: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J064158.75+144221.1,2461317.7974,11.50,0.05,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 J064158.75+144221.1 20261004.2974 11.50CV 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 10 04.2974 2461317.7974 10.55 06:25:32.13 +13:31:40.0
197.96905 0.51990 galactic Ori Second-epoch detections are separated by 0.8" and 5.9 pix
The object was found in VSX 1" ASAS J062532+1331.7
Type: MISC
# Max. Min./Amp. JD0 Period
11.980 V Y 0.690 V 2452861.90000 105.333360000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:25:32.13 +13:31:40.0: 11.72 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:25:32.13 +13:31:40.0: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.00
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 04.2974* 06 25 32.13 +13 31 40.0 10.6 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 J062532+1331.7,2461317.7974,10.55,0.05,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 J062532+1331.7 20261004.2974 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 04.2974 2461317.7974 12.77 06:34:40.07 +11:17:35.9
200.98264 1.46066 galactic Mon Second-epoch detections are separated by 0.1" and 6.0 pix
The object was found in VSX 1" NSVS 9832822
Type: SR
# Max. Min./Amp. JD0 Period
13.163 r Y 0.543 R1 2451274.24000 80.917154100000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:40.07 +11:17:35.9: 13.91 +/- 0.05 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:40.07 +11:17:35.9: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 9832822,2461317.7974,12.77,0.05,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 9832822 20261004.2974 12.77CV 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 10 04.2974 2461317.7974 12.79 06:24:59.32 +12:21:49.3
198.93611 -0.14165 galactic Ori Second-epoch detections are separated by 1.6" and 5.9 pix
The object was found in VSX 1" ASASSN-V J062459.27+122148.4
Type: SR
# Max. Min./Amp. JD0 Period
14.310 V 14.540 V 2458170.00000 255.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:59.32 +12:21:49.3: 13.82 +/- 0.05 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:59.32 +12:21:49.3: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 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 10 04.2974* 06 24 59.32 +12 21 49.3 12.8 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 J062459.27+122148.4,2461317.7974,12.79,0.05,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 J062459.27+122148.4 20261004.2974 12.79CV 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 10 04.2974 2461317.7974 12.69 06:17:11.11 +11:20:18.1
198.94259 -2.30880 galactic Ori Second-epoch detections are separated by 3.4" and 5.7 pix
The object was found in VSX 1" ASASSN-V J061711.18+112018.1
Type: L:
# Max. Min./Amp. JD0 Period
13.970 V 14.230 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:11.11 +11:20:18.1: 13.80 +/- 0.05 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:11.11 +11:20:18.1: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 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 10 04.2974* 06 17 11.11 +11 20 18.1 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 J061711.18+112018.1,2461317.7974,12.69,0.05,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 J061711.18+112018.1 20261004.2974 12.69CV 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: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
First image: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Last image: 2461317.79772699 04.10.2026 07:08:33.612 /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 7 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): 28151
Objects passed selection criteria: 27997
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: 18120
Average stars matched: 17249.8 (95.1973 %)
Memory usage VmPeak: 253100 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Oct 3 04:56:41 CDT 2026
VaST build number 1.0rc89-231-g50972ca5
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 4 02:12:46 CDT 2026
Host name: tau
############################################################
ERROR: large change in astrometric-star counts between the two new images (q3: 655 -> 506, 22.748% > 20%; fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits vs fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
First image: 2461032.81662337 23.12.2025 07:35:46.259 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Last image: 2461317.79772699 04.10.2026 07:08:33.612 /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 83
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.17
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 46 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): 203627
Objects passed selection criteria: 203006
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: 132092
Average stars matched: 124904 (94.5581 %)
Memory usage VmPeak: 667752 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sat Oct 3 04:56:41 CDT 2026
VaST build number 1.0rc89-231-g50972ca5
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Oct 4 02:14:32 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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
SExtractor catalog cache: saved Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.cat to cache
SExtractor catalog cache: saved Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461317.79715041
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits exists and is non-empty
wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (1st reference image)
verification OK: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Image size: 941.6'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: 06:13:27.287 +13:59:26.52 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-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits (1st new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
Image size: 943.1'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:43.998 +13:59:02.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:43.998 +13:59:02.40
Angular distance between the image centers 0.0679 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits (2nd new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Image size: 943.0'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:43.218 +13:59:34.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:43.218 +13:59:34.84
Angular distance between the image centers 0.0645 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 06:13:43.998 +13:59:02.40
Second-epoch second image center 06:13:43.218 +13:59:34.84
Angular distance between the image centers 0.00955 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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits &> /tmp/tmp.EyJgX2DVwB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.6GmGQBwZkc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits &> /tmp/tmp.DskTZoP5LM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits &> /tmp/tmp.wL2bmHeWM8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Found non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
The reference image (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits) and catalog (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat) found
'wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat' -> 'wcsmag.cat'
Read 31404 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6789 deg, Dec +8.6286 to +19.2777 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 85.0776 to 101.6789 deg, Dec 8.6286 to 19.2777 deg
Loaded 17819 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): 13015 out of 14781 total matches.
Matched with Tycho-2 14781 out of 31404 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.949600
a=0.000000 b=1.000000 c=22.949600
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31404 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6789 deg, Dec +8.6286 to +19.2777 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 85.0776 to 101.6789 deg, Dec 8.6286 to 19.2777 deg
Loaded 17819 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): 13015 out of 14781 total matches.
Matched with Tycho-2 14781 out of 31404 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (aperture=6.1)
Read 31324 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 84.9118 to 101.4962 deg, Dec +8.4421 to +19.3403 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 84.9118 to 101.4962 deg, Dec 8.4421 to 19.3403 deg
Loaded 18085 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): 12980 out of 14663 total matches.
Matched with Tycho-2 14663 out of 31324 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
2.1 pix Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
3.6 pix fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
3.6 pix fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Limiting magnitude estimates:
15.4 mag. Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
15.5 mag. Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
13.2 mag. fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
13.2 mag. fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.EyJgX2DVwB (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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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=3718, bad_region=0, passed=31404
Got 31404 stars (including 27641 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
util/solve_plate_with_UCAC5 got 31404 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4785 matched stars entering correct_measured_positions(), 4786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4785 matched stars entering correct_measured_positions(), 31404 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4848 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 31404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 31404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4783 stars left (next iteration limit 5263)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits N_match=4783 sigma_overall_arcsec=0.380 sigma_q1_arcsec=0.478 sigma_q2_arcsec=0.377 sigma_q3_arcsec=0.342 sigma_q4_arcsec=0.323 n_q1=1170 n_q2=1223 n_q3=1237 n_q4=1153 worst_quadrant_to_overall_ratio=1.257
The image catalog is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -region wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.6GmGQBwZkc (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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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=3619, bad_region=0, passed=31324
Got 31324 stars (including 27657 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat
util/solve_plate_with_UCAC5 got 31324 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 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4850 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4788 matched stars entering correct_measured_positions(), 4788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4788 matched stars entering correct_measured_positions(), 31324 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 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4788 matched stars entering correct_measured_positions(), 31324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4787 matched stars entering correct_measured_positions(), 31324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4787 stars left (next iteration limit 5266)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits N_match=4787 sigma_overall_arcsec=0.407 sigma_q1_arcsec=0.498 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.371 sigma_q4_arcsec=0.355 n_q1=1017 n_q2=1324 n_q3=1130 n_q4=1316 worst_quadrant_to_overall_ratio=1.226
The image catalog is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.DskTZoP5LM (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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.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=245, bad_region=0, passed=5207
Got 5207 stars (including 4955 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat
util/solve_plate_with_UCAC5 got 5207 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.1'
Seting catalog search parameters based on the expected field of view 943.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013099 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010479 (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 491 to 549 (Dec 8.2 to 19.4)
Done reading UCAC5 zone files...
Matched 4780 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4695 matched stars entering correct_measured_positions(), 4671 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4695 matched stars entering correct_measured_positions(), 5174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 491 to 549 (Dec 8.2 to 19.4)
Done reading UCAC5 zone files...
Matched 4780 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4697 matched stars entering correct_measured_positions(), 5173 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 4697 matched stars entering correct_measured_positions(), 5174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 4697 stars left (next iteration limit 5164)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4697 robust_rms=7.381 arcsec worst_region_rms=16.027 arcsec outer_annulus_rms=10.027 arcsec
SIP_REFIT: SIP order 3 trial: matched=4697 robust_rms=0.714 arcsec worst_region_rms=0.967 arcsec outer_annulus_rms=0.967 arcsec
SIP_REFIT: SIP order 5 trial: matched=4697 robust_rms=0.486 arcsec worst_region_rms=0.736 arcsec outer_annulus_rms=0.736 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4697 robust_rms_before=1.124 arcsec robust_rms_before_corrected=0.574 arcsec robust_rms_after=0.486 arcsec worst_region_rms_before=0.861 worst_region_rms_after=0.736 outer_annulus_rms_before=1.367 outer_annulus_rms_after=0.736
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
Image size: 943.3'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:44.039 +13:59:01.33 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5207 stars ###
'wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/correct_sextractor_wcs_catalog_usingxy2sky861734.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.124 -> 0.486 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4697 pairs from the initial matching)
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 491 to 549 (Dec 8.2 to 19.4)
Done reading UCAC5 zone files...
Matched 4411 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4411 pairs (4697 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4411 robust_rms=7.191 arcsec worst_region_rms=15.315 arcsec outer_annulus_rms=8.962 arcsec
SIP_REFIT: SIP order 3 trial: matched=4411 robust_rms=0.701 arcsec worst_region_rms=0.893 arcsec outer_annulus_rms=0.893 arcsec
SIP_REFIT: SIP order 5 trial: matched=4411 robust_rms=0.473 arcsec worst_region_rms=0.720 arcsec outer_annulus_rms=0.720 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4411 robust_rms_before=0.472 arcsec robust_rms_before_corrected=0.472 arcsec robust_rms_after=0.473 arcsec worst_region_rms_before=0.718 worst_region_rms_after=0.720 outer_annulus_rms_before=0.718 outer_annulus_rms_after=0.720
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-region 0.720 vs 0.718 arcsec) - keeping the current solution
SIP_REFIT: the second refit on the re-matched pairs was not applied - keeping the first refit solution
Accuracy estimation diagnostic: 4411 matched stars entering correct_measured_positions(), 5173 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4411 matched stars entering correct_measured_positions(), 5169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits N_match=4411 sigma_overall_arcsec=0.482 sigma_q1_arcsec=0.455 sigma_q2_arcsec=0.522 sigma_q3_arcsec=0.328 sigma_q4_arcsec=0.545 n_q1=687 n_q2=1874 n_q3=655 n_q4=1195 worst_quadrant_to_overall_ratio=1.131
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits -region wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.wL2bmHeWM8 (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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.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=255, bad_region=0, passed=5040
Got 5040 stars (including 4782 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat
util/solve_plate_with_UCAC5 got 5040 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.0'
Seting catalog search parameters based on the expected field of view 943.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013097 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010478 (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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4593 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 4500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4507 matched stars entering correct_measured_positions(), 5030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4593 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4509 matched stars entering correct_measured_positions(), 5030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 4509 matched stars entering correct_measured_positions(), 5030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 4509 stars left (next iteration limit 4957)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4509 robust_rms=7.134 arcsec worst_region_rms=17.046 arcsec outer_annulus_rms=10.904 arcsec
SIP_REFIT: SIP order 3 trial: matched=4509 robust_rms=0.684 arcsec worst_region_rms=1.105 arcsec outer_annulus_rms=1.105 arcsec
SIP_REFIT: SIP order 5 trial: matched=4509 robust_rms=0.474 arcsec worst_region_rms=0.770 arcsec outer_annulus_rms=0.770 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4509 robust_rms_before=1.028 arcsec robust_rms_before_corrected=0.561 arcsec robust_rms_after=0.474 arcsec worst_region_rms_before=0.920 worst_region_rms_after=0.770 outer_annulus_rms_before=1.341 outer_annulus_rms_after=0.770
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Image size: 943.2'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:43.250 +13:59:34.01 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5040 stars ###
'wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/correct_sextractor_wcs_catalog_usingxy2sky861462.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.028 -> 0.474 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (search radius 3.0 arcsec, 4509 pairs from the initial matching)
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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4257 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4257 pairs (4509 from the initial matching)
SIP_REFIT: SIP order 2 trial: matched=4257 robust_rms=6.809 arcsec worst_region_rms=16.638 arcsec outer_annulus_rms=9.749 arcsec
SIP_REFIT: SIP order 3 trial: matched=4257 robust_rms=0.669 arcsec worst_region_rms=1.032 arcsec outer_annulus_rms=1.032 arcsec
SIP_REFIT: SIP order 5 trial: matched=4257 robust_rms=0.463 arcsec worst_region_rms=0.736 arcsec outer_annulus_rms=0.736 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4257 robust_rms_before=0.462 arcsec robust_rms_before_corrected=0.462 arcsec robust_rms_after=0.463 arcsec worst_region_rms_before=0.736 worst_region_rms_after=0.736 outer_annulus_rms_before=0.736 outer_annulus_rms_after=0.736
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Image size: 943.2'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:43.250 +13:59:34.01 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5040 stars ###
'wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/correct_sextractor_wcs_catalog_usingxy2sky904789.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.462 -> 0.463 arcsec)
Accuracy estimation diagnostic: 4257 matched stars entering correct_measured_positions(), 5031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4257 matched stars entering correct_measured_positions(), 5031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits N_match=4257 sigma_overall_arcsec=0.473 sigma_q1_arcsec=0.450 sigma_q2_arcsec=0.513 sigma_q3_arcsec=0.363 sigma_q4_arcsec=0.490 n_q1=824 n_q2=1798 n_q3=506 n_q4=1129 worst_quadrant_to_overall_ratio=1.086
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits -region wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits to local_wcs_cache/
'wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'local_wcs_cache/wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits'
Saving the final (post-refit) wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits'
Saving the final (post-refit) wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits'
Saving the final (post-refit) wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits to local_wcs_cache/
'wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits' -> 'local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits sigma_overall=0.380 worst_q_ratio=1.257
ref2=Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits sigma_overall=0.407 worst_q_ratio=1.226
new1=fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits sigma_overall=0.482 worst_q_ratio=1.131
new2=fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits sigma_overall=0.473 worst_q_ratio=1.086
reference average sigma_overall=0.3935 worst_q_ratio=1.2415
warn-on-ratio threshold: 2.0x reference
###################################
ERROR: large change in astrometric-star counts between the two new images (q3: 655 -> 506, 22.748% > 20%; fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits vs fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386_astrometric_residuals.png (4783 matched stars from wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042_astrometric_residuals.png (4787 matched stars from wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077_astrometric_residuals.png (4411 matched stars from wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078_astrometric_residuals.png (4257 matched stars from wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits'
Saving fully-calibrated image wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits'
Preparing the HTML report for the field Ori-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Ori-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
SExtractor catalog cache: saved Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.cat to cache
SExtractor catalog cache: saved Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Creating symlink local_wcs_cache/wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Checking 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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits exists and is non-empty
wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits exists and is non-empty
wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (1st reference image)
verification OK: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Image size: 941.6'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: 06:13:27.287 +13:59:26.52 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-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits (1st new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
Image size: 943.3'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:44.039 +13:59:01.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:44.039 +13:59:01.33
Angular distance between the image centers 0.0681 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits (2nd new image)
verification OK: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Image size: 943.2'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:13:43.250 +13:59:34.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:13:27.287 +13:59:26.52
Second-epoch image center 06:13:43.250 +13:59:34.01
Angular distance between the image centers 0.0646 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 06:13:44.039 +13:59:01.33
Second-epoch second image center 06:13:43.250 +13:59:34.01
Angular distance between the image centers 0.00962 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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits &> /tmp/tmp.zOjeWc8W41
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.HgRIGtL8cH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits &> /tmp/tmp.sdkdjWkjcY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits &> /tmp/tmp.wA40Trw2Rp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
Found non-empty wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits and wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
The reference image (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits) and catalog (wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat) found
'wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat' -> 'wcsmag.cat'
Read 229058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6828 deg, Dec +8.6174 to +19.2791 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 85.0776 to 101.6828 deg, Dec 8.6174 to 19.2791 deg
Loaded 17847 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): 9852 out of 15551 total matches.
Matched with Tycho-2 15551 out of 229058 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.805100
a=0.000000 b=1.000000 c=22.805100
From vast_summary.log: estimated ref. image limiting mag.: -7.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.64
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.64
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 229058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 85.0776 to 101.6828 deg, Dec +8.6174 to +19.2791 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 85.0776 to 101.6828 deg, Dec 8.6174 to 19.2791 deg
Loaded 17847 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): 9852 out of 15551 total matches.
Matched with Tycho-2 15551 out of 229058 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (aperture=4.6)
Read 230307 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 84.9070 to 101.4968 deg, Dec +8.4421 to +19.3422 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 84.9070 to 101.4968 deg, Dec 8.4421 to 19.3422 deg
Loaded 18095 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): 10167 out of 15481 total matches.
Matched with Tycho-2 15481 out of 230307 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Forced-photometry filter: calibrated wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -> calib.txt_param_ref_wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 72 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
1.9 pix Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
3.2 pix fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
3.2 pix fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Limiting magnitude estimates:
15.6 mag. Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
15.6 mag. Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
13.6 mag. fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
13.5 mag. fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 12.7 (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.zOjeWc8W41 (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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits' -> 'wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.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=66, blended=37651, bad_region=12, passed=228992
Got 228992 stars (including 190970 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat
util/solve_plate_with_UCAC5 got 228992 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4823 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 4773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4772 matched stars entering correct_measured_positions(), 228992 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 228992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 228992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4770 stars left (next iteration limit 5249)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits N_match=4770 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.454 sigma_q2_arcsec=0.379 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.325 n_q1=1096 n_q2=1242 n_q3=1241 n_q4=1191 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits -region wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.HgRIGtL8cH (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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat corresponding to the image wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.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=82, blended=35229, bad_region=4, passed=230225
Got 230225 stars (including 194609 good ones) from the SExtractor catalog wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat
util/solve_plate_with_UCAC5 got 230225 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 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4832 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(), 230225 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 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4831 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 230225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4778 matched stars entering correct_measured_positions(), 230225 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4778 stars left (next iteration limit 5259)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits N_match=4778 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.484 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.356 sigma_q4_arcsec=0.328 n_q1=1035 n_q2=1329 n_q3=1162 n_q4=1252 worst_quadrant_to_overall_ratio=1.248
The image catalog is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.sdkdjWkjcY (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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.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=11, blended=2075, bad_region=14, passed=36388
Got 36388 stars (including 34273 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat
util/solve_plate_with_UCAC5 got 36388 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.3'
Seting catalog search parameters based on the expected field of view 943.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013101 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010481 (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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4811 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4739 matched stars entering correct_measured_positions(), 4713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4739 matched stars entering correct_measured_positions(), 36030 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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4811 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4739 matched stars entering correct_measured_positions(), 36030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4739 matched stars entering correct_measured_positions(), 36022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 4739 stars left (next iteration limit 5212)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4739 robust_rms=7.391 arcsec worst_region_rms=14.703 arcsec outer_annulus_rms=10.665 arcsec
SIP_REFIT: SIP order 3 trial: matched=4739 robust_rms=0.707 arcsec worst_region_rms=0.990 arcsec outer_annulus_rms=0.990 arcsec
SIP_REFIT: SIP order 5 trial: matched=4739 robust_rms=0.485 arcsec worst_region_rms=0.738 arcsec outer_annulus_rms=0.738 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4739 robust_rms_before=0.481 arcsec robust_rms_before_corrected=0.545 arcsec robust_rms_after=0.485 arcsec worst_region_rms_before=0.733 worst_region_rms_after=0.738 outer_annulus_rms_before=0.733 outer_annulus_rms_after=0.738
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.733 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits worst_region_rms_kept=0.733 arcsec robust_rms_kept=0.481 arcsec matched=4739
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits N_match=4739 sigma_overall_arcsec=0.521 sigma_q1_arcsec=0.476 sigma_q2_arcsec=0.595 sigma_q3_arcsec=0.320 sigma_q4_arcsec=0.537 n_q1=764 n_q2=2003 n_q3=744 n_q4=1228 worst_quadrant_to_overall_ratio=1.141
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits -region wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.wA40Trw2Rp (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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
WCS_IMAGE_NAME=wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
WCS-calibrated image found: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Checking if the catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat corresponding to the image wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
WCS catalog name: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.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=10, blended=1970, bad_region=14, passed=35871
Got 35871 stars (including 33856 good ones) from the SExtractor catalog wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat
util/solve_plate_with_UCAC5 got 35871 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.2'
Seting catalog search parameters based on the expected field of view 943.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013100 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010480 (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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4801 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4732 matched stars entering correct_measured_positions(), 4725 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4732 matched stars entering correct_measured_positions(), 35705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4801 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4730 matched stars entering correct_measured_positions(), 35705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4730 matched stars entering correct_measured_positions(), 35705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 4730 stars left (next iteration limit 5205)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4730 robust_rms=6.869 arcsec worst_region_rms=17.139 arcsec outer_annulus_rms=11.220 arcsec
SIP_REFIT: SIP order 3 trial: matched=4730 robust_rms=0.666 arcsec worst_region_rms=1.121 arcsec outer_annulus_rms=1.121 arcsec
SIP_REFIT: SIP order 5 trial: matched=4730 robust_rms=0.473 arcsec worst_region_rms=0.781 arcsec outer_annulus_rms=0.781 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4730 robust_rms_before=0.473 arcsec robust_rms_before_corrected=0.553 arcsec robust_rms_after=0.473 arcsec worst_region_rms_before=0.792 worst_region_rms_after=0.781 outer_annulus_rms_before=0.792 outer_annulus_rms_after=0.781
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.792 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits worst_region_rms_kept=0.792 arcsec robust_rms_kept=0.473 arcsec matched=4730
WCS_QUALITY_DIAG: file=fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits N_match=4730 sigma_overall_arcsec=0.526 sigma_q1_arcsec=0.501 sigma_q2_arcsec=0.584 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.518 n_q1=909 n_q2=1971 n_q3=617 n_q4=1233 worst_quadrant_to_overall_ratio=1.110
The image catalog is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits -region wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-07-43_20.00sec_0.00C_LIGHTs_0077.fits
Saving fully-calibrated image wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.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_2026-10-04_CI_Ori-02-Q1b1x1_021009_TTUQ1b1x1_706552_3GFBUApZ/wcs_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078.fits
Preparing the HTML report for the field Ori-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:54:13.64 +14:24:29.3: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 05:58:18.42 +15:07:32.0: 12.48 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:23:41.95 +09:35:43.1: 12.79 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:09:42.30 +10:10:47.3: 13.13 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:01.21 +11:37:03.6: 12.36 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:09:42.30 +10:10:47.3: 13.13 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:54:13.64 +14:24:29.3: 13.01 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:23:41.95 +09:35:43.1: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry reference-image weighted average: 13.00 +/- 0.02
Forced photometry filter REJECTED candidate at 06:09:42.30 +10:10:47.3: ref_mag=13.13 +/- 0.02 new_mean_mag=12.5810 delta=0.55 (need > 0.90)
Forced photometry reference-image weighted average: 12.78 +/- 0.01
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 05:58:18.42 +15:07:32.0: 12.59 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 05:54:13.64 +14:24:29.3: ref_mag=13.00 +/- 0.02 new_mean_mag=12.9971 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 06:23:41.95 +09:35:43.1: ref_mag=12.78 +/- 0.01 new_mean_mag=11.9687 delta=0.81 (need > 0.90)
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter REJECTED candidate at 05:58:18.42 +15:07:32.0: ref_mag=12.54 +/- 0.01 new_mean_mag=12.5384 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:33.19 +13:00:11.0: 12.61 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:16:10.46 +11:11:54.0: 12.81 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:01.21 +11:37:03.6: 12.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.40 +/- 0.02
Forced photometry filter REJECTED candidate at 06:21:01.21 +11:37:03.6: ref_mag=12.40 +/- 0.02 new_mean_mag=12.1627 delta=0.24 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:33.19 +13:00:11.0: 12.63 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter REJECTED candidate at 06:24:33.19 +13:00:11.0: ref_mag=12.62 +/- 0.01 new_mean_mag=12.4037 delta=0.22 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:16:10.46 +11:11:54.0: 12.84 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.82 +/- 0.02
Forced photometry filter REJECTED candidate at 06:16:10.46 +11:11:54.0: ref_mag=12.82 +/- 0.02 new_mean_mag=12.5779 delta=0.25 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:13:48.90 +11:33:49.0: 13.46 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:13:48.90 +11:33:49.0: 13.38 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry filter REJECTED candidate at 06:13:48.90 +11:33:49.0: ref_mag=13.42 +/- 0.02 new_mean_mag=12.5402 delta=0.88 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:29:45.82 +13:05:51.1: 13.22 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:30:25.99 +09:22:59.5: 13.13 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:21:12.30 +12:29:12.7: 12.98 +/- 0.02 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:41:58.62 +14:42:19.9: 12.96 +/- 0.03 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:29:45.82 +13:05:51.1: 13.49 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter KEPT candidate at 06:29:45.82 +13:05:51.1: ref_mag=13.32 +/- 0.02 new_mean_mag=12.3270 delta=0.99 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:30:25.99 +09:22:59.5: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter KEPT candidate at 06:30:25.99 +09:22:59.5: ref_mag=13.21 +/- 0.02 new_mean_mag=12.3048 delta=0.90 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:21:12.30 +12:29:12.7: 12.88 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.93 +/- 0.01
Forced photometry filter KEPT candidate at 06:21:12.30 +12:29:12.7: ref_mag=12.93 +/- 0.01 new_mean_mag=12.0255 delta=0.90 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:41:58.62 +14:42:19.9: 12.41 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry filter KEPT candidate at 06:41:58.62 +14:42:19.9: ref_mag=12.56 +/- 0.01 new_mean_mag=11.4968 delta=1.07 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:22:01.73 +12:10:28.7: 12.19 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:22:01.73 +12:10:28.7: 12.16 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter REJECTED candidate at 06:22:01.73 +12:10:28.7: ref_mag=12.17 +/- 0.01 new_mean_mag=11.3858 delta=0.79 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:25:32.13 +13:31:40.0: 11.72 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:34:40.07 +11:17:35.9: 13.91 +/- 0.05 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:25:32.13 +13:31:40.0: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.52 +/- 0.00
Forced photometry filter KEPT candidate at 06:25:32.13 +13:31:40.0: ref_mag=11.52 +/- 0.00 new_mean_mag=10.5485 delta=0.97 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:34:40.07 +11:17:35.9: 13.63 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.75 +/- 0.04
Forced photometry filter KEPT candidate at 06:34:40.07 +11:17:35.9: ref_mag=13.75 +/- 0.04 new_mean_mag=12.7701 delta=0.98 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:39:29.71 +11:24:32.2: 10.85 +/- 0.01 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:39:29.71 +11:24:32.2: 10.32 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.46 +/- 0.00
Forced photometry filter REJECTED candidate at 06:39:29.71 +11:24:32.2: ref_mag=10.46 +/- 0.00 new_mean_mag=9.5677 delta=0.90 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:24:59.32 +12:21:49.3: 13.82 +/- 0.05 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2025-12-23_01-35-46_20.00sec_-15.00C_LIGHT_0386.fits at 06:17:11.11 +11:20:18.1: 13.80 +/- 0.05 detection
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:24:59.32 +12:21:49.3: 13.63 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter KEPT candidate at 06:24:59.32 +12:21:49.3: ref_mag=13.71 +/- 0.03 new_mean_mag=12.7920 delta=0.91 (need > 0.90)
Forced photometry on wcs_Ori-02-Q1b1x1_2026-02-11_20-37-12_20.00sec_-14.90C_LIGHT_0042.fits at 06:17:11.11 +11:20:18.1: 13.74 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter KEPT candidate at 06:17:11.11 +11:20:18.1: ref_mag=13.77 +/- 0.03 new_mean_mag=12.6876 delta=1.08 (need > 0.90)
Adding exclusion_list_local.txt__out128306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out215232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96669.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 266161_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266161_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
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Considering the candidate 266168_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266168_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
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Considering the candidate 266172_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266172_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:19:03.46 +10:29:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266173_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266173_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
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Considering the candidate 266179_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266179_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:32:31.40 +11:41:14.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 266180_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266180_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
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Considering the candidate 266218_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266218_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:25:56.00 +08:43:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266224_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266224_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:27:20.17 +08:42:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266454_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266454_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:42:18.88 +17:37:58.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 266461_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266461_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:43:56.12 +13:15:36.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 266468_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266468_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:30:34.08 +13:46:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266600_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266600_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:37:52.93 +16:26:09.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 266629_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266629_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:37:38.38 +16:26:10.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 266772_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266772_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
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Considering the candidate 266802_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266802_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:40:59.20 +09:55:19.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 266948_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266948_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:35:38.35 +09:51:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 266960_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266960_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:28:14.34 +10:19:30.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 266969_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266969_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
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Considering the candidate 266987_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 266987_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:34:42.66 +15:04:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267007_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 267007_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:21:44.11 +12:53:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267047_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 267047_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
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Considering the candidate 267116_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 267116_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:07:50.59 +08:58:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267189_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 267189_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:13:23.03 +10:16:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144640_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 144640_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:24:35.50 +12:44:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137851_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 137851_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:27:24.57 +13:02:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96807_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 96807_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:32:23.87 +14:45:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216934_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 216934_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:36:32.60 +09:25:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150105_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 150105_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:25:56.52 +12:30:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155639_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 155639_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:24:19.45 +12:15:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171471_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 171471_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
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Considering the candidate 190707_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 190707_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:40:36.26 +10:38:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189000_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 189000_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:39:55.79 +10:33:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170626_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 170626_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:34:00.67 +11:33:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203533_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 203533_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
Rejecting candidate due to large distance (34.2") between the two second-epoch detections
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Considering the candidate 107662_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 107662_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:34:05.79 +14:17:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114977_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 114977_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:24:44.22 +14:01:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216984_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 216984_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:39:49.34 +09:29:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243350_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 243350_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:06:07.71 +09:27:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164118_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 164118_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:16:28.00 +11:54:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219420_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 219420_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:17:37.31 +09:37:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166271_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 166271_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
Rejecting candidate due to large distance (34.9") between the two second-epoch detections
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Considering the candidate 136193_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
Preparing report for the candidate 136193_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
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Considering the candidate 215232_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
Preparing report for the candidate 215232_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
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Considering the candidate 165415_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 165415_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:43:16.92 +11:44:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184758_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 184758_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:26:52.71 +10:23:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151105_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
Preparing report for the candidate 151105_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
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Considering the candidate 96669_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
Preparing report for the candidate 96669_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
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Considering the candidate 205235_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 205235_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:15:34.89 +08:57:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209620_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 209620_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:35:42.24 +09:05:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87174_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 87174_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:40:04.90 +15:06:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178081_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 178081_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:14:53.77 +11:15:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192045_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 192045_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:16:00.23 +10:47:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157967_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 157967_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
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Considering the candidate 173160_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 173160_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:21:59.07 +11:28:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165625_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 165625_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:20:20.17 +11:48:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129928_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 129928_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:23:35.67 +13:22:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153706_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 153706_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:29:05.31 +12:19:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102507_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 102507_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:28:57.60 +14:36:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128306_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
Preparing report for the candidate 128306_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
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Considering the candidate 174423_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 174423_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:14:39.10 +11:25:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228618_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 228618_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:20:18.73 +10:06:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175761_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
Preparing report for the candidate 175761_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
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Considering the candidate 144946_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 144946_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:34:47.78 +12:41:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202975_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 202975_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:34:45.85 +08:49:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104176_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 104176_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:32:05.81 +14:31:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148908_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 148908_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:22:48.67 +12:34:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174800_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 174800_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
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Considering the candidate 105146_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 105146_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:35:37.80 +14:23:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153335_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
Preparing report for the candidate 153335_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
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Considering the candidate 176475_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
Preparing report for the candidate 176475_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
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Considering the candidate 176251_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 176251_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
**** FOUND 06:15:58.39 +11:20:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62388_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078
The candidate 62388_fd_Ori-02-Q1b1x1_2026-10-04_02-08-33_20.00sec_-0.00C_LIGHTs_0078 did not pass the final checks
